{"as_of":"2026-08-16T19:53:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:60c76748bf065641d5b2e3ddfe97ef357bbe8e473ead104ea66bbb15fc73068c","coverage":[{"denominator":102,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T14:14:38.267487Z","state":"measured"},{"denominator":101,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":101,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-03T11:41:15.280154Z","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":[{"citation":{"cited_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.03657","snapshot_observed_at":"2026-08-03T11:41:15.280154Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2601.05646","last_updated":"2026-06-25T07:04:53Z","snapshot_observed_at":"2026-08-03T11:41:11.085957Z","submitted_at":"2026-01-09T09:06:09Z","title":"A microphysically inspired approach to dark matter-dark energy interactions: first bounds on dark-sector scattering cross sections","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-03T11:41:15.280154Z"},"links":{"cited_paper":"/paper/1908.03657","citing_paper":"/paper/2601.05646"},"observation_digest":"sha256:e24a4972cf52bd72bc354bb64d89e3447541e1568d5278573d975b066fa4557e","observation_id":"8fe6c2e6-c373-488b-997a-0ea3cc9d9fb8","resolution":{"observed_at":"2026-08-03T11:41:15.280154Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1908.03657/citation-record","integrity":"/paper/1908.03657/integrity","json":"/paper/1908.03657/citation-record.json","paper":"/paper/1908.03657"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:37.899465Z","title":null,"venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:37.899465Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:15685235ef67ba83f4d046ed43042df04d12bbb6aaca53e75c5d3212a1811f17","observation_id":"12df8a2f-4e89-4ed2-982f-afc1c6cb61c7","resolution":{"observed_at":"2026-08-14T14:14:37.899465Z","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":"2026-08-14T14:14:37.904006Z","title":"Perlmutter et al","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:37.904006Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:662bba6fbddf51db0c81427a1ccf55db78b543808cc3c1a2c046247bd22f0d38","observation_id":"688e3d88-4a40-459b-baa6-973bd7b08487","resolution":{"observed_at":"2026-08-14T14:14:37.904006Z","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":"2026-08-14T14:14:37.908184Z","title":"Aghanim et al","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:37.908184Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:e9f09d80239509bb7347be6fa3a4b823290d934feb55ab04c1d7c5149a821a96","observation_id":"d5c54126-70e6-440b-aad8-be6e3daf21a3","resolution":{"observed_at":"2026-08-14T14:14:37.908184Z","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":"2026-08-14T14:14:37.912605Z","title":null,"venue":null,"work_id":null,"year":1988},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:37.912605Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:ab87e947d6a796fe3873eb6ffe834a06b0b81deaee4231bf101fd9c0cdb3cdd7","observation_id":"bf3ac84d-55f2-4f34-9e4b-2c3c64f02eb3","resolution":{"observed_at":"2026-08-14T14:14:37.912605Z","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":"2026-08-14T14:14:37.916955Z","title":"Ratra and P","venue":null,"work_id":null,"year":1988},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:37.916955Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:fa0cd4e1a038ce9fdf257c755f894d29768fdc32c25f296a00d9d3359fa203c2","observation_id":"3d7e149e-1c74-4b35-8525-f58fc63ef662","resolution":{"observed_at":"2026-08-14T14:14:37.916955Z","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":"2026-08-14T14:14:37.920891Z","title":null,"venue":null,"work_id":null,"year":1992},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:37.920891Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:00b07d53c1e01b321a5de831ac4fddd4320c805cba016f0c9a58bbc0e3ce8316","observation_id":"f8fa2fc6-6145-4d0f-ad1d-b8c015c6451f","resolution":{"observed_at":"2026-08-14T14:14:37.920891Z","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":"2026-08-14T14:14:37.925296Z","title":null,"venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:37.925296Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:1d9715fbc9fa2ec282bb19c3da7b556ddee94bfdab48ccdefae9b897f0942e47","observation_id":"1b5ddb43-d490-4c18-bb0c-0d22ac448321","resolution":{"observed_at":"2026-08-14T14:14:37.925296Z","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":"2026-08-14T14:14:37.929024Z","title":null,"venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:37.929024Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:a51ad0a4471702d79874acb3f878f3261923f56c7d2dc23ee1b76252c301fe29","observation_id":"c898460d-338d-49ef-a1b1-7b42ce7496e3","resolution":{"observed_at":"2026-08-14T14:14:37.929024Z","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":"2026-08-14T14:14:37.932799Z","title":"Padmanabhan","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:37.932799Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:f142578cc491f70bedd0b61cb876565a895761936c4271b2fa38c742770108d2","observation_id":"528ff95d-10fc-480f-86e5-d9e35779fa07","resolution":{"observed_at":"2026-08-14T14:14:37.932799Z","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":"2026-08-14T14:14:37.936299Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:37.936299Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:dacf611154c7759a156b200e338632aa671a1357cbb4e65579ecd1cb9129712d","observation_id":"621b89e9-8edf-4364-a076-67870ae1e9e7","resolution":{"observed_at":"2026-08-14T14:14:37.936299Z","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":"2026-08-14T14:14:37.939898Z","title":"Armendariz-Picon, V","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:37.939898Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:c85e1fbba1370230fe52db05a57074972e97d1ab0fcac212689aa7f76a2fb9d3","observation_id":"3a7e8737-0562-40f4-8942-f142444d1ce7","resolution":{"observed_at":"2026-08-14T14:14:37.939898Z","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":"2026-08-14T14:14:37.943685Z","title":"Brax and J","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:37.943685Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:5843f11f76cb91c589c46c0626bf4264be0a2eb17802c4f96989cc3c7d8349d0","observation_id":"e68f4fee-b69a-4c35-82b0-762ae8fb4069","resolution":{"observed_at":"2026-08-14T14:14:37.943685Z","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":"2026-08-14T14:14:37.947510Z","title":null,"venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:37.947510Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:7053ffaf9ba40541970610d63a1d926106ecce283dc4b83257916da05d65d489","observation_id":"ed16514e-1159-448a-aacb-9d98ae71b568","resolution":{"observed_at":"2026-08-14T14:14:37.947510Z","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":"2026-08-14T14:14:37.951060Z","title":"Vagnozzi, S","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:37.951060Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:4a46c306ff56136cb7cce2f04b78f4d2b4e976bb74acc35846e601409897e6d5","observation_id":"caed891c-ce8e-4bef-b319-c8b75853b8c5","resolution":{"observed_at":"2026-08-14T14:14:37.951060Z","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":"2026-08-14T14:14:37.954728Z","title":"Koivisto and D","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:37.954728Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:18a8bc12e6bf07d075b2d6c2ea7f5e63a41b54928d88d1aae25e4a2f0a9203db","observation_id":"d22e48e3-e195-409c-9c11-37a3f4ae0658","resolution":{"observed_at":"2026-08-14T14:14:37.954728Z","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":"2026-08-14T14:14:37.958280Z","title":"Bamba and S","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:37.958280Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:9397bd3d6435d0fd51d92a4f741f177ddca6d90ba3951fe1cec0dbaf21227be7","observation_id":"61ac0e03-ac9f-413d-b6c9-3cb15179590c","resolution":{"observed_at":"2026-08-14T14:14:37.958280Z","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":"2026-08-14T14:14:37.962018Z","title":"Emelyanov and F","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:37.962018Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:65879eed72b8e8fdb0d2a83c63515907dcb15869b5bafecccafbd0a2a005afc6","observation_id":"54d677db-1a91-4cc5-aaca-fe6c90330d2c","resolution":{"observed_at":"2026-08-14T14:14:37.962018Z","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":"2026-08-14T14:14:37.965572Z","title":"Emelyanov and F","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:37.965572Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:8b57b2635475649b97f7c28c3c4cfaf46e505357fc3dc2d251a00e2f6459f446","observation_id":"05368a96-20f2-4aa7-ae67-9eba91497b52","resolution":{"observed_at":"2026-08-14T14:14:37.965572Z","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":"2026-08-14T14:14:37.969237Z","title":"Emelyanov and F","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:37.969237Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:5cbd19a60d1caf72ff212386407aff1401ac72bdf17d473d2ab3ff34754aef1c","observation_id":"50acf4aa-ff32-4d23-b119-55f6f5696118","resolution":{"observed_at":"2026-08-14T14:14:37.969237Z","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":"2026-08-14T14:14:37.972668Z","title":"Kouwn, P","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:37.972668Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:6d296250beb669fc119c4369e98fe0fa8e310cff632eea683c2a33d406767ee1","observation_id":"4cc9b5e9-5b36-4d30-a231-9a44f5d6f86a","resolution":{"observed_at":"2026-08-14T14:14:37.972668Z","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":"2026-08-14T14:14:37.976676Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:37.976676Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:688f3c94a36290d76863d7a67ca038634cc3cb3895d4aa8202ad768435b09c5a","observation_id":"0d73fa7f-8877-454f-b41f-fd98af786a0a","resolution":{"observed_at":"2026-08-14T14:14:37.976676Z","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":"2026-08-14T14:14:37.980288Z","title":null,"venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:37.980288Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:06901a99bd870ee763f45b26b6ab031241468a5dcf9c4cfd428b8074d5a349a8","observation_id":"278ac2bf-15bb-4d1c-b3b5-dc11d7b06091","resolution":{"observed_at":"2026-08-14T14:14:37.980288Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:39.349228Z","title":null,"venue":null,"work_id":"bc61652c-69b6-4eef-9946-83603ecb276d","year":2004},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:37.983731Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:d0e8387e1fcdd06a331ea87518b290c8728eeb3d0af0c6d299b22982aea46470","observation_id":"7b7f6ea4-fd2c-4180-ac26-293877351524","resolution":{"observed_at":"2026-08-14T14:14:39.353099Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:39.336314Z","title":"Pavon and W","venue":null,"work_id":"c8e183b9-d70b-450d-affb-5856987a1da6","year":2005},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:37.987318Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:586223b8ab1667ec6ae630ebaddc81baa0cdba18e02bbd8beef6885c2f656d4d","observation_id":"c8e7ba60-6116-49ab-8a11-2ae30ec85955","resolution":{"observed_at":"2026-08-14T14:14:39.340586Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:39.321411Z","title":"Wang, Y .-G","venue":null,"work_id":"b093b806-5ba1-47b3-a8ab-650db429b5ea","year":2005},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:37.991049Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:761e9581047755a4ff17b827bd8320fe0c173db19e1a7fe51494a000eb9abe0f","observation_id":"48c1ea63-5d3f-46d1-8661-c92f227dfb19","resolution":{"observed_at":"2026-08-14T14:14:39.326417Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:39.306982Z","title":null,"venue":null,"work_id":"5ee0509b-9a22-44ab-90f1-46b4eddbe5dc","year":2006},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:37.994919Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:174e3da70e54f42b9c854db58e77525af45194544b2a538a7b2755093717ce34","observation_id":"3db8b659-77c4-4648-80bf-2cbdc2cf3a14","resolution":{"observed_at":"2026-08-14T14:14:39.311236Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:39.293134Z","title":"Wang, C.-Y","venue":null,"work_id":"ca921177-d56b-454d-ab9c-56b9167309c3","year":2006},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:37.998617Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:be11d90f1bf33daedc8c7978903bd65e44550b9c2d96d0c44549a273c3b0e8ca","observation_id":"ea5e731c-8c17-4ea2-8092-91e22b718640","resolution":{"observed_at":"2026-08-14T14:14:39.297683Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:39.279360Z","title":"Wang, C.-Y","venue":null,"work_id":"eacbdbe4-38bb-4c78-8ae7-283a73eafa95","year":2008},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.002289Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:8e2a3c4e65bc543a5b0923b9ef0e0a715c1e4d07c55e46270f394814411629cd","observation_id":"35f2679f-fa0b-44c8-953a-3fab25579c3e","resolution":{"observed_at":"2026-08-14T14:14:39.283746Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:39.265776Z","title":null,"venue":null,"work_id":"bdc3f2a4-576f-46f0-935c-be46d088cf03","year":2016},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.006210Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:6c444be78b7f7532c04221829dde678d8bde482930b8b92c960aa36aac2c01b4","observation_id":"34bc9c0b-3f46-453c-913e-9c29efe7fac1","resolution":{"observed_at":"2026-08-14T14:14:39.270155Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:39.253023Z","title":"Li, X.-D","venue":null,"work_id":"24f6d6fa-a1f5-416a-ae1e-5ea4e021834e","year":2009},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.009754Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:294748111db8ddfae84a9d8177d1cac4ba76503ddfd4834a71c716506a4b0c8e","observation_id":"6beba67a-9b69-462d-ab00-3a1796c5b080","resolution":{"observed_at":"2026-08-14T14:14:39.256843Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:39.240372Z","title":"Li, X.-D","venue":null,"work_id":"de40a78c-5b41-4a26-9dbb-47d90b29c4bd","year":2009},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.013276Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:577939872dd320d1bdf0414c193b60271dc428d50afec1706ea5ec4cbab0d9a6","observation_id":"fa1a3371-258a-4795-903c-6469ca65f03e","resolution":{"observed_at":"2026-08-14T14:14:39.244205Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:39.227620Z","title":"Li, X.-D","venue":null,"work_id":"68611c18-649c-45a7-89a5-53937e475b43","year":2011},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.016784Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:acc8a18e208ccecfeeccc0be414ef1577556852e12850b56ea668c712e4cb262","observation_id":"21795f77-c94b-4fda-bd65-ba0e11b11219","resolution":{"observed_at":"2026-08-14T14:14:39.231458Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:39.214309Z","title":"Saridakis","venue":null,"work_id":"4d4e2b13-fce7-4fc1-8425-efa11c12f501","year":2018},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.020689Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:d34ca9c3b969c9c60de65710e3f6c1e19c14acb495e88b6d9aed0d2e1097fabd","observation_id":"af3e9b03-b0f6-4ca2-94c4-92d5a82d611c","resolution":{"observed_at":"2026-08-14T14:14:39.218650Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:39.202033Z","title":"Al Mamon","venue":null,"work_id":"5df51450-4f31-4279-a7f7-df732009df87","year":2017},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.024260Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:39204e9904519e5c51f0d53047e3970aa800ff4654a5e93270facad3979fd288","observation_id":"a3fe346a-ddd3-46a1-a30c-f09342a5e779","resolution":{"observed_at":"2026-08-14T14:14:39.205656Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:39.190278Z","title":"Mukherjee","venue":null,"work_id":"2081cc8e-1b53-4842-bead-d0871b766479","year":2016},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.027900Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:358d8e14ce3ccf09b6f3b7c71aba233468030cc8582377513b1fa05b39ae2951","observation_id":"72ac63a8-5b9f-4421-87e0-8d8313cc873f","resolution":{"observed_at":"2026-08-14T14:14:39.193941Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:39.176810Z","title":"Feng and X","venue":null,"work_id":"31d040a9-f6ed-44b7-aa8e-fddb9b9483b9","year":2015},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.031420Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:6ae697271229e5721502d3d2fa02a886462a632829c4fdcac6f29744a22e8939","observation_id":"833f1a1f-21b4-4291-94e7-8a40f77960e0","resolution":{"observed_at":"2026-08-14T14:14:39.181189Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:39.163197Z","title":"Herrera, W","venue":null,"work_id":"ad87c6f9-2271-4aa8-aec5-16e9c2df65f5","year":2016},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.035026Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:1b7a3a181e0f61a2dcbbf0a613eb356de75342fa210980f8d63798f00389c491","observation_id":"108301b5-a437-422a-89b2-47bed1ebb6e4","resolution":{"observed_at":"2026-08-14T14:14:39.167575Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:39.149890Z","title":null,"venue":null,"work_id":"6fead4fa-cb5b-4dd4-adb9-2b39d3cf5004","year":2016},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.038861Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:0d7c517056c7b98b1a8a8277559db576eaa55b236865a2c40daafd6ce189dbcd","observation_id":"2d92fbca-d0d3-401a-8861-7eed8b84ef1d","resolution":{"observed_at":"2026-08-14T14:14:39.154057Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:39.136326Z","title":"Stachowski, and K","venue":null,"work_id":"70bed918-77be-4051-a80f-d1f29ed5212a","year":2017},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.042195Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:31d1193f427685b1ac488a294251959dd084f0cb17f14512acae901f43343fd8","observation_id":"49f20b81-3eab-476d-ba46-191fcbcdf894","resolution":{"observed_at":"2026-08-14T14:14:39.140495Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:39.122821Z","title":"Stachowski, M","venue":null,"work_id":"96a98738-2534-4e5f-bf63-7f548d83fc41","year":2017},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.045720Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:c0738e08326199ab0f1ff3014ae8241684eab90c2ee78b54ca0ba749990691d9","observation_id":"cdbfa562-bf44-4536-a131-bfd50af7f192","resolution":{"observed_at":"2026-08-14T14:14:39.127187Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:39.109032Z","title":"Stojkovic, G","venue":null,"work_id":"1269ab77-bf0a-4b22-829d-d7145f9ded7c","year":2008},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.049150Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:a8628fab79bcfc1c8d1ba297030b7ae156f38683b0a06dafe252908666161895","observation_id":"5956e23d-4f23-4d7c-afb2-e25369852345","resolution":{"observed_at":"2026-08-14T14:14:39.113584Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:39.096349Z","title":"Greenwood, E","venue":null,"work_id":"c68fffee-a69c-4b86-9012-1f69408831f5","year":2009},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.052704Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:33c30b1c32bf71b73d0c4ee78ff98bc5f15ff2690096faa2b6db87ad707a1f06","observation_id":"08661fb3-9f6a-4ecb-81d7-3f1ebbdd8250","resolution":{"observed_at":"2026-08-14T14:14:39.100022Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:39.083805Z","title":"Abdalla, L","venue":null,"work_id":"b6431410-a1f9-4b64-93c0-0d5d66ae18ca","year":2013},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.055981Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:940f1df5b86c5ebc95129d4c817a2639373655a889e96bbeb3346cb38dce1da6","observation_id":"22cec1c6-14de-4827-b1f4-2f2209ff6956","resolution":{"observed_at":"2026-08-14T14:14:39.087764Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:39.070966Z","title":"Shaﬁeloo, D","venue":null,"work_id":"71e0537e-10e7-4fc3-9d9f-a80b872e1e1a","year":2018},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.059373Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:5841bdf9dd5aa5ebff3f3e6e4c2801baca128840d0b23ad4bd40ec55f2dff027","observation_id":"e420dd85-d0a7-48d6-a1db-7d61b4cecffa","resolution":{"observed_at":"2026-08-14T14:14:39.074893Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:39.058519Z","title":null,"venue":null,"work_id":"f95a8d9a-8b2d-4c20-b834-f85509bc9255","year":2017},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.063078Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:d0b9f6acb023d4d333148c7534e59d15591057adddafeef6524dbe31f6832a1b","observation_id":"667d08bf-5da9-4096-a709-0e26e3c04167","resolution":{"observed_at":"2026-08-14T14:14:39.062359Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:39.045879Z","title":null,"venue":null,"work_id":"d797f581-aee0-49ef-ac63-df082aa860e1","year":1936},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.066558Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:d5714ee208935a1a8dd1a3351441028c2a788b810a8915c006cb2eff9b8619cd","observation_id":"8c0cd742-0bd3-448d-ad4e-11ef8e8e4f8e","resolution":{"observed_at":"2026-08-14T14:14:39.049833Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:39.033041Z","title":"Dvali, G","venue":null,"work_id":"4f6efde1-d40c-479a-9907-ecb877647438","year":2000},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.070224Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:38dc5744ba22bd43e3a849f644450e070f64d262db9496bfd61fefe96a634fbb","observation_id":"efc059a0-3993-4e90-9f3a-3019fa5590b7","resolution":{"observed_at":"2026-08-14T14:14:39.037082Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:39.018074Z","title":null,"venue":null,"work_id":"773b4916-c63b-4ed2-b8a3-4fbc42f62395","year":2007},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.073816Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:a92f865049b252fd3ade9444d260b0c0f40203cd2ce9d10caf437f22a4bde51c","observation_id":"92b5995e-bcc7-4c26-91bb-869e8db31720","resolution":{"observed_at":"2026-08-14T14:14:39.022724Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:39.003827Z","title":"Wetterich","venue":null,"work_id":"bbf6d0af-ab7f-4482-aebf-7e630f0fe4fb","year":1995},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.077312Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:081e002010d06ad107090f6c8fb788b6a0c98497c969b886c981ce3c03f91c59","observation_id":"f6be64e3-1543-4415-9ab1-827d7ac7b332","resolution":{"observed_at":"2026-08-14T14:14:39.008613Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.990478Z","title":"Amendola","venue":null,"work_id":"61710f9c-5311-40ec-93fe-52ceafe2ba24","year":2000},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.080726Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:de8491afb3b713e972e012303531b599ef934ce81a19bd498ba349e87f89afc6","observation_id":"39c311c7-a439-4ce5-8e68-929a2bdf52d8","resolution":{"observed_at":"2026-08-14T14:14:38.994718Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.977045Z","title":"Guo and Y .-Z","venue":null,"work_id":"59bf3ab4-6ce0-49d7-8aee-fc1c3831194f","year":2005},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.084614Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:f2d7545c5b3baf08013b0164b35725eeddcf307313e1da81adb404a7e471fa1d","observation_id":"75c93318-3dc9-49a5-b69e-75baa48b792e","resolution":{"observed_at":"2026-08-14T14:14:38.981432Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.963220Z","title":"Cai and A","venue":null,"work_id":"650ce9b6-eba7-4e38-9c3c-1e8ce2596709","year":2005},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.088222Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:d52764ce72a4f5f1819d3682e1696a4307835d23baac32621ec99ed704a537ed","observation_id":"dff94bba-ca07-4949-b67f-2559b0f3927f","resolution":{"observed_at":"2026-08-14T14:14:38.967613Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.949383Z","title":"Guo, R.-G","venue":null,"work_id":"85fd406e-061e-4df5-b2fd-5d8d3e514b83","year":2005},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.092102Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:dd356d895d3241f131aa7cd00e601ec41893b72375fa5fa4e9ff30e827ca8edf","observation_id":"a44ce82f-dce5-4def-b949-e38e7a8bb8e3","resolution":{"observed_at":"2026-08-14T14:14:38.953757Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.936305Z","title":null,"venue":null,"work_id":"daa5f4fc-4372-4d47-958e-490f218478c4","year":2005},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.095807Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:0b657d8be9767d574d84ac6e304974f955b0ab7f991cd538255ee1e5976c2027","observation_id":"fa2ee674-544c-487b-8cf6-88accee63eb3","resolution":{"observed_at":"2026-08-14T14:14:38.940336Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.922660Z","title":"Gumjudpai, T","venue":null,"work_id":"1c7fab95-2e81-4206-b3d1-4677761b03c3","year":2005},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.099340Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:30837d199bb82240d40a034aa6d6ed89a663890942ab6c8ffe0fab711e923d09","observation_id":"b820e7dd-15d3-400c-8295-1f849be24eab","resolution":{"observed_at":"2026-08-14T14:14:38.926770Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.909469Z","title":null,"venue":null,"work_id":"f1d56bda-7207-4233-b5be-7b189238c907","year":2014},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.102974Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:183b8978f6abaa8b9bd855f9c19ce11de3aadd2946db80bf6464396af4251268","observation_id":"2897014e-4640-4fe8-bbd3-043533a63fcb","resolution":{"observed_at":"2026-08-14T14:14:38.913520Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.897313Z","title":null,"venue":null,"work_id":"efa51aba-7e99-4842-8abe-8af21a821ae5","year":2017},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.106672Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:e2808269a539d8ff50d32154242205d5b7c2e30981acd972b5ec8c5f473d18fb","observation_id":"c630b9f9-c8fe-4f07-93e2-bcd11d7a0a5c","resolution":{"observed_at":"2026-08-14T14:14:38.901260Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.885453Z","title":null,"venue":null,"work_id":"92ad20a8-8408-4933-9360-88942639e551","year":2015},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.110631Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:51c72f7506664d0c649a986ceebede986eb704eeb3a14e5b6c156da9f0e9451a","observation_id":"b64c0ade-f852-40cb-acec-4d356bf035d1","resolution":{"observed_at":"2026-08-14T14:14:38.889026Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.873629Z","title":null,"venue":null,"work_id":"bbc329b8-9911-4ecf-9de1-13898f5e7313","year":2015},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.114257Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:7e533a1ba9645a221e78a2fbdb3366b2dfeff3965c67f88338be2203d5f1de05","observation_id":"45310f00-2627-4186-821c-aef2c48c680d","resolution":{"observed_at":"2026-08-14T14:14:38.877221Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.859933Z","title":null,"venue":null,"work_id":"274904d4-fe47-4ada-8dc6-a043317311e0","year":2016},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.117833Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:dc6f04a85392f7901bdc051d035241dddba520d3d018aae9fd96d248bf44f00d","observation_id":"cb3cce33-9ea9-456b-8486-3bc1f2796186","resolution":{"observed_at":"2026-08-14T14:14:38.864445Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.846734Z","title":null,"venue":null,"work_id":"f4e81b0d-6b3a-4797-9a23-f4e2c5690792","year":2017},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.122269Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:ea7d85adebf84de386495b9a4a84325940378c0b6a2b8cb8a934261fcf8bc628","observation_id":"2a523d9e-7661-4c90-a557-7132124c9a16","resolution":{"observed_at":"2026-08-14T14:14:38.850913Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.833297Z","title":null,"venue":null,"work_id":"0ca08cc9-b4e8-4b9b-b14a-34b823e99784","year":2016},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.126003Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:8eacd4b68c0f3a353233cd9e729c127c534c58ad8dfe7c3c66cff8fb26f5a1c8","observation_id":"2bd6239c-8d0d-4ea1-abe9-20d58ee729ce","resolution":{"observed_at":"2026-08-14T14:14:38.837497Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.820156Z","title":null,"venue":null,"work_id":"5b551bc9-2fd9-458b-bdfd-74dc89f74009","year":2004},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.129507Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:8de34dee2fab1a6208c8448c1fe5589bc8c117f79de9b132bdb6dfedecae8f56","observation_id":"76b4d640-0a1f-4d01-bbc3-b6c0b46a874f","resolution":{"observed_at":"2026-08-14T14:14:38.824065Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.807936Z","title":"Micheletti, E","venue":null,"work_id":"64d387d5-4993-4927-a72a-10d20d422c67","year":2009},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.133013Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:73c24a48bf5ddfa77044f19df739c83921ce4a5e2109c213309493301c526d0e","observation_id":"5951b978-026b-4cd1-b9e2-aaa17330ee8e","resolution":{"observed_at":"2026-08-14T14:14:38.811754Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.795532Z","title":"Yang and S","venue":null,"work_id":"55f32333-89db-48f6-92dc-31f864e0bc1a","year":2017},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.136580Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:2760967a7fea46f79815a9add79f6ca0f7b70f904a06d09c9514cdb7a5db43f8","observation_id":"2626f297-24a8-4f35-be0d-8dc07da8922d","resolution":{"observed_at":"2026-08-14T14:14:38.799493Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.783384Z","title":null,"venue":null,"work_id":"81c2fb72-4baa-4d48-9a4b-b4619d5eaed0","year":2017},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.140315Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:936e526489efbd7bdb51ae3617022872ff10456064ab7b5e855bd0add21ea794","observation_id":"34ffe1d0-598a-4ba7-8976-9c4edee0b4fd","resolution":{"observed_at":"2026-08-14T14:14:38.787029Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.771766Z","title":"Bar- row","venue":null,"work_id":"0cdee937-360b-41dd-b53b-b7e89f4d9622","year":2018},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.143659Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:ecf407bb16c4729df6da401d028affc9321d5b2d2542945292bef6d00d198962","observation_id":"701c20bb-02e8-4d0f-b808-b16b54db6962","resolution":{"observed_at":"2026-08-14T14:14:38.775301Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.759856Z","title":null,"venue":null,"work_id":"609c2996-740b-448b-b352-fc155c162c7b","year":2018},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.147126Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:56064e7446d4719f8459b0d63870ee4cdb0dcf45ee3647e433f8879ab989e0d7","observation_id":"ae46e2b7-3e6f-4b87-84f5-e0f6d755e13e","resolution":{"observed_at":"2026-08-14T14:14:38.763438Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.746551Z","title":null,"venue":null,"work_id":"e8bc6e9b-c4eb-4e0a-a502-162adb00c11b","year":2018},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.150939Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:00e2281bbfd818ce2e6d027d7dd3bb5cb7797a097020367082f0ffa938dca610","observation_id":"8bf1d450-21ee-4914-afc9-dad772a018fb","resolution":{"observed_at":"2026-08-14T14:14:38.751151Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.732509Z","title":"Zimdahl, D","venue":null,"work_id":"63c753a5-c443-41d9-8ca8-4a68cb32055a","year":2001},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.154199Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:3190fadacfb9563ed1fdfab773403007a2a3c92389908620bf1819295c031472","observation_id":"bdb5e774-f07d-45f9-b094-378e7aa2bfc5","resolution":{"observed_at":"2026-08-14T14:14:38.737486Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.718243Z","title":null,"venue":null,"work_id":"d14ffc6b-fc61-46c2-8a3d-352c8cf9da0c","year":2003},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.157657Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:b34561e81f53905e7766f3be189dddab7629ea6bee336ad00f474a736165ce52","observation_id":"aceb4713-c7ae-4438-b3bb-c714e669c6cc","resolution":{"observed_at":"2026-08-14T14:14:38.722579Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.705257Z","title":null,"venue":null,"work_id":"f404dd5a-e8b7-475b-8794-5a33f80da4b8","year":1998},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.161034Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:474eaff88835a23f827df61846480902a5d62dee9b53eb4b8f82298035a300ca","observation_id":"7133dcba-067d-4ad7-bcde-af15fc8db458","resolution":{"observed_at":"2026-08-14T14:14:38.709326Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.691580Z","title":null,"venue":null,"work_id":"4dc13d1d-734f-4612-ae4b-e0f3a71dea82","year":2001},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.164578Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:a78fe5b6b3b7e6bd736ab40bd88fffdef63fea7bc7cc758ebb5cdad5515b35fa","observation_id":"4edee57b-95f1-4600-a397-7a36b75a1fb0","resolution":{"observed_at":"2026-08-14T14:14:38.695883Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.678122Z","title":null,"venue":null,"work_id":"20f089cb-5255-4366-9c24-92085db97942","year":2005},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.168023Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:2a59973229263c54bfe2c000980184a2faf1c5c1dbf069af8e05e2c911fd0c1b","observation_id":"e108d26b-18b2-4aec-9939-4c10c8d7802b","resolution":{"observed_at":"2026-08-14T14:14:38.682361Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.664600Z","title":"Zhai and Y .-B","venue":null,"work_id":"9dad52ee-9869-4d1e-adf8-63c116525f97","year":2005},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.171635Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:45c374757320cbcef0a3812bf0c8cb82344bc77c79476c8f375475ae6f0c33fa","observation_id":"315766fe-54dc-4d80-8b38-fee264a947ec","resolution":{"observed_at":"2026-08-14T14:14:38.668727Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.649674Z","title":"De-Santiago, J","venue":null,"work_id":"94b8ca24-45a5-45d6-81a3-9c10b0b6f7e6","year":2013},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.175294Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:fc55d202d66af36243ebfa66aa2577a0a064e92ab4a7d8e6466c203274c96651","observation_id":"28d56b88-a21c-42d8-8240-60abef95f829","resolution":{"observed_at":"2026-08-14T14:14:38.654190Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.635653Z","title":"Tsujikawa","venue":null,"work_id":"d1ab6b66-99a5-4122-8763-cec529175e8d","year":2006},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.179108Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:89795a3c39bfdb8bba9677567b1485d32f8eb0d5b6341ebb38ded22b54c5adcb","observation_id":"bb60368a-5f18-4ac5-bee2-ad32bf2d2a66","resolution":{"observed_at":"2026-08-14T14:14:38.639988Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.622433Z","title":"Amendola, M","venue":null,"work_id":"7c4df08c-fae3-4d0b-97c6-4904d4dfd716","year":2006},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.182691Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:459a76ca6210beee0df84d8b67cf2dcd10f9d251aa759ead8f3e4b5aef8e4056","observation_id":"23ecc9ee-d60c-42be-935a-421f5ad29857","resolution":{"observed_at":"2026-08-14T14:14:38.626647Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.608816Z","title":"Chen, Y .-G","venue":null,"work_id":"9dc82f2e-297e-4867-af76-959419e0050e","year":2009},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.186162Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:01e12f1690098c025f15dbf4ae914c4b4bf36ee0a3a5832c59e1192b9679d6ec","observation_id":"da8f2ebc-9325-4c83-9af9-9ec61860eedf","resolution":{"observed_at":"2026-08-14T14:14:38.613545Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.595806Z","title":"Mahata and S","venue":null,"work_id":"3812a04d-2885-4539-9933-455609a02ecc","year":2015},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.189769Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:e683b0bda453bae331926ac377c4832fecf76cb98b9da69e46543348915fe661","observation_id":"469cbe45-fe9a-4efa-a80b-8d9a0b8dbcc4","resolution":{"observed_at":"2026-08-14T14:14:38.600348Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.582547Z","title":null,"venue":null,"work_id":"580ac299-3504-4f3c-8714-c2f4cf477003","year":2015},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.193708Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:049bcb6db71ea2790f86ab1033217f17e120618c9288c540839b2f5be44a80ee","observation_id":"80b0105f-b284-44c3-97fc-b48564faa9f0","resolution":{"observed_at":"2026-08-14T14:14:38.587008Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.567874Z","title":null,"venue":null,"work_id":"73ef0192-7893-43ba-b9b0-8fb1deb91aac","year":2016},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.198035Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:75a692dd48b82a9e1df2491d95439b8141b9dc035b85e0e023d94a1641c9c0ef","observation_id":"50563d21-5526-47c2-9ac2-08fa9fb863fa","resolution":{"observed_at":"2026-08-14T14:14:38.572962Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.554681Z","title":"Per- turbations of the Lambda-CDM model in a dynamical systems perspective","venue":null,"work_id":"37fe0d62-2025-43b7-af0c-41051006698e","year":1909},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.201875Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:eb7f6a4f85b3a758e17def87304aa3864387295f7ccb119d4898b96e6a46b03a","observation_id":"e96194bb-40eb-477d-8b62-517ad03aba3e","resolution":{"observed_at":"2026-08-14T14:14:38.559100Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.541944Z","title":"Papagiannopou- los, and Emmanuel N","venue":null,"work_id":"19c5ce8c-f86c-47b7-a3e8-80041713496c","year":2019},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.206425Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:0d4cbf2d5a49396bc354a1e19e4ab26e50b29ccc746999ac256a1ddabb105024","observation_id":"52d92ca0-4f29-40b8-8aa5-e30748072148","resolution":{"observed_at":"2026-08-14T14:14:38.545857Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.529426Z","title":"Bertolami and P","venue":null,"work_id":"ec470723-eaac-4cd8-b552-0769afebed56","year":2000},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.210871Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:865224707f74677ad77cc1e0ae70f65e7c542c08c85d6db50abb2aeff1fd55be","observation_id":"bda9b227-bd09-4926-9a20-2cdb1649029a","resolution":{"observed_at":"2026-08-14T14:14:38.533236Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.516837Z","title":"Constraints on ﬂat cosmologies with tracking quintessence from cos- mic microwave background observations","venue":null,"work_id":"ff559867-6719-450a-ad40-e3c21d44e083","year":2002},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.214851Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:a99efea022a1bea46da8bdc95a456b802262e19d5229ad355e32e74613b95fea","observation_id":"717e41b7-dcad-41b8-9b1c-f328ce1fb7ed","resolution":{"observed_at":"2026-08-14T14:14:38.520773Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.504312Z","title":null,"venue":null,"work_id":"ab5b9e62-1c55-4b7f-9b57-63e880f87815","year":2002},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.218686Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:b08c83ca0091d8acf7b5581a96a5e0c08609bc10a2d936db928af420feb9760d","observation_id":"14029cba-c5ad-48fe-ba41-09c9aa72e906","resolution":{"observed_at":"2026-08-14T14:14:38.508040Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.491850Z","title":"Extended quintessence with an exponential coupling","venue":null,"work_id":"fadf6225-a582-4d7b-a435-f132867b1a5b","year":2005},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.222266Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:0dd77c0cdf4160b85d29d14d2517bbc37d4e5925ae933346cfb1805a17a9ffdc","observation_id":"8b628cd1-69e6-4a14-b4c5-01a5f60489c3","resolution":{"observed_at":"2026-08-14T14:14:38.495938Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.479467Z","title":"Brookﬁeld, C","venue":null,"work_id":"90023bfa-1bc1-4d71-8c4e-53f064d1c016","year":2007},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.225886Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:f6b34c0755656af8fc8c5ba1bf0c39112ca6b0af7d6188b53d5f675ee2ed6294","observation_id":"912a0b6a-b0c4-413c-a748-2ffada9ccc3f","resolution":{"observed_at":"2026-08-14T14:14:38.483386Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.466693Z","title":"Growth of perturbations in dark matter coupled with quintessence","venue":null,"work_id":"42df9035-8386-4464-90ef-f7df13297bda","year":2005},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.229724Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:19ed3e18b96fd5999d0ccb34460ef8a50e66acbcb08337e9c6de56618775cfdd","observation_id":"8c79cafb-b63b-49b2-ba1f-408b62cfded5","resolution":{"observed_at":"2026-08-14T14:14:38.471030Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.452921Z","title":"Constraints on the coupled quintessence from cosmic microwave background anisotropy and matter power spectrum","venue":null,"work_id":"80cd1615-5fae-46f9-a91e-e9b2d1521639","year":2006},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.233437Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:c73f54a4d5e369b51b6b04308b252badd88aa6270148860d77037a21967ad0bf","observation_id":"afbcd0ed-b01a-4dfe-af95-3c134ef5f0ea","resolution":{"observed_at":"2026-08-14T14:14:38.457638Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.439521Z","title":"Atrio-Barandela, and D","venue":null,"work_id":"d46a4deb-8ec1-45bf-aa4a-69184f62733c","year":2006},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.237122Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:b0a43eff1bee482fda84031830aaffcdcbefb088d19a0217ededab67ad93dc62","observation_id":"e87620e3-a944-45a5-a8f5-017a28db6118","resolution":{"observed_at":"2026-08-14T14:14:38.443726Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.426894Z","title":"Coupled and Extended Quintessence: theoretical differences and structure formation","venue":null,"work_id":"1b2ffe7d-e9f2-45e2-a3b7-907e50692a64","year":2008},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.240932Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:e3203d251dd04972e5b81b98bd2339073949384fd49b12d159ca8ae3d0ed5ccc","observation_id":"da0e3503-73e5-47f7-bcac-12dde7f5a97c","resolution":{"observed_at":"2026-08-14T14:14:38.430810Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.413367Z","title":null,"venue":null,"work_id":"7da355b9-e62c-4486-a304-ae70f0f61ea1","year":2012},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.244571Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:1ce630b9236487507542f231c9489591a2c88525884811e21190b93577038ecc","observation_id":"5b63f3cb-499c-4cf2-89b0-45ba6cc2f7d7","resolution":{"observed_at":"2026-08-14T14:14:38.418008Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.400514Z","title":"Cosmolog- ical structure formation with clustering quintessence","venue":null,"work_id":"10da5da5-e541-45e4-ac62-0d52e45d99d5","year":2011},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.248290Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:cf8b404e534323ccf12116c27a47a4c0e7dd1386827399d59675b4d596cac7ca","observation_id":"aca0fbdb-bbc5-4443-b5fc-e0d0721b3f14","resolution":{"observed_at":"2026-08-14T14:14:38.404589Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.388020Z","title":"Constraining coupled quintessence with the 21cm sig- nal","venue":null,"work_id":"dd8d58a3-9e99-475a-9a81-fedfeddd918c","year":2019},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.251994Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:572525273c3180681fac76aca6d8c57487bc35636e0f5befef3b0f902243c507","observation_id":"078910ad-e86e-44df-b081-dd4305db2e0b","resolution":{"observed_at":"2026-08-14T14:14:38.392065Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.374762Z","title":"França and R","venue":null,"work_id":"7b53552a-706b-4cb6-8608-22d9ebb82645","year":2002},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.255713Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:9c80653fe903cfceb7e8c51cd01ba92fa8febb22a94d9e9b7f66252f1f12e71c","observation_id":"a210854e-6d88-41cf-99d7-8732f77812f7","resolution":{"observed_at":"2026-08-14T14:14:38.379025Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.359297Z","title":"Duniya, D","venue":null,"work_id":"614bb5b2-53ea-46cf-ab74-c337a4484161","year":2013},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.259955Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:3c760f0e0b918cf0d009c77816e69bebfc23772dc5084d8d9a407d53a776610e","observation_id":"2a179101-0a41-47f8-99a2-2341a62f8b71","resolution":{"observed_at":"2026-08-14T14:14:38.363104Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.345747Z","title":"Bahamonde, C","venue":null,"work_id":"e94d9fae-ea80-4414-b20b-96e2935a6421","year":2018},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.263710Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:799d0b9e1dfc231ac927a139c821459ac2f590edd301cad5ad7d024e66fad97e","observation_id":"27de245b-7445-4f8b-bb4c-d69f276c3a9f","resolution":{"observed_at":"2026-08-14T14:14:38.349672Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:14:38.333016Z","title":null,"venue":null,"work_id":"5a72daba-78f0-406f-9a74-640e7fa3de78","year":2012},"citing_paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence","version":3},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:38.267487Z"},"links":{"citing_paper":"/paper/1908.03657"},"observation_digest":"sha256:8c022fef7bb7933f841292ac75b9385894c8fea515a992d49354d75c8122a9ec","observation_id":"cea05128-7872-4384-8e7b-33c06c1aabe1","resolution":{"observed_at":"2026-08-14T14:14:38.336784Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"1908.03657","last_updated":"2019-10-21T16:49:52Z","latest_version":3,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-14T14:04:30.015573Z","submitted_at":"2019-08-10T00:52:11Z","title":"Cosmological perturbations and dynamical analysis for interacting quintessence"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":50,"verified_exact":0,"verified_fuzzy":50},"total_outbound_references":102},"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":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 100 of 102 outbound references and 1 inbound Pith citation observation for arXiv:1908.03657."}