{"as_of":"2026-08-08T22:24:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:3d252db7fa88fe9b78deca778e594b24b234a3a49e00f1025bbf8bd55691a802","coverage":[{"denominator":175,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T05:29:04.565393Z","state":"measured"},{"denominator":100,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":100,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-08T06:32:00.761636+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2508.01876/citation-record","integrity":"/paper/2508.01876/integrity","json":"/paper/2508.01876/citation-record.json","paper":"/paper/2508.01876"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:53.157245Z","title":"It always exists and it verifies Ωm = 1","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:53.157245Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:500d343904162f47ea58f886e5be9e3205662d08c857943d301fedfc6edbf684","observation_id":"bbe4805f-04dd-46cb-83ec-3d4034a24746","resolution":{"observed_at":"2026-08-06T05:28:53.157245Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:52.943209Z","title":"Moreover, the evo- lution equation for H, given by the Raychaudhuri equation, decouples","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:52.943209Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:fe489d356f506d1cf43cbdb1523cd9529997e50ddaec1a525d51116fe8f354b9","observation_id":"0f0bfad3-4fbe-443e-a839-1460bbab57a5","resolution":{"observed_at":"2026-08-06T05:28:52.943209Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:53.021987Z","title":"This means that for each of the interactions (26)-(34), we obtain a different dynamical system when the corresponding values of α, β, δare substituted into (41)-(44)","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:53.021987Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:28a73c197f27ee3af7c92abed909b1e47e4538db507b748cc36d1cd385c3e8f3","observation_id":"d27d423d-70c3-44db-af8f-3cfaef2b2837","resolution":{"observed_at":"2026-08-06T05:28:53.021987Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:53.373021Z","title":"They always exist and both represent an anisotropic Bianchi I vacuum solution","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:53.373021Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:e143562d23b3863b3a0345caa2d96167dd852eb68f697734e3f26deadf8d2616","observation_id":"c69d9e15-d7d9-423c-b4ef-10b62fbc0d59","resolution":{"observed_at":"2026-08-06T05:28:53.373021Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:53.505128Z","title":"It always exists and we verify that Ωm = 1","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:53.505128Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:d19d821378eaf3050298df26718149288f9d5b61034b608d64d0aa6112d42812","observation_id":"ceff70db-13be-4efa-ad3d-cb403b31d9a8","resolution":{"observed_at":"2026-08-06T05:28:53.505128Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:53.564309Z","title":"It always exists It always exists and represents a scalar field dominated flat FLRW solution","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:53.564309Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:e3ca99cd41a0621d471ea45a12e723b3b34f280c48988919d4cd0974dd7a8a87","observation_id":"17d8f258-c022-4d14-acc4-653bf22bf63c","resolution":{"observed_at":"2026-08-06T05:28:53.564309Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:53.693851Z","title":"These points are anisotropic vacuum Bianchi I solutions","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:53.693851Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:dca7bcdd8b99cc66ab47b407b1ed2b466a39707b17200b6370716ef5c81cb03c","observation_id":"cb1a2da9-e85f-4c38-94a0-c200720f46b3","resolution":{"observed_at":"2026-08-06T05:28:53.693851Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:53.877539Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:53.877539Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:ebb9e0f5df3c0da134aef3f72923bbb276284f9afade24b87c1b4d690a2ef4e5","observation_id":"2fd23616-9c08-47af-890d-9395b7d564a1","resolution":{"observed_at":"2026-08-06T05:28:53.877539Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:54.120578Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:54.120578Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:663e311c6b92c4348ff1a8fd136b14f74bb723941cedefad68cc9ae885ded65a","observation_id":"c7574c75-8f3e-4b74-aad5-c851f8369cce","resolution":{"observed_at":"2026-08-06T05:28:54.120578Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:54.229783Z","title":"It always exists and is i) sink for 0 ≤ γ <2, ¯Γ < −3(γ − 1), ii) saddle for 0 ≤ γ <2, ¯Γ > −3(γ − 1), iii) non-hyperbolic for ¯Γ = −3(γ − 1) or γ = 2","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:54.229783Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:8db7ec7c1204711c3b44f50fadc0e91ed73a120a6ad93c22cd8e7ae54dac0da7","observation_id":"d4d3c655-3b96-4219-b7f7-e32ef8d633a7","resolution":{"observed_at":"2026-08-06T05:28:54.229783Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:54.345725Z","title":"They always exist and are i) sources for 0 ≤ γ <2, ¯Γ > −3, ii) saddles for 0 ≤ γ <2, ¯Γ < −3, iii) non-hyperbolic for ¯Γ = −3 or γ = 2","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:54.345725Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:18061bc048fd6594c38dafe0826c8567d74e7859ba551be51fcadc2eed7a85b2","observation_id":"5e7627bd-7d31-4bf7-a358-4a8056caa84b","resolution":{"observed_at":"2026-08-06T05:28:54.345725Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:54.440326Z","title":"This point verifies Ωm = ¯Γ 3−3γ","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:54.440326Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:10034af5331ca86326a5fc6ed34144f00a585762d3a38b20edd2a78725ef6ff9","observation_id":"5d93c7f0-e6fa-45e1-9a73-270c088a8ec0","resolution":{"observed_at":"2026-08-06T05:28:54.440326Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:54.530875Z","title":"They belong to the singular line ¯Ω = 0 and are non-hyperbolic","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:54.530875Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:b5e8957cd303734acb25cbf526d8e9c821e80ef23113a6cdb2d1a22d53d832f3","observation_id":"6c53ea7f-66c8-422e-a063-a1e76b08ff0a","resolution":{"observed_at":"2026-08-06T05:28:54.530875Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:54.695435Z","title":"It has Ωm = 1 6 3 − √ 9γ+12¯Γ−9√γ−1 and it exists exists for 0 ≤ γ < 1, 0 ≤ ¯Γ ≤ 1 4 (3 − 3γ) or 1 < γ ≤ 2, 1 4 (3 − 3γ) ≤ ¯Γ ≤ 0","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:54.695435Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:70434fd2d6a3358b2382eebbe3cd0add7a8c8e7518eeb71248fa809973d23a6a","observation_id":"569f7a54-fbf8-44bb-a85f-4eb08e812876","resolution":{"observed_at":"2026-08-06T05:28:54.695435Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:54.836656Z","title":"It has Ωm = 1 6 √ 9γ+12¯Γ−9√γ−1 + 3 , it exists for 0 ≤ γ <1, 0 ≤ ¯Γ ≤ 1 4 (3 − 3γ) or 1 < γ≤ 2, 1 4 (3 − 3γ) ≤ ¯Γ ≤ 0","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:54.836656Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:e7d638135d7f7eb9a6323d0da95eefc6aad83aeffcc8886bff0dc1049261095a","observation_id":"15021203-a64b-4ee0-93e0-03e49b799b55","resolution":{"observed_at":"2026-08-06T05:28:54.836656Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:55.185877Z","title":"It exist for i) m <0, 1 ≤ γ ≤ 2 or ii) m = 0, 0 ≤ γ <1 or iii) m = 0, 1 < γ≤ 2 or iv) m >0, 0 ≤ γ ≤ 1","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:55.185877Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:f4e41e4573261e658f249629134cb1e3336c76fef6b34c5b914094b657acaf8c","observation_id":"1febb70f-54ab-457f-b2e2-192e95ee4350","resolution":{"observed_at":"2026-08-06T05:28:55.185877Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:55.322147Z","title":"It always exists and it verifies Ωm = 1","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:55.322147Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:2a44415edaf1872e08d4966315a7e33258c3112d3683a004336c4926072a498c","observation_id":"faf948dd-0a20-47bb-81cf-dfdfa7ab668e","resolution":{"observed_at":"2026-08-06T05:28:55.322147Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:55.434760Z","title":"It always exists and represents a scalar field domi- nated solution","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:55.434760Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:da8a223d73d87105b9156c21b116c7fe0004c34ce235ec67276dc7ff231e4667","observation_id":"a7a8824b-c5f7-4972-852d-c20c9b2537f6","resolution":{"observed_at":"2026-08-06T05:28:55.434760Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:55.529735Z","title":"They always exist and both represent an anisotropic Bianchi I vacuum solution","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:55.529735Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:cf2452e575d4c8ba66b7293f473db1f712910948ee4209744db624110ada16c0","observation_id":"92b78682-21dd-448c-8a9c-fb09c5712cb9","resolution":{"observed_at":"2026-08-06T05:28:55.529735Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:55.666926Z","title":"The points M1,2 = ± q γ+m−1 m , q 2−γ m only exist for γ = 2 and m ≤ −1","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:55.666926Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:5a7a1e9dadd3550440ba8f5285ef7eeb72861f66adcfb442511b7a0f79df949e","observation_id":"b0cc5ceb-0dd1-481b-a0ca-275609739635","resolution":{"observed_at":"2026-08-06T05:28:55.666926Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:55.806591Z","title":"It always exists and it verifies Ωm = 1","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:55.806591Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:2312750a3395f72242dd1f9f65c549dd20cc7685716ea7c19e054145543a1caa","observation_id":"19bfce06-b7b0-491d-92a7-6167d321b81a","resolution":{"observed_at":"2026-08-06T05:28:55.806591Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:55.918089Z","title":"It always exists and represents a scalar field dominated flat FLRW solution","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:55.918089Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:7dee94b7ca71d806e926fe133ef0a162b3c867f830bdde0a078d0a5d31155d94","observation_id":"4cc1f344-5ffa-41b8-b16c-765174650bcc","resolution":{"observed_at":"2026-08-06T05:28:55.918089Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:56.017276Z","title":"They always exist and both represent an anisotropic Bianchi I vacuum solution","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:56.017276Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:aea092d75cc602a3b00424f43a0c39890de3c972a7f8f5eca497b0db6f088e20","observation_id":"1aa9afa9-9ee9-4286-8a37-38fe10985e82","resolution":{"observed_at":"2026-08-06T05:28:56.017276Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:56.125085Z","title":"It always exists and it verifies Ωm = 1","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:56.125085Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:16c68afc5478b534e7d062375ed3e9a8915145d58a256c3053820c15bf4f059e","observation_id":"dfaaf535-19e9-4c4e-9bcf-381e97382e60","resolution":{"observed_at":"2026-08-06T05:28:56.125085Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:56.250036Z","title":"It always exists and represents a scalar field domi- nated solution","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:56.250036Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:26e126e0c652873a16e040bf32f528d0c0a4d78e823a8f66afab39eb37cb9e82","observation_id":"94d98d12-682d-4600-b4f7-0194dabe8204","resolution":{"observed_at":"2026-08-06T05:28:56.250036Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:56.372120Z","title":"They always exist, to study their stability we substitute ¯Ω = 0 in the Jacobian matrix and then take the limit as Σ → ±1","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:56.372120Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:27dbd2e5472eb216797c89ee9787a7f61c6f12f6e1e7faa47a714fb486fc6bd4","observation_id":"9c27d056-4742-45ef-8027-87f8b9611651","resolution":{"observed_at":"2026-08-06T05:28:56.372120Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:56.464263Z","title":"The point exists for m > 0, 0 ≤ γ ≤ 1 or m <0, 1 ≤ γ ≤ 2 and is a i) sink for 0 ≤ γ <1, −γ2+2γ−1 γ−2 < m <1 − γ or 1 < γ≤ 2, m <1 − γ, ii) saddle for i","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:56.464263Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:faa3810463ff2e7673236302927b9ea1fdb7c804921a84a271fcb8e39c8088e2","observation_id":"a8a4f835-a764-4340-8102-425ec6eabafe","resolution":{"observed_at":"2026-08-06T05:28:56.464263Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:56.559720Z","title":"The definition of the deceleration parameter q is as follows q := −1 − ˙H(t) H 2(t)","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:56.559720Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:33123ab78704b7b51b0c80b81fe4995471efd73e13e2b6fe32547f1b30d3ef35","observation_id":"a28aa2bd-7f61-4eb4-8e11-b0b0a0174476","resolution":{"observed_at":"2026-08-06T05:28:56.559720Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:56.669302Z","title":"It describes acceleration for 0 ≤ γ < 2 3","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:56.669302Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:a6b9babaa61454be2fa4b6b97585789a65cdfca4f00bc91f0bce349686621082","observation_id":"d911cb4d-b969-4f1d-9d18-2309939772de","resolution":{"observed_at":"2026-08-06T05:28:56.669302Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:56.796286Z","title":"(152) In Figure 21 we see that qseries oscillates between deceleration and acceleration","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:56.796286Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:75ae24b21fe376fefb65c004be3f06bd0487f25d6dfbafee0336eab67f1768a4","observation_id":"22b565f9-2502-4c37-8b20-89df724d3021","resolution":{"observed_at":"2026-08-06T05:28:56.796286Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:56.944474Z","title":"The Hubble function is H(t) = 1 3t","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:56.944474Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:b5080f72ce737bba5a8c04c986b9a23600178158bd53bdbe252435e3a616ae79","observation_id":"90c6175b-f741-4bbc-88b2-c619d7c54988","resolution":{"observed_at":"2026-08-06T05:28:56.944474Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:57.054861Z","title":"(154) We focus on qaveraged, it describes acceleration for ¯Γ < 2 − 3γ","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:57.054861Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:b62751c9d73dac798bafe6aa7ca123607d81548160ae784d7fbc5ff1ee6e4ae7","observation_id":"047ef38a-c392-4cfd-9d20-9a83f108331d","resolution":{"observed_at":"2026-08-06T05:28:57.054861Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:57.194255Z","title":"(157) We focus on qaveraged, it describes acceleration for ¯Γ > 1","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:57.194255Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:b837bc17e4a98bcb99440802181db726f73b2564a8fe1b3ab3a6e7557de34a7e","observation_id":"d262e8ae-a1eb-4887-aab6-0e95054705ed","resolution":{"observed_at":"2026-08-06T05:28:57.194255Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:57.347983Z","title":"(160) We focus on qaveraged","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:57.347983Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:ce05a393367a587370ecb980a6aa192de18e00f9fa19e904ea5197d5a3ba5c5e","observation_id":"9319a71c-ab33-4e63-93ca-56f1fde7f0cd","resolution":{"observed_at":"2026-08-06T05:28:57.347983Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:57.443566Z","title":"(163) We focus on qaveraged","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:57.443566Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:e7f02f84b72391f9d545002fe7b4935a2d04f16afc0827cc37e3848da550e26b","observation_id":"f089a3c6-bd84-4e78-8a67-314273062a3d","resolution":{"observed_at":"2026-08-06T05:28:57.443566Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:57.595384Z","title":"(166) We focus on qaveraged","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:57.595384Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:d807919bf657a3eba75352a8862acdca8300bed435065ade9595bbb196ecad93","observation_id":"b56c694b-5157-4ef5-9681-b7ab2a31ae18","resolution":{"observed_at":"2026-08-06T05:28:57.595384Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:57.694596Z","title":"They describe acceleration for 0 ≤ γ <2, 1 4 (3γ − 6) < m <0","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:57.694596Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:10f665c78348e3434488a22a1e92dc4231f888e0c6a7f1869901061a66e22b0c","observation_id":"0d787b85-6c9d-46f7-be6d-b352b0f39d22","resolution":{"observed_at":"2026-08-06T05:28:57.694596Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:57.804613Z","title":"(170) We focus on qaveraged","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:57.804613Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:5a0022af6dad4227f393e0a9a70e92b139267e0797390bfa644d1698c97661b3","observation_id":"ad282bc8-ceda-4a53-9dad-75e2e09ba8bc","resolution":{"observed_at":"2026-08-06T05:28:57.804613Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:57.942319Z","title":"StiffnessSwitching","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:57.942319Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:3dc83806e37ae425927d5b93dbdaa9becce8fe96cfcffde81e9db084cbb7f570","observation_id":"f33e4322-773f-4e5f-9a58-11d79b8e4296","resolution":{"observed_at":"2026-08-06T05:28:57.942319Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:28:58.053913Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:58.053913Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:14569bb360567c94e1e128c8b1c2881d1dc36b8776ba9710ee51b6c67f7b9392","observation_id":"e9cbdcd6-0b1d-4505-8cd4-481cdddcefa6","resolution":{"observed_at":"2026-08-06T05:28:58.053913Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9908023","last_updated":"1999-08-03T16:13:46Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"1999-08-03T16:13:46Z","title":"Coupled Quintessence","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9908023","snapshot_observed_at":"2026-08-06T05:28:58.190611Z","title":"Amendola, Phys","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:58.190611Z"},"links":{"cited_paper":"/paper/astro-ph/9908023","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:4ea44dea54173826072df21c86a2a0bfafae8646dc001b00bccd2f3dcfb3a7e0","observation_id":"cf75b553-7d4b-400d-a89f-ea827c09468c","resolution":{"observed_at":"2026-08-06T05:28:58.190611Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1109.6234","last_updated":"2012-01-23T11:32:10Z","snapshot_observed_at":"2026-08-07T07:45:13.815697Z","submitted_at":"2011-09-28T15:07:34Z","title":"Interacting Dark Energy -- constraints and degeneracies","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1109.6234","snapshot_observed_at":"2026-08-06T05:28:58.303008Z","title":"Clemson, K","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:58.303008Z"},"links":{"cited_paper":"/paper/1109.6234","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:198f27eb5b5846929e7c3de45579e3069641aa12e88042a516c8656a450ba45b","observation_id":"51debe04-2cb7-424d-9b01-375b0d21c1df","resolution":{"observed_at":"2026-08-06T05:28:58.303008Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0607126","last_updated":"2007-05-02T12:34:15Z","snapshot_observed_at":"2026-07-07T01:01:32.905306Z","submitted_at":"2006-07-07T07:09:32Z","title":"Interacting Dark Energy and Dark Matter: observational Constraints from Cosmological Parameters","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0607126","snapshot_observed_at":"2026-08-06T05:28:58.432430Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:58.432430Z"},"links":{"cited_paper":"/paper/astro-ph/0607126","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:2035aa69eefae24230dbab39f277311dc21f85083337f0690f9dd8b73b2cb686","observation_id":"f008bf31-4357-4599-b64e-cd2ea16b74a8","resolution":{"observed_at":"2026-08-06T05:28:58.432430Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0411025","last_updated":"2005-01-08T00:55:32Z","snapshot_observed_at":"2026-07-07T04:52:20.024398Z","submitted_at":"2004-11-02T01:46:29Z","title":"Cosmology with Interaction between Phantom Dark Energy and Dark Matter and the Coincidence Problem","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0411025","snapshot_observed_at":"2026-08-06T05:28:58.555246Z","title":"Cai and A","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:58.555246Z"},"links":{"cited_paper":"/paper/hep-th/0411025","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:14941450050de8502af6f8ba9867a81ab89ca2ca25e542f3cffd7c5c52ba6717","observation_id":"f1a8856e-1a4d-4e5a-9574-971e3d2d806c","resolution":{"observed_at":"2026-08-06T05:28:58.555246Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.15726","last_updated":"2024-05-24T17:17:28Z","snapshot_observed_at":"2026-07-06T18:19:29.996982Z","submitted_at":"2024-05-24T17:17:28Z","title":"Interaction in the dark sector: a phenomenological approach","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.15726","snapshot_observed_at":"2026-08-06T05:28:58.700236Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:58.700236Z"},"links":{"cited_paper":"/paper/2405.15726","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:a92e340aa9fccbe40d0e3a80fcff329cd2e57a5d26d1c873963c3ccf58608391","observation_id":"abaa536d-339f-462b-8cc1-b210a39df918","resolution":{"observed_at":"2026-08-06T05:28:58.700236Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.05348","last_updated":"2024-11-22T06:51:35Z","snapshot_observed_at":"2026-08-02T20:04:38.113537Z","submitted_at":"2024-09-09T06:06:17Z","title":"Compartmentalization and Coexistence in the Dark Sector of the Universe","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.05348","snapshot_observed_at":"2026-08-06T05:28:58.843017Z","title":"Paliathanasis, K","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:58.843017Z"},"links":{"cited_paper":"/paper/2409.05348","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:5a0b5e9000b1ee3bc780f4c5877e7dc73e4e9ed9f9b4e68fdd90b40f3d547cc4","observation_id":"9233e1d4-bf8e-4fc9-a5b8-09078f837af2","resolution":{"observed_at":"2026-08-06T05:28:58.843017Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2210.01184","last_updated":"2022-10-03T18:54:50Z","snapshot_observed_at":"2026-08-05T08:47:21.630757Z","submitted_at":"2022-10-03T18:54:50Z","title":"Perturbations in the interacting vacuum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2210.01184","snapshot_observed_at":"2026-08-06T05:28:58.962927Z","title":"Munyeshyaka, J","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:58.962927Z"},"links":{"cited_paper":"/paper/2210.01184","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:479b7aead1faa4d3469c640e96418d1dc30d87b7d86922b37844a9d95ee05028","observation_id":"31b76dfb-70dd-4052-a68a-f9ea45e37c50","resolution":{"observed_at":"2026-08-06T05:28:58.962927Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.07213","last_updated":"2019-08-20T08:18:47Z","snapshot_observed_at":"2026-08-07T16:47:53.602777Z","submitted_at":"2019-08-20T08:18:47Z","title":"Looking for interactions in the cosmological dark sector","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.07213","snapshot_observed_at":"2026-08-06T05:28:59.024926Z","title":"Benetti, W","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:59.024926Z"},"links":{"cited_paper":"/paper/1908.07213","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:4e7788d8f291e0df67ed1beba249508de03a993e63859073c55b01812d082c0b","observation_id":"ecae731f-ac48-4d97-a39b-f78fd8de2d54","resolution":{"observed_at":"2026-08-06T05:28:59.024926Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1304.3829","last_updated":"2013-04-13T18:13:22Z","snapshot_observed_at":"2026-07-06T03:11:05.752009Z","submitted_at":"2013-04-13T18:13:22Z","title":"Modeling dark energy through an Ising fluid with network interactions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1304.3829","snapshot_observed_at":"2026-08-06T05:28:59.128323Z","title":"Luongo and D","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:59.128323Z"},"links":{"cited_paper":"/paper/1304.3829","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:5558e3bb82f5a0af76632b4a6faf20ff9377574524eeb1e0ab5c6dc7dd6cb4c7","observation_id":"f045838d-eedd-4ebf-ab59-7f2e3bc90bd1","resolution":{"observed_at":"2026-08-06T05:28:59.128323Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.01669","last_updated":"2025-08-04T13:56:55Z","snapshot_observed_at":"2026-08-01T19:48:28.599955Z","submitted_at":"2025-04-02T12:17:19Z","title":"The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.01669","snapshot_observed_at":"2026-08-06T05:28:59.273736Z","title":"Di Valentino et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:59.273736Z"},"links":{"cited_paper":"/paper/2504.01669","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:13e75f3d0c4b846e379118d6269896f62521db1de4936972dcfd14999649278b","observation_id":"11cc10ab-63a0-48a9-987b-dbf713bf8d17","resolution":{"observed_at":"2026-08-06T05:28:59.273736Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.06142","last_updated":"2022-04-24T16:57:09Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2022-03-11T18:13:52Z","title":"Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.06142","snapshot_observed_at":"2026-08-06T05:28:59.388019Z","title":"Abdalla et al., JHEAp 34, 49 (2022), 2203.06142","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:59.388019Z"},"links":{"cited_paper":"/paper/2203.06142","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:b24f7aed47c8047f0ba0458b34dd20c60aa05c70e930f46c19f1ff8f246c97c6","observation_id":"a8b43846-c1d1-4154-bccb-58792836b042","resolution":{"observed_at":"2026-08-06T05:28:59.388019Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1809.03224","last_updated":"2019-07-17T16:31:05Z","snapshot_observed_at":"2026-08-08T19:46:33.120486Z","submitted_at":"2018-09-10T09:59:32Z","title":"Testing a quintessence model with Yukawa interaction from cosmological observations and N-body simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1809.03224","snapshot_observed_at":"2026-08-06T05:28:59.482509Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:59.482509Z"},"links":{"cited_paper":"/paper/1809.03224","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:4fb0db2565248e33dc43b83ad718d1413bfedd599aa9f181138e0bafe2e8b918","observation_id":"fd5022d4-6bc8-43cb-aee1-afd18c8f0813","resolution":{"observed_at":"2026-08-06T05:28:59.482509Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.00610","last_updated":"2020-06-06T09:47:22Z","snapshot_observed_at":"2026-07-06T09:09:13.177340Z","submitted_at":"2020-04-01T17:51:17Z","title":"Update on Coupled Dark Energy and the $H_0$ tension","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.00610","snapshot_observed_at":"2026-08-06T05:28:59.585298Z","title":"Gómez-Valent, V","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:59.585298Z"},"links":{"cited_paper":"/paper/2004.00610","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:383bf5a2b3fa1bd983b78792ba9de31973bf219560eb8c0ff960d57ec4bc5c62","observation_id":"bd750522-5d90-4622-ba07-ff800e44466e","resolution":{"observed_at":"2026-08-06T05:28:59.585298Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0311175","last_updated":"2003-11-27T11:25:01Z","snapshot_observed_at":"2026-07-07T00:38:05.919368Z","submitted_at":"2003-11-07T12:27:19Z","title":"Linear and non-linear perturbations in dark energy models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0311175","snapshot_observed_at":"2026-08-06T05:28:59.710092Z","title":"Amendola, Phys","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:59.710092Z"},"links":{"cited_paper":"/paper/astro-ph/0311175","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:9aefd2c8f7afc34f2a0312f8fd2faf1c70874c523a50952b8c27837ec989b117","observation_id":"ec6d6515-d8ac-413d-83e9-d2f6128065cd","resolution":{"observed_at":"2026-08-06T05:28:59.710092Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.04281","last_updated":"2020-07-01T09:13:30Z","snapshot_observed_at":"2026-07-06T08:13:55.544875Z","submitted_at":"2019-08-12T17:48:35Z","title":"Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.04281","snapshot_observed_at":"2026-08-06T05:28:59.809102Z","title":"Di Valentino, A","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:59.809102Z"},"links":{"cited_paper":"/paper/1908.04281","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:33b42cffc52199f9f9d391ffb6e7295b91fb3800a8c9fce048b7163929f3f194","observation_id":"e55833c5-6aa5-474b-b9de-c8428cad290c","resolution":{"observed_at":"2026-08-06T05:28:59.809102Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.04865","last_updated":"2019-07-14T11:54:15Z","snapshot_observed_at":"2026-07-06T07:38:41.728739Z","submitted_at":"2019-03-12T12:21:21Z","title":"Dark sector interaction: a remedy of the tensions between CMB and LSS data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.04865","snapshot_observed_at":"2026-08-06T05:28:59.934875Z","title":"Kumar, R","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-06T05:28:59.934875Z"},"links":{"cited_paper":"/paper/1903.04865","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:ba90b61867db8155ba73fd8b4b19420b67ffd492b24550e36b24f82ee02b2d1a","observation_id":"58c72245-faca-4465-b5f9-fac0bfd6a421","resolution":{"observed_at":"2026-08-06T05:28:59.934875Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:29:00.025374Z","title":"Carloni, O","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:00.025374Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:13f6b9847450cdeb7bcedd1663a13e51c6f181352c342b495bfb5ef8a1ba97b7","observation_id":"9ad79361-2de8-4cc8-a0ce-d16892c77657","resolution":{"observed_at":"2026-08-06T05:29:00.025374Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.10436","last_updated":"2019-09-27T20:26:44Z","snapshot_observed_at":"2026-07-06T07:47:51.328297Z","submitted_at":"2019-04-23T17:31:43Z","title":"Observational constraints of a new unified dark fluid and the $H_0$ tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.10436","snapshot_observed_at":"2026-08-06T05:29:00.143128Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:00.143128Z"},"links":{"cited_paper":"/paper/1904.10436","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:0769452ca3082d075b61e908bf130aa00385ee41a6437e94467e829175f51b59","observation_id":"7dfb7f55-4276-4fc6-a73b-b85d1d88b83f","resolution":{"observed_at":"2026-08-06T05:29:00.143128Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.15196","last_updated":"2021-09-24T08:00:03Z","snapshot_observed_at":"2026-07-06T11:24:06.451781Z","submitted_at":"2021-06-29T09:30:48Z","title":"Multi-interacting dark energy and its cosmological implications","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.15196","snapshot_observed_at":"2026-08-06T05:29:00.246942Z","title":"Lucca, Phys","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:00.246942Z"},"links":{"cited_paper":"/paper/2106.15196","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:0cd7f472ad731e148bb3c74737e7eefce64cd2615cac8b59b7da195c2be8e2cb","observation_id":"16d76090-1bf2-406f-a86a-5bed88c92fe5","resolution":{"observed_at":"2026-08-06T05:29:00.246942Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.02536","last_updated":"2021-12-20T06:24:24Z","snapshot_observed_at":"2026-07-06T11:54:50.811616Z","submitted_at":"2021-10-06T06:58:58Z","title":"Exploration of interacting dynamical dark energy model with interaction term including the equation-of-state parameter: alleviation of the $H_{0}$ tension","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.02536","snapshot_observed_at":"2026-08-06T05:29:00.381382Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:00.381382Z"},"links":{"cited_paper":"/paper/2110.02536","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:3693c9411fff43709020b6931c04a881ae98a02579a284db0204596bb43f32df","observation_id":"05d301e8-2778-4d08-b7bd-e35c1161a0ea","resolution":{"observed_at":"2026-08-06T05:29:00.381382Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.04200","last_updated":"2023-02-11T20:04:17Z","snapshot_observed_at":"2026-08-05T02:28:29.071939Z","submitted_at":"2023-01-10T20:32:05Z","title":"Smoothing the $H_0$ tension with a dynamical dark energy model","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.04200","snapshot_observed_at":"2026-08-06T05:29:00.517706Z","title":"Dahmani, A","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:00.517706Z"},"links":{"cited_paper":"/paper/2301.04200","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:a96193ecc7fbc40d428baf5761850c0f9eb9e17c3be50daa2ae80a486583c58e","observation_id":"9f538751-3a3f-4993-92e9-24e970e519bb","resolution":{"observed_at":"2026-08-06T05:29:00.517706Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.10714","last_updated":"2021-05-26T07:56:37Z","snapshot_observed_at":"2026-08-07T02:01:29.693961Z","submitted_at":"2021-01-26T11:20:45Z","title":"Relieving the $H_0$ tension with a new interacting dark energy model","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.10714","snapshot_observed_at":"2026-08-06T05:29:00.615033Z","title":"Gao, Z.-W","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:00.615033Z"},"links":{"cited_paper":"/paper/2101.10714","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:09969eb631a33f280d4cddbe46c05902c7fc1ffedd7f8096d418ff331d1a3bd3","observation_id":"45c7aab6-34b4-40f6-97d9-9e8bfe4edd28","resolution":{"observed_at":"2026-08-06T05:29:00.615033Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.08743","last_updated":"2023-03-30T18:35:09Z","snapshot_observed_at":"2026-07-06T14:43:16.371886Z","submitted_at":"2023-01-19T21:19:03Z","title":"Cosmological implications of an interacting model of dark matter \\& dark energy","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.08743","snapshot_observed_at":"2026-08-06T05:29:00.732394Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:00.732394Z"},"links":{"cited_paper":"/paper/2301.08743","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:51b1498f17e4d47d476f23eeef085358fae7b56f9d43a658198249539340db2e","observation_id":"aeaabf5e-4cc9-45ed-9afc-49ec2bd7ff6d","resolution":{"observed_at":"2026-08-06T05:29:00.732394Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.11949","last_updated":"2024-01-20T04:14:46Z","snapshot_observed_at":"2026-07-06T14:55:00.475642Z","submitted_at":"2023-02-23T11:49:27Z","title":"Interacting dark energy: clarifying the cosmological implications and viability conditions","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.11949","snapshot_observed_at":"2026-08-06T05:29:00.850445Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:00.850445Z"},"links":{"cited_paper":"/paper/2302.11949","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:f634aa352166d270ba93d22666d265db02934948f6029e17ab37c02594fd52ff","observation_id":"e9cfe380-33ab-49a3-a4a4-7de3139219d1","resolution":{"observed_at":"2026-08-06T05:29:00.850445Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.03152","last_updated":"2022-07-19T21:49:28Z","snapshot_observed_at":"2026-07-06T12:05:39.208452Z","submitted_at":"2021-11-04T20:45:18Z","title":"Late time interacting cosmologies and the Hubble constant tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.03152","snapshot_observed_at":"2026-08-06T05:29:00.993497Z","title":"Gariazzo, E","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:00.993497Z"},"links":{"cited_paper":"/paper/2111.03152","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:8ba48006e422cd4f8b6adcfcc4ae3ee9dd38c95ab6e40c54546ae6fb18ec3316","observation_id":"b7992508-e649-43f5-95ad-1a9c25bb5495","resolution":{"observed_at":"2026-08-06T05:29:00.993497Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.13354","last_updated":"2024-05-22T05:16:39Z","snapshot_observed_at":"2026-07-06T18:17:42.417326Z","submitted_at":"2024-05-22T05:16:39Z","title":"Some Classes of Interacting Two-Fluid Model of the Expanding Universe","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.13354","snapshot_observed_at":"2026-08-06T05:29:01.100292Z","title":"Bhattacharya, Phys","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:01.100292Z"},"links":{"cited_paper":"/paper/2405.13354","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:438852efe9e8b1cb9fdd56e699d6be3c28b554ac1cc399c9cd5e1072ee6f327b","observation_id":"62724885-5ac0-4d85-a97d-ecd48a95b30c","resolution":{"observed_at":"2026-08-06T05:29:01.100292Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.06396","last_updated":"2024-12-22T10:57:21Z","snapshot_observed_at":"2026-08-06T01:12:50.754766Z","submitted_at":"2024-04-09T15:39:16Z","title":"Reconciling $S_8$: Insights from Interacting Dark Sectors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.06396","snapshot_observed_at":"2026-08-06T05:29:01.205976Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:01.205976Z"},"links":{"cited_paper":"/paper/2404.06396","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:c22d37964f6868e0f50e1e0ff38b86599daf36184b2a206f54b85bf54ba8b815","observation_id":"43c14924-a39b-4618-8515-39dec55cbcb3","resolution":{"observed_at":"2026-08-06T05:29:01.205976Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.06097","last_updated":"2023-06-01T13:25:22Z","snapshot_observed_at":"2026-08-07T23:06:57.980757Z","submitted_at":"2023-01-15T13:39:02Z","title":"Exploring the $H_0$ tension and the evidence of dark sector interaction from 2D BAO measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.06097","snapshot_observed_at":"2026-08-06T05:29:01.353564Z","title":"Bernui, E","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:01.353564Z"},"links":{"cited_paper":"/paper/2301.06097","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:f12743d9b116fa589ad159e4e9ae967a6198b00902a43bb546ad475131351ca8","observation_id":"c3d0989d-07b8-4c2b-bab8-8c1158ab1214","resolution":{"observed_at":"2026-08-06T05:29:01.353564Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1901.02540","last_updated":"2019-06-14T03:03:30Z","snapshot_observed_at":"2026-08-05T23:54:29.994904Z","submitted_at":"2019-01-08T22:31:30Z","title":"J-PAS: forecasts on interacting dark energy from baryon acoustic oscillations and redshift-space distortions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1901.02540","snapshot_observed_at":"2026-08-06T05:29:01.485032Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:01.485032Z"},"links":{"cited_paper":"/paper/1901.02540","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:5703d66532028d89067a79a3f2b37296e5657b2a2c65f55fe2048d0e419a3bdd","observation_id":"423bccd1-a2ce-4d53-9178-17d6c2db99be","resolution":{"observed_at":"2026-08-06T05:29:01.485032Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.07167","last_updated":"2022-12-05T14:53:23Z","snapshot_observed_at":"2026-07-06T13:52:32.151640Z","submitted_at":"2022-09-15T09:37:15Z","title":"Forecast Analysis on Interacting Dark Energy Models from Future Generation PICO and DESI Missions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.07167","snapshot_observed_at":"2026-08-06T05:29:01.623476Z","title":"Joseph and R","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:01.623476Z"},"links":{"cited_paper":"/paper/2209.07167","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:5f4c72e11e0860a5bd3af50d560d2e7bfd2fb33e3a21fd4a2a9608fd165be337","observation_id":"aa3ae12b-23aa-4234-a764-a901733074a9","resolution":{"observed_at":"2026-08-06T05:29:01.623476Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.01383","last_updated":"2023-09-06T13:38:24Z","snapshot_observed_at":"2026-08-05T05:57:32.174323Z","submitted_at":"2023-05-02T12:59:06Z","title":"Extended Analysis of Neutrino-Dark Matter Interactions with Small-Scale CMB Experiments","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.01383","snapshot_observed_at":"2026-08-06T05:29:01.709828Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:01.709828Z"},"links":{"cited_paper":"/paper/2305.01383","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:6a0dbb3d3f3c88bd0028e9d5602e708cdceb19abb132fafaa6285f1325c4d102","observation_id":"f3b3fd0d-bb88-4a50-9257-47f957da1471","resolution":{"observed_at":"2026-08-06T05:29:01.709828Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:29:01.813045Z","title":"Chakraborty, T","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:01.813045Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:3832846051e11e7aba70d0487d6d2fdb510f050bbb0ac8b6fa307060021f0903","observation_id":"fc3aca07-458b-4ab9-b88f-3bd85bd62173","resolution":{"observed_at":"2026-08-06T05:29:01.813045Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-07T16:10:37.036129Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-06T05:29:01.892565Z","title":"Giarè, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:01.892565Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:97499625085325b642e39883ce3e75511cde504c13731263af2e5f7ceac82a2f","observation_id":"c006d971-c973-4e23-8da8-16efbc43dd5a","resolution":{"observed_at":"2026-08-06T05:29:01.892565Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15977","last_updated":"2025-02-21T10:00:55Z","snapshot_observed_at":"2026-07-06T18:05:03.284784Z","submitted_at":"2024-04-24T16:52:15Z","title":"Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15977","snapshot_observed_at":"2026-08-06T05:29:02.010016Z","title":"Montani, N","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:02.010016Z"},"links":{"cited_paper":"/paper/2404.15977","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:2e6e63c6e1c3efdea390df1ff3b90436a47bf11d2c2139342ce457cc38e5522c","observation_id":"ad815fa9-5887-4f99-88a4-7e868a3072d5","resolution":{"observed_at":"2026-08-06T05:29:02.010016Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.14934","last_updated":"2024-11-12T01:42:43Z","snapshot_observed_at":"2026-08-06T12:07:52.318618Z","submitted_at":"2024-07-20T16:52:17Z","title":"Constraints on Interacting Dark Energy Models from the DESI Baryon Acoustic Oscillation and DES Supernovae Data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.14934","snapshot_observed_at":"2026-08-06T05:29:02.139269Z","title":"Li, P.-J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:02.139269Z"},"links":{"cited_paper":"/paper/2407.14934","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:3801ed11085b3d0c59e7efda39fd1efd872573215e6bfac4829b5b3e799c5268","observation_id":"f63b7d5f-0ea4-4499-8e69-90d2faa0a0f4","resolution":{"observed_at":"2026-08-06T05:29:02.139269Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.12403","last_updated":"2024-12-04T13:32:05Z","snapshot_observed_at":"2026-08-04T04:55:14.714524Z","submitted_at":"2024-08-22T13:49:22Z","title":"Quantifying the $S_8$ tension and evidence for interacting dark energy from redshift-space distortion measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.12403","snapshot_observed_at":"2026-08-06T05:29:02.243918Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:02.243918Z"},"links":{"cited_paper":"/paper/2408.12403","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:958e0afd4dc1d3c79efcdd924a6033664baba4a9c28d7f1ee98e453fa07f8227","observation_id":"ebf91d30-c1de-4bc1-94b0-174b788fd3ac","resolution":{"observed_at":"2026-08-06T05:29:02.243918Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.16299","last_updated":"2025-04-18T20:54:20Z","snapshot_observed_at":"2026-07-06T20:11:15.503499Z","submitted_at":"2024-12-20T19:17:28Z","title":"Interacting dark sector with quadratic coupling: theoretical and observational viability","version":4},"cited_work":{"arxiv_id":"2412.16299","doi":null,"metadata_source":"pith","pith_arxiv_id":"2412.16299","snapshot_observed_at":"2026-08-06T05:29:18.359970Z","title":"Interacting dark sector with quadratic coupling: theoretical and observational viability","venue":"astro-ph.CO","work_id":"d17b1967-1412-4733-80b5-cc2adbb0d263","year":2024},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:02.328275Z"},"links":{"cited_paper":"/paper/2412.16299","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:38b0af00a8e71734dd1c446c91cb7d00b0b07abc6f41fb4b03717313b8c8b50a","observation_id":"7e5b8f9e-86dd-40fb-946c-f4b0b4d330bc","resolution":{"observed_at":"2026-08-06T05:29:18.500205Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.17792","last_updated":"2025-03-08T08:41:48Z","snapshot_observed_at":"2026-08-07T17:51:28.316068Z","submitted_at":"2025-02-25T02:50:16Z","title":"Cosmological constraints on two vacuum decay models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.17792","snapshot_observed_at":"2026-08-06T05:29:02.425542Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:02.425542Z"},"links":{"cited_paper":"/paper/2502.17792","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:17952f196afa4f1afcbb41efc69da9aa11298303aae1749488540aa910ed9160","observation_id":"aded0440-68fd-450c-93dd-53e0db2340a8","resolution":{"observed_at":"2026-08-06T05:29:02.425542Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.21652","last_updated":"2025-09-08T07:08:45Z","snapshot_observed_at":"2026-08-07T16:32:22.960010Z","submitted_at":"2025-03-27T16:16:43Z","title":"Interacting Dark Sectors in light of DESI DR2","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.21652","snapshot_observed_at":"2026-08-06T05:29:02.523163Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:02.523163Z"},"links":{"cited_paper":"/paper/2503.21652","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:a347810cdb40f47bb44c457f7283869d4441e8b3da13f8c78a316d10296781d0","observation_id":"4b74d059-6719-472e-a3e2-5fd4147f6f0b","resolution":{"observed_at":"2026-08-06T05:29:02.523163Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.23225","last_updated":"2025-06-11T18:36:13Z","snapshot_observed_at":"2026-08-07T16:28:07.594746Z","submitted_at":"2025-03-29T21:11:16Z","title":"New constraints on interacting dark energy from DESI DR2 BAO observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.23225","snapshot_observed_at":"2026-08-06T05:29:02.632978Z","title":"Silva, M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:02.632978Z"},"links":{"cited_paper":"/paper/2503.23225","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:6f1dac7d13e3fa132c4f17d16afa1adb3c243e9bd1715c5399aaab7893fdf79f","observation_id":"45e27586-f073-4249-b29b-81386e38c0ff","resolution":{"observed_at":"2026-08-06T05:29:02.632978Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.00985","last_updated":"2025-08-02T04:31:49Z","snapshot_observed_at":"2026-08-07T16:16:52.536563Z","submitted_at":"2025-04-01T17:21:09Z","title":"Dynamical Dark Energy Implies a Coupled Dark Sector: Insights from DESI DR2 via a Data-Driven Approach","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.00985","snapshot_observed_at":"2026-08-06T05:29:02.744198Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:02.744198Z"},"links":{"cited_paper":"/paper/2504.00985","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:735eab1e84ec9bec09c0b7eddc9a174b245605c0043b063f16070ead72ab9d9e","observation_id":"6bc727ac-65dd-4a4d-87ca-837f73e41eae","resolution":{"observed_at":"2026-08-06T05:29:02.744198Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.09879","last_updated":"2025-05-29T02:04:48Z","snapshot_observed_at":"2026-08-07T15:45:15.410148Z","submitted_at":"2025-05-15T00:50:34Z","title":"New cosmological constraints on the evolution of dark matter energy density","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.09879","snapshot_observed_at":"2026-08-06T05:29:02.797751Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:02.797751Z"},"links":{"cited_paper":"/paper/2505.09879","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:7293612e52aebdd5ed2c41c07246aae94b92619330a9996d815354f9f7bae5d5","observation_id":"f14da499-3227-489d-9dfa-e76c99adcadd","resolution":{"observed_at":"2026-08-06T05:29:02.797751Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:29:02.844907Z","title":"van der Westhuizen, D","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:02.844907Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:4492bd2be5c8ba3d6fb1fdfb5d33649c51bce4c8d22d6e8298d1e70b3ae39610","observation_id":"b00d8804-5541-4a8c-89e4-dff5962c6cf4","resolution":{"observed_at":"2026-08-06T05:29:02.844907Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2506.21295","last_updated":"2025-06-26T14:14:57Z","snapshot_observed_at":"2026-08-06T22:25:05.483948Z","submitted_at":"2025-06-26T14:14:57Z","title":"Constraint on Momentum-coupled Dark Energy using DESI DR2","version":1},"cited_work":{"arxiv_id":"2506.21295","doi":null,"metadata_source":"pith","pith_arxiv_id":"2506.21295","snapshot_observed_at":"2026-08-06T05:29:17.812649Z","title":"Constraint on Momentum-coupled Dark Energy using DESI DR2","venue":"astro-ph.CO","work_id":"93037892-b52b-4536-84bb-b2f5609d196e","year":2025},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:02.937354Z"},"links":{"cited_paper":"/paper/2506.21295","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:bf67489593c51f28d8fec270445975155828b365e00dd3007c36eab5f605b315","observation_id":"34075756-de46-4ef4-bc00-0111981fb50f","resolution":{"observed_at":"2026-08-06T05:29:17.908374Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:29:03.066621Z","title":"Paliathanasis (2025), 2503.20896","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:03.066621Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:b6fc6c4bcf13d38b30eb9c6204c4d8dd973c9d4d705baa6fffa787cbcb464855","observation_id":"48c9aa2c-7286-4026-953e-dbdbeec21ecb","resolution":{"observed_at":"2026-08-06T05:29:03.066621Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2506.16223","last_updated":"2025-06-19T11:28:24Z","snapshot_observed_at":"2026-08-07T14:20:22.884968Z","submitted_at":"2025-06-19T11:28:24Z","title":"Observational Constraints on Scalar Field--Matter Interaction in Weyl Integrable Spacetime","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2506.16223","snapshot_observed_at":"2026-08-06T05:29:03.143295Z","title":"Paliathanasis (2025), 2506.16223","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:03.143295Z"},"links":{"cited_paper":"/paper/2506.16223","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:67a81c8538f6d8b963d4981abe71b95a4af74e244228fd30a1b5c41f73eae6b5","observation_id":"7f9c33e9-24db-46c3-a5e0-928625377506","resolution":{"observed_at":"2026-08-06T05:29:03.143295Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:29:03.212372Z","title":"Li and X","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:03.212372Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:f42b931e9f434f0029a10ebbc8b3efa00a3162e73669a3b0cfc4e68721561184","observation_id":"c11ccf52-bf0a-4381-bc2c-a412225403f2","resolution":{"observed_at":"2026-08-06T05:29:03.212372Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T05:29:03.380691Z","title":null,"venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:03.380691Z"},"links":{"citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:62268d4426780615114d39d0db0898113424203848060da0709568672cc163ae","observation_id":"7f86fe27-65bb-4651-94db-e2241c6e0652","resolution":{"observed_at":"2026-08-06T05:29:03.380691Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1201.1469","last_updated":"2012-01-06T18:32:54Z","snapshot_observed_at":"2026-07-06T02:40:30.614166Z","submitted_at":"2012-01-06T18:32:54Z","title":"General Relativity and Weyl Geometry","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1201.1469","snapshot_observed_at":"2026-08-06T05:29:03.460981Z","title":"Romero, J","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:03.460981Z"},"links":{"cited_paper":"/paper/1201.1469","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:bec2949937df6f840c50b98527a131a89281d093a2b0562c4e2338ed9923de7e","observation_id":"921d20a7-401d-4b85-8833-a113aa100c5b","resolution":{"observed_at":"2026-08-06T05:29:03.460981Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.06639","last_updated":"2022-06-14T06:59:59Z","snapshot_observed_at":"2026-08-05T07:19:29.265450Z","submitted_at":"2022-06-14T06:59:59Z","title":"Interacting dark energy in curved FLRW spacetime from Weyl Integrable Spacetime","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.06639","snapshot_observed_at":"2026-08-06T05:29:03.524844Z","title":"Chatzidakis, A","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:03.524844Z"},"links":{"cited_paper":"/paper/2206.06639","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:9740be3d20bcc1c071cac3504f3f9c5b4ee244df6acce1548d56e464cd593d3d","observation_id":"3977328a-11ee-4480-b7f2-6cd85377c841","resolution":{"observed_at":"2026-08-06T05:29:03.524844Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9406030","last_updated":"1994-06-17T19:24:16Z","snapshot_observed_at":"2026-07-07T03:24:45.763672Z","submitted_at":"1994-06-17T19:24:16Z","title":"Integrable Weyl Geometry in Multidimensional Cosmology. Numerical Investigation","version":1},"cited_work":{"arxiv_id":"gr-qc/9406030","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/9406030","snapshot_observed_at":"2026-08-06T05:29:17.172536Z","title":"Integrable Weyl Geometry in Multidimensional Cosmology. Numerical Investigation","venue":"gr-qc","work_id":"39dd5014-5b0a-4246-b596-069cd6552209","year":1994},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:03.624735Z"},"links":{"cited_paper":"/paper/gr-qc/9406030","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:e8ce9b4271fdc82ad621e6bea3164ff49134a930ed175304614f4f89f6e4a54b","observation_id":"c2997d30-2d25-43b5-abaf-0494948e03b3","resolution":{"observed_at":"2026-08-06T05:29:17.265153Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.19437","last_updated":"2024-07-19T14:51:47Z","snapshot_observed_at":"2026-08-02T02:33:19.507291Z","submitted_at":"2024-04-30T10:35:04Z","title":"Quintom cosmology and modified gravity after DESI 2024","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.19437","snapshot_observed_at":"2026-08-06T05:29:03.744635Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:03.744635Z"},"links":{"cited_paper":"/paper/2404.19437","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:b5f2393c462341540cb82d08fa8e42ce2cdc6cc011a6029621040fcfab6b43c3","observation_id":"262d45e9-b62f-463c-835f-d64bee91d03d","resolution":{"observed_at":"2026-08-06T05:29:03.744635Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0609039","last_updated":"2007-03-23T12:26:27Z","snapshot_observed_at":"2026-08-03T21:11:31.654526Z","submitted_at":"2006-09-12T09:58:51Z","title":"Cosmic Duality in Quintom Universe","version":5},"cited_work":{"arxiv_id":"gr-qc/0609039","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/0609039","snapshot_observed_at":"2026-08-06T05:29:16.903419Z","title":"Cosmic Duality in Quintom Universe","venue":"gr-qc","work_id":"4ccd14f4-eea5-4d7c-8e24-738f21493b10","year":2006},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:03.831794Z"},"links":{"cited_paper":"/paper/gr-qc/0609039","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:5cbd060094ac8f113c307d9acef9327d29f1cb61363843c696699f2e0cebc232","observation_id":"f4de0fae-fd6c-43c6-90f0-21f1812246a2","resolution":{"observed_at":"2026-08-06T05:29:16.999452Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2504.07791","last_updated":"2025-04-18T11:42:39Z","snapshot_observed_at":"2026-08-07T16:06:50.260852Z","submitted_at":"2025-04-10T14:27:03Z","title":"Quantum Gravity Meets DESI: Dynamical Dark Energy in Light of the Trans-Planckian Censorship Conjecture","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.07791","snapshot_observed_at":"2026-08-06T05:29:03.928886Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:03.928886Z"},"links":{"cited_paper":"/paper/2504.07791","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:0057fba2cf8462da43b7212d894881318d9a474d562f601791cf0a4382c86cfd","observation_id":"b60a7e3d-7bf8-4996-a9f2-6d9a074baaea","resolution":{"observed_at":"2026-08-06T05:29:03.928886Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.06784","last_updated":"2025-08-12T13:06:49Z","snapshot_observed_at":"2026-08-07T16:07:13.474763Z","submitted_at":"2025-04-09T11:17:20Z","title":"Modified gravity realizations of quintom dark energy after DESI DR2","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.06784","snapshot_observed_at":"2026-08-06T05:29:04.039842Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:04.039842Z"},"links":{"cited_paper":"/paper/2504.06784","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:1b3996a3d109aec700ed3ef1565425a337d64b9805b563bc57b6adda49c8db31","observation_id":"11dd371a-7793-4d12-a71f-9bc6da59ea55","resolution":{"observed_at":"2026-08-06T05:29:04.039842Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.19864","last_updated":"2025-06-12T06:48:04Z","snapshot_observed_at":"2026-08-07T16:37:43.386131Z","submitted_at":"2025-03-25T17:31:53Z","title":"Equivalence of $f(Q)$ cosmology with quintom-like scenario: the phantom field as effective realization of the non-trivial connection","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.19864","snapshot_observed_at":"2026-08-06T05:29:04.134717Z","title":"Basilakos, A","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:04.134717Z"},"links":{"cited_paper":"/paper/2503.19864","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:518dc084a5797b6f9d084801f7805751fe1e9d879c7179ffb284600cebc5864d","observation_id":"663285bd-341d-4e22-900c-eeea17a85783","resolution":{"observed_at":"2026-08-06T05:29:04.134717Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0909.2776","last_updated":"2010-04-22T15:03:24Z","snapshot_observed_at":"2026-08-08T19:33:35.491944Z","submitted_at":"2009-09-15T11:39:10Z","title":"Quintom Cosmology: Theoretical implications and observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0909.2776","snapshot_observed_at":"2026-08-06T05:29:04.222183Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":101,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:04.222183Z"},"links":{"cited_paper":"/paper/0909.2776","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:ccaf4184d56e26f3fb00b7021b080e692914b654e05a7b253d4a3fad7601ae44","observation_id":"f9eacbba-b0bb-42be-86c4-90ad711424a4","resolution":{"observed_at":"2026-08-06T05:29:04.222183Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.06538","last_updated":"2022-11-18T03:06:52Z","snapshot_observed_at":"2026-08-06T11:55:52.508769Z","submitted_at":"2022-04-13T17:32:11Z","title":"The dynamics of scalar-field Quintom cosmological models","version":2},"cited_work":{"arxiv_id":"2204.06538","doi":null,"metadata_source":"pith","pith_arxiv_id":"2204.06538","snapshot_observed_at":"2026-08-06T05:29:16.600401Z","title":"The dynamics of scalar-field Quintom cosmological models","venue":"gr-qc","work_id":"bb3da32c-5c75-479f-889a-61b401d80d59","year":2022},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":102,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:04.331977Z"},"links":{"cited_paper":"/paper/2204.06538","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:dbd6a3289f3c9d37af8c66842d8fd57e0c5f93922f53c6f9d674716f79e9ee63","observation_id":"698ebfb2-0b6d-4e1b-853c-c8482fc7c14f","resolution":{"observed_at":"2026-08-06T05:29:16.714485Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1808.05634","last_updated":"2018-09-21T16:59:05Z","snapshot_observed_at":"2026-07-06T06:56:02.159474Z","submitted_at":"2018-08-16T18:26:01Z","title":"The past and future dynamics of quintom dark energy models","version":2},"cited_work":{"arxiv_id":"1808.05634","doi":null,"metadata_source":"pith","pith_arxiv_id":"1808.05634","snapshot_observed_at":"2026-08-06T05:29:16.382905Z","title":"The past and future dynamics of quintom dark energy models","venue":"gr-qc","work_id":"eb2447c6-c911-4e75-ae94-d331f968ae71","year":2018},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":103,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:04.473356Z"},"links":{"cited_paper":"/paper/1808.05634","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:88d8bd24f9c32924e6333a8f188f050788776c6f702d1d307c118e6dc9bd69ed","observation_id":"a611b045-058b-4894-a691-5999c4018646","resolution":{"observed_at":"2026-08-06T05:29:16.478734Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1208.0061","last_updated":"2013-02-25T23:30:10Z","snapshot_observed_at":"2026-07-06T02:52:56.435184Z","submitted_at":"2012-08-01T00:59:45Z","title":"Quintom phase-space: beyond the exponential potential","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1208.0061","snapshot_observed_at":"2026-08-06T05:29:04.565393Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":104,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:04.565393Z"},"links":{"cited_paper":"/paper/1208.0061","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:e2f4bd0420bfa457ab659b9a8770025688a4758563a2801afff76218b405e6aa","observation_id":"2297601f-7323-467e-9bbc-16d17a772ff3","resolution":{"observed_at":"2026-08-06T05:29:04.565393Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-08T09:31:49.383907Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":94,"verified_exact":6,"verified_fuzzy":0},"total_outbound_references":175},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"thesis":"As of 8 August 2026, this Paper Citation Record lists 100 of 175 outbound references and 0 inbound Pith citation observations for arXiv:2508.01876."}