{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:EZXXKBN53ZHKDUES7DLI4PP4Z2","short_pith_number":"pith:EZXXKBN5","schema_version":"1.0","canonical_sha256":"266f7505bdde4ea1d092f8d68e3dfcce8611e3f5f6c2bcb5d2052be35220ce85","source":{"kind":"arxiv","id":"2509.07076","version":1},"attestation_state":"computed","paper":{"title":"Boiling After the Dust Settles: Constraining First-Order Phase Transitions During Dark Energy Domination","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Runqing Wang, Seth Koren, Yuhsin Tsai","submitted_at":"2025-09-08T18:00:02Z","abstract_excerpt":"A first-order phase transition could occur in the late universe when vacuum energy begins dominating the energy density ($z \\lesssim 0.3$) and convert some latent heat into other forms such as invisible radiation. This generic possibility also has concrete motivation in particle physics models which invoke a multitude of vacua to address theoretical puzzles. The na\\\"{i}ve constraint on such an event comes from measurements of the Hubble expansion rate, but this can only probe transitions involving $\\mathcal{O}(10)\\%$ of the dark energy. In this work, we show that significantly tighter constrai"},"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":"2509.07076","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-ph","submitted_at":"2025-09-08T18:00:02Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"3e87b2d3e3c1fb4bf173c41537571e260d03b192f1c2ee6d1470a9ae9be76801","abstract_canon_sha256":"b4b6053df48d0d8073ed5103ca8c130a441d70650a90e00c78ae07e07909a576"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T12:07:15.203421Z","signature_b64":"d40iAIZ/kK3HR9Zux+6vW/qv597bwAtadg+ndKIMXUSedSLMHkKO4yUXR5SAx/RAIJA9zVLoshx7Ku+6hxwZCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"266f7505bdde4ea1d092f8d68e3dfcce8611e3f5f6c2bcb5d2052be35220ce85","last_reissued_at":"2026-07-05T12:07:15.202647Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T12:07:15.202647Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Boiling After the Dust Settles: Constraining First-Order Phase Transitions During Dark Energy Domination","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Runqing Wang, Seth Koren, Yuhsin Tsai","submitted_at":"2025-09-08T18:00:02Z","abstract_excerpt":"A first-order phase transition could occur in the late universe when vacuum energy begins dominating the energy density ($z \\lesssim 0.3$) and convert some latent heat into other forms such as invisible radiation. This generic possibility also has concrete motivation in particle physics models which invoke a multitude of vacua to address theoretical puzzles. The na\\\"{i}ve constraint on such an event comes from measurements of the Hubble expansion rate, but this can only probe transitions involving $\\mathcal{O}(10)\\%$ of the dark energy. In this work, we show that significantly tighter constrai"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2509.07076","kind":"arxiv","version":1},"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/2509.07076/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":"2509.07076","created_at":"2026-07-05T12:07:15.202802+00:00"},{"alias_kind":"arxiv_version","alias_value":"2509.07076v1","created_at":"2026-07-05T12:07:15.202802+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2509.07076","created_at":"2026-07-05T12:07:15.202802+00:00"},{"alias_kind":"pith_short_12","alias_value":"EZXXKBN53ZHK","created_at":"2026-07-05T12:07:15.202802+00:00"},{"alias_kind":"pith_short_16","alias_value":"EZXXKBN53ZHKDUES","created_at":"2026-07-05T12:07:15.202802+00:00"},{"alias_kind":"pith_short_8","alias_value":"EZXXKBN5","created_at":"2026-07-05T12:07:15.202802+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.25014","citing_title":"Probing Confining Dark Sectors with Cosmological Perturbations","ref_index":59,"is_internal_anchor":false},{"citing_arxiv_id":"2605.30259","citing_title":"Late-time Quantum Vacuum Decay and its Cosmological Implications","ref_index":64,"is_internal_anchor":false},{"citing_arxiv_id":"2605.03007","citing_title":"Post-Recombination Fluctuations from a Sequestered Dark Sector","ref_index":25,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/EZXXKBN53ZHKDUES7DLI4PP4Z2","json":"https://pith.science/pith/EZXXKBN53ZHKDUES7DLI4PP4Z2.json","graph_json":"https://pith.science/api/pith-number/EZXXKBN53ZHKDUES7DLI4PP4Z2/graph.json","events_json":"https://pith.science/api/pith-number/EZXXKBN53ZHKDUES7DLI4PP4Z2/events.json","paper":"https://pith.science/paper/EZXXKBN5"},"agent_actions":{"view_html":"https://pith.science/pith/EZXXKBN53ZHKDUES7DLI4PP4Z2","download_json":"https://pith.science/pith/EZXXKBN53ZHKDUES7DLI4PP4Z2.json","view_paper":"https://pith.science/paper/EZXXKBN5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2509.07076&json=true","fetch_graph":"https://pith.science/api/pith-number/EZXXKBN53ZHKDUES7DLI4PP4Z2/graph.json","fetch_events":"https://pith.science/api/pith-number/EZXXKBN53ZHKDUES7DLI4PP4Z2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EZXXKBN53ZHKDUES7DLI4PP4Z2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EZXXKBN53ZHKDUES7DLI4PP4Z2/action/storage_attestation","attest_author":"https://pith.science/pith/EZXXKBN53ZHKDUES7DLI4PP4Z2/action/author_attestation","sign_citation":"https://pith.science/pith/EZXXKBN53ZHKDUES7DLI4PP4Z2/action/citation_signature","submit_replication":"https://pith.science/pith/EZXXKBN53ZHKDUES7DLI4PP4Z2/action/replication_record"}},"created_at":"2026-07-05T12:07:15.202802+00:00","updated_at":"2026-07-05T12:07:15.202802+00:00"}