{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:VPXKCDP66MX7JIPNIDOCREQLCA","short_pith_number":"pith:VPXKCDP6","schema_version":"1.0","canonical_sha256":"abeea10dfef32ff4a1ed40dc28920b100f18000e7cf4878c0ba6a1c70b3c22cb","source":{"kind":"arxiv","id":"1502.04673","version":2},"attestation_state":"computed","paper":{"title":"Reheating predictions in single field inflation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph","hep-th"],"primary_cat":"astro-ph.CO","authors_text":"Damien A. Easson, Emanuela Dimastrogiovanni, Jessica L. Cook, Lawrence M. Krauss","submitted_at":"2015-02-16T19:31:21Z","abstract_excerpt":"Reheating is a transition era after the end of inflation, during which the inflaton is converted into the particles that populate the Universe at later times. No direct cosmological observables are normally traceable to this period of reheating. Indirect bounds can however be derived. One possibility is to consider cosmological evolution for observable CMB scales from the time of Hubble crossing to the present time. Depending upon the model, the duration and final temperature after reheating, as well as its equation of state, may be directly linked to inflationary observables. For single-field"},"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":"1502.04673","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2015-02-16T19:31:21Z","cross_cats_sorted":["gr-qc","hep-ph","hep-th"],"title_canon_sha256":"5d18791d55149f9ece11af5160b348317ffc53be035c80af7e6d8862252feef0","abstract_canon_sha256":"d70b17ae7a00220a630aab7c6ca19e9d09a27029443a8768bc44c0c398c8a9d3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:41:01.332590Z","signature_b64":"xyMBZZFtnThHLXxzKkqwz7cAVFaGc60uIKH+jeRnEJelYQFiF0xPyKrSUUEecDSz2NDSnKvxGBUt2wIYbvjmBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"abeea10dfef32ff4a1ed40dc28920b100f18000e7cf4878c0ba6a1c70b3c22cb","last_reissued_at":"2026-05-18T01:41:01.332001Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:41:01.332001Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Reheating predictions in single field inflation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph","hep-th"],"primary_cat":"astro-ph.CO","authors_text":"Damien A. Easson, Emanuela Dimastrogiovanni, Jessica L. Cook, Lawrence M. Krauss","submitted_at":"2015-02-16T19:31:21Z","abstract_excerpt":"Reheating is a transition era after the end of inflation, during which the inflaton is converted into the particles that populate the Universe at later times. No direct cosmological observables are normally traceable to this period of reheating. Indirect bounds can however be derived. One possibility is to consider cosmological evolution for observable CMB scales from the time of Hubble crossing to the present time. Depending upon the model, the duration and final temperature after reheating, as well as its equation of state, may be directly linked to inflationary observables. For single-field"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1502.04673","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"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":"1502.04673","created_at":"2026-05-18T01:41:01.332082+00:00"},{"alias_kind":"arxiv_version","alias_value":"1502.04673v2","created_at":"2026-05-18T01:41:01.332082+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1502.04673","created_at":"2026-05-18T01:41:01.332082+00:00"},{"alias_kind":"pith_short_12","alias_value":"VPXKCDP66MX7","created_at":"2026-05-18T12:29:47.479230+00:00"},{"alias_kind":"pith_short_16","alias_value":"VPXKCDP66MX7JIPN","created_at":"2026-05-18T12:29:47.479230+00:00"},{"alias_kind":"pith_short_8","alias_value":"VPXKCDP6","created_at":"2026-05-18T12:29:47.479230+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":10,"internal_anchor_count":7,"sample":[{"citing_arxiv_id":"2505.10534","citing_title":"ACT-ing on inflation: Implications of non Bunch-Davies initial condition and reheating on single-field slow roll models","ref_index":84,"is_internal_anchor":true},{"citing_arxiv_id":"2605.19825","citing_title":"Inflaton Accretion onto Primordial Black Holes During Reheating","ref_index":69,"is_internal_anchor":true},{"citing_arxiv_id":"2507.13465","citing_title":"Equation of state during (p)reheating with trilinear interactions","ref_index":23,"is_internal_anchor":true},{"citing_arxiv_id":"2508.10103","citing_title":"Leptogenesis and neutrino mass with one right-handed neutrino and Higgs inflaton","ref_index":58,"is_internal_anchor":true},{"citing_arxiv_id":"2511.04933","citing_title":"Low-reheating scenario in dark Higgs inflation and its impact on dark photon dark matter production","ref_index":78,"is_internal_anchor":true},{"citing_arxiv_id":"2602.00317","citing_title":"Reheating in geometric Weyl-invariant Einstein-Cartan gravity","ref_index":45,"is_internal_anchor":true},{"citing_arxiv_id":"2605.14044","citing_title":"The Magnetic Origin of Primordial Black Holes: Ultralight PBHs and Secondary GWs","ref_index":105,"is_internal_anchor":true},{"citing_arxiv_id":"2604.14659","citing_title":"Constraining Quintessential Inflation with ACT: A Gauss-Bonnet Gateway","ref_index":103,"is_internal_anchor":false},{"citing_arxiv_id":"2604.15194","citing_title":"Dilaton-Flattened Axion Inflation","ref_index":43,"is_internal_anchor":false},{"citing_arxiv_id":"2604.18641","citing_title":"Inflation from a Weyl-flat null origin","ref_index":26,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/VPXKCDP66MX7JIPNIDOCREQLCA","json":"https://pith.science/pith/VPXKCDP66MX7JIPNIDOCREQLCA.json","graph_json":"https://pith.science/api/pith-number/VPXKCDP66MX7JIPNIDOCREQLCA/graph.json","events_json":"https://pith.science/api/pith-number/VPXKCDP66MX7JIPNIDOCREQLCA/events.json","paper":"https://pith.science/paper/VPXKCDP6"},"agent_actions":{"view_html":"https://pith.science/pith/VPXKCDP66MX7JIPNIDOCREQLCA","download_json":"https://pith.science/pith/VPXKCDP66MX7JIPNIDOCREQLCA.json","view_paper":"https://pith.science/paper/VPXKCDP6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1502.04673&json=true","fetch_graph":"https://pith.science/api/pith-number/VPXKCDP66MX7JIPNIDOCREQLCA/graph.json","fetch_events":"https://pith.science/api/pith-number/VPXKCDP66MX7JIPNIDOCREQLCA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VPXKCDP66MX7JIPNIDOCREQLCA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VPXKCDP66MX7JIPNIDOCREQLCA/action/storage_attestation","attest_author":"https://pith.science/pith/VPXKCDP66MX7JIPNIDOCREQLCA/action/author_attestation","sign_citation":"https://pith.science/pith/VPXKCDP66MX7JIPNIDOCREQLCA/action/citation_signature","submit_replication":"https://pith.science/pith/VPXKCDP66MX7JIPNIDOCREQLCA/action/replication_record"}},"created_at":"2026-05-18T01:41:01.332082+00:00","updated_at":"2026-05-18T01:41:01.332082+00:00"}