{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:RXW4EHIIJ7XOFVN7UQ2G7YHE4H","short_pith_number":"pith:RXW4EHII","schema_version":"1.0","canonical_sha256":"8dedc21d084feee2d5bfa4346fe0e4e1e782db6db02aa65c1a8fe285c9512e61","source":{"kind":"arxiv","id":"2407.16644","version":3},"attestation_state":"computed","paper":{"title":"Testing the phenomenological interacting dark energy model with gamma-ray bursts and Pantheon+ type Ia supernovae","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Nan Liang, Xiao-Dong Nong","submitted_at":"2024-07-23T16:58:14Z","abstract_excerpt":"In this paper, we utilize recent observational data from gamma-ray bursts (GRBs) and Pantheon+ supernovae Ia (SNe Ia) sample to explore the interacting dark energy (IDE) model in a phenomenological scenario. Results from GRBs alone, SNe Ia and GRBs+SNe Ia indicate that the energy is transferred from dark energy to dark matter and the coincidence problem is alleviated. The value of $H_0$ from GRBs+SNe Ia in the IDE scenario shows agreement with the SH0ES measurement. Considering the age estimate of the quasar APM 08279+5255 at $z = 3.91$, we find that the phenomenological IDE scenario can predi"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"2407.16644","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2024-07-23T16:58:14Z","cross_cats_sorted":[],"title_canon_sha256":"a6e42ff7ae44ad2814a9003318cfcc0c7e3e6321322044c1aedd8c9bcc6b3cde","abstract_canon_sha256":"aa2b4048de1231357d9e2428da5131a3d7163bc92f518ea48fe7b88145cfc5cc"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:43:31.913926Z","signature_b64":"3WiyDii73eN/JM7y86KuFSyjK58sspl21h2uQM2QnTmGcelyx3kOcVe2UPgz7TpUUh/7hVvEbqjFRvustyDgCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8dedc21d084feee2d5bfa4346fe0e4e1e782db6db02aa65c1a8fe285c9512e61","last_reissued_at":"2026-07-05T09:43:31.913465Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:43:31.913465Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Testing the phenomenological interacting dark energy model with gamma-ray bursts and Pantheon+ type Ia supernovae","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Nan Liang, Xiao-Dong Nong","submitted_at":"2024-07-23T16:58:14Z","abstract_excerpt":"In this paper, we utilize recent observational data from gamma-ray bursts (GRBs) and Pantheon+ supernovae Ia (SNe Ia) sample to explore the interacting dark energy (IDE) model in a phenomenological scenario. Results from GRBs alone, SNe Ia and GRBs+SNe Ia indicate that the energy is transferred from dark energy to dark matter and the coincidence problem is alleviated. The value of $H_0$ from GRBs+SNe Ia in the IDE scenario shows agreement with the SH0ES measurement. Considering the age estimate of the quasar APM 08279+5255 at $z = 3.91$, we find that the phenomenological IDE scenario can predi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2407.16644","kind":"arxiv","version":3},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2407.16644/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"2407.16644","created_at":"2026-07-05T09:43:31.913524+00:00"},{"alias_kind":"arxiv_version","alias_value":"2407.16644v3","created_at":"2026-07-05T09:43:31.913524+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2407.16644","created_at":"2026-07-05T09:43:31.913524+00:00"},{"alias_kind":"pith_short_12","alias_value":"RXW4EHIIJ7XO","created_at":"2026-07-05T09:43:31.913524+00:00"},{"alias_kind":"pith_short_16","alias_value":"RXW4EHIIJ7XOFVN7","created_at":"2026-07-05T09:43:31.913524+00:00"},{"alias_kind":"pith_short_8","alias_value":"RXW4EHII","created_at":"2026-07-05T09:43:31.913524+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2505.16438","citing_title":"Exploring parametrized dark energy models in interacting scenario","ref_index":20,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/RXW4EHIIJ7XOFVN7UQ2G7YHE4H","json":"https://pith.science/pith/RXW4EHIIJ7XOFVN7UQ2G7YHE4H.json","graph_json":"https://pith.science/api/pith-number/RXW4EHIIJ7XOFVN7UQ2G7YHE4H/graph.json","events_json":"https://pith.science/api/pith-number/RXW4EHIIJ7XOFVN7UQ2G7YHE4H/events.json","paper":"https://pith.science/paper/RXW4EHII"},"agent_actions":{"view_html":"https://pith.science/pith/RXW4EHIIJ7XOFVN7UQ2G7YHE4H","download_json":"https://pith.science/pith/RXW4EHIIJ7XOFVN7UQ2G7YHE4H.json","view_paper":"https://pith.science/paper/RXW4EHII","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2407.16644&json=true","fetch_graph":"https://pith.science/api/pith-number/RXW4EHIIJ7XOFVN7UQ2G7YHE4H/graph.json","fetch_events":"https://pith.science/api/pith-number/RXW4EHIIJ7XOFVN7UQ2G7YHE4H/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RXW4EHIIJ7XOFVN7UQ2G7YHE4H/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RXW4EHIIJ7XOFVN7UQ2G7YHE4H/action/storage_attestation","attest_author":"https://pith.science/pith/RXW4EHIIJ7XOFVN7UQ2G7YHE4H/action/author_attestation","sign_citation":"https://pith.science/pith/RXW4EHIIJ7XOFVN7UQ2G7YHE4H/action/citation_signature","submit_replication":"https://pith.science/pith/RXW4EHIIJ7XOFVN7UQ2G7YHE4H/action/replication_record"}},"created_at":"2026-07-05T09:43:31.913524+00:00","updated_at":"2026-07-05T09:43:31.913524+00:00"}