{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:MJM37SY533W56LM5L3XOLIOLYY","short_pith_number":"pith:MJM37SY5","schema_version":"1.0","canonical_sha256":"6259bfcb1ddeeddf2d9d5eeee5a1cbc615ca81712a7d1f8f2f132cd8111b2f52","source":{"kind":"arxiv","id":"2406.04161","version":3},"attestation_state":"computed","paper":{"title":"Gravitational reheating in Starobinsky inflation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Gl\\'auber C. Dorsch, Luiz Miranda, Nelson Yokomizo","submitted_at":"2024-06-06T15:19:56Z","abstract_excerpt":"We investigate the possibility of achieving post-inflationary reheating exclusively through the gravitational interaction in Starobinsky inflation, which itself assumes nothing but gravity. We consider the possibility that the reheating sector couples to gravity via a non-minimal coupling. Our analysis is performed both in a perturbative and in a non-perturbative approach, where particle production is computed from Bogoliubov coefficients. Our findings indicate that, for a minimal coupling, a reheating temperature $T_\\text{reh}\\sim 10^{8}$~GeV is obtained, with a reheating duration of approxim"},"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":"2406.04161","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2024-06-06T15:19:56Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"ec106f458318dfb6139ab4717ea1be06136b5f237e4df545270100cec256a21a","abstract_canon_sha256":"62336a7c43a26397aaf0e8d29a4c0c674a942e346e198ea507f5e65aedd0dd09"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:33:14.827621Z","signature_b64":"cxO8mE6Pad9NeEvWxCqcN2PObAQ/QvEdMzB8ey9BWPfegq//FACIgjpIO//WzhrxGw/JRWG0S32k7gIfpjOtCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6259bfcb1ddeeddf2d9d5eeee5a1cbc615ca81712a7d1f8f2f132cd8111b2f52","last_reissued_at":"2026-07-05T11:33:14.827112Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:33:14.827112Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gravitational reheating in Starobinsky inflation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Gl\\'auber C. Dorsch, Luiz Miranda, Nelson Yokomizo","submitted_at":"2024-06-06T15:19:56Z","abstract_excerpt":"We investigate the possibility of achieving post-inflationary reheating exclusively through the gravitational interaction in Starobinsky inflation, which itself assumes nothing but gravity. We consider the possibility that the reheating sector couples to gravity via a non-minimal coupling. Our analysis is performed both in a perturbative and in a non-perturbative approach, where particle production is computed from Bogoliubov coefficients. Our findings indicate that, for a minimal coupling, a reheating temperature $T_\\text{reh}\\sim 10^{8}$~GeV is obtained, with a reheating duration of approxim"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2406.04161","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/2406.04161/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":"2406.04161","created_at":"2026-07-05T11:33:14.827170+00:00"},{"alias_kind":"arxiv_version","alias_value":"2406.04161v3","created_at":"2026-07-05T11:33:14.827170+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2406.04161","created_at":"2026-07-05T11:33:14.827170+00:00"},{"alias_kind":"pith_short_12","alias_value":"MJM37SY533W5","created_at":"2026-07-05T11:33:14.827170+00:00"},{"alias_kind":"pith_short_16","alias_value":"MJM37SY533W56LM5","created_at":"2026-07-05T11:33:14.827170+00:00"},{"alias_kind":"pith_short_8","alias_value":"MJM37SY5","created_at":"2026-07-05T11:33:14.827170+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.28502","citing_title":"Reheating matters: Starobinsky inflation in light of joint CMB+BAO results and gravitational-wave forecasts","ref_index":5,"is_internal_anchor":false},{"citing_arxiv_id":"2601.07670","citing_title":"Tachyonic gravitational dark matter production after inflation","ref_index":90,"is_internal_anchor":false},{"citing_arxiv_id":"2604.09356","citing_title":"CMB signatures of gravity-mediated dark radiation in $\\mathbf{\\Delta N_{\\rm eff}}$","ref_index":61,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/MJM37SY533W56LM5L3XOLIOLYY","json":"https://pith.science/pith/MJM37SY533W56LM5L3XOLIOLYY.json","graph_json":"https://pith.science/api/pith-number/MJM37SY533W56LM5L3XOLIOLYY/graph.json","events_json":"https://pith.science/api/pith-number/MJM37SY533W56LM5L3XOLIOLYY/events.json","paper":"https://pith.science/paper/MJM37SY5"},"agent_actions":{"view_html":"https://pith.science/pith/MJM37SY533W56LM5L3XOLIOLYY","download_json":"https://pith.science/pith/MJM37SY533W56LM5L3XOLIOLYY.json","view_paper":"https://pith.science/paper/MJM37SY5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2406.04161&json=true","fetch_graph":"https://pith.science/api/pith-number/MJM37SY533W56LM5L3XOLIOLYY/graph.json","fetch_events":"https://pith.science/api/pith-number/MJM37SY533W56LM5L3XOLIOLYY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MJM37SY533W56LM5L3XOLIOLYY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MJM37SY533W56LM5L3XOLIOLYY/action/storage_attestation","attest_author":"https://pith.science/pith/MJM37SY533W56LM5L3XOLIOLYY/action/author_attestation","sign_citation":"https://pith.science/pith/MJM37SY533W56LM5L3XOLIOLYY/action/citation_signature","submit_replication":"https://pith.science/pith/MJM37SY533W56LM5L3XOLIOLYY/action/replication_record"}},"created_at":"2026-07-05T11:33:14.827170+00:00","updated_at":"2026-07-05T11:33:14.827170+00:00"}