{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:YVCTNK5ILNAHANBPQWBNRLNBQ2","short_pith_number":"pith:YVCTNK5I","schema_version":"1.0","canonical_sha256":"c54536aba85b4070342f8582d8ada186bb7ebe21466aa84d329b643f50b7f1eb","source":{"kind":"arxiv","id":"2311.16222","version":1},"attestation_state":"computed","paper":{"title":"Finite Bubble Statistics Constrain Late Cosmological Phase Transitions","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Gilly Elor, Robert McGehee, Ryusuke Jinno, Soubhik Kumar, Yuhsin Tsai","submitted_at":"2023-11-27T19:00:00Z","abstract_excerpt":"We consider first order cosmological phase transitions (PT) happening at late times, below Standard Model (SM) temperatures $T_{\\rm PT} \\lesssim$ GeV. The inherently stochastic nature of bubble nucleation and the finite number of bubbles associated with a late-time PT lead to superhorizon fluctuations in the PT completion time. We compute how such fluctuations eventually source curvature fluctuations with universal properties, independent of the microphysics of the PT dynamics. Using Cosmic Microwave Background (CMB) and Large Scale Structure (LSS) measurements, we constrain the energy release"},"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":"2311.16222","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-ph","submitted_at":"2023-11-27T19:00:00Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"6db6f07dddcd6b3057d32b16b574e37e446620e4cc97bfe1b392a0038830892b","abstract_canon_sha256":"43c52851a7131c5780500b48fd368544505e093c0ec7a485acb7377d94a3867f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:17:38.054389Z","signature_b64":"fc4FBh67VadTZ2+DldwORsvTbhhYzW+QHs3GmdXURn0UejKsiDBKxqXsoUFva/pkMtguEcnaYAHNtyx8Yv8MCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c54536aba85b4070342f8582d8ada186bb7ebe21466aa84d329b643f50b7f1eb","last_reissued_at":"2026-07-05T07:17:38.053892Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:17:38.053892Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Finite Bubble Statistics Constrain Late Cosmological Phase Transitions","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Gilly Elor, Robert McGehee, Ryusuke Jinno, Soubhik Kumar, Yuhsin Tsai","submitted_at":"2023-11-27T19:00:00Z","abstract_excerpt":"We consider first order cosmological phase transitions (PT) happening at late times, below Standard Model (SM) temperatures $T_{\\rm PT} \\lesssim$ GeV. The inherently stochastic nature of bubble nucleation and the finite number of bubbles associated with a late-time PT lead to superhorizon fluctuations in the PT completion time. We compute how such fluctuations eventually source curvature fluctuations with universal properties, independent of the microphysics of the PT dynamics. Using Cosmic Microwave Background (CMB) and Large Scale Structure (LSS) measurements, we constrain the energy release"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2311.16222","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/2311.16222/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":"2311.16222","created_at":"2026-07-05T07:17:38.053953+00:00"},{"alias_kind":"arxiv_version","alias_value":"2311.16222v1","created_at":"2026-07-05T07:17:38.053953+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2311.16222","created_at":"2026-07-05T07:17:38.053953+00:00"},{"alias_kind":"pith_short_12","alias_value":"YVCTNK5ILNAH","created_at":"2026-07-05T07:17:38.053953+00:00"},{"alias_kind":"pith_short_16","alias_value":"YVCTNK5ILNAHANBP","created_at":"2026-07-05T07:17:38.053953+00:00"},{"alias_kind":"pith_short_8","alias_value":"YVCTNK5I","created_at":"2026-07-05T07:17:38.053953+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":11,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.25014","citing_title":"Probing Confining Dark Sectors with Cosmological Perturbations","ref_index":54,"is_internal_anchor":false},{"citing_arxiv_id":"2605.27519","citing_title":"Probing Dynamical Inverse Seesaw with Low-frequency Gravitational Waves","ref_index":125,"is_internal_anchor":false},{"citing_arxiv_id":"2605.30259","citing_title":"Late-time Quantum Vacuum Decay and its Cosmological Implications","ref_index":63,"is_internal_anchor":false},{"citing_arxiv_id":"2410.23348","citing_title":"Observable CMB B-modes from Cosmological Phase Transitions","ref_index":57,"is_internal_anchor":false},{"citing_arxiv_id":"2502.20166","citing_title":"Numerical simulations of density perturbation and gravitational wave production from cosmological first-order phase transition","ref_index":106,"is_internal_anchor":false},{"citing_arxiv_id":"2503.01962","citing_title":"Curvature Perturbations from First-Order Phase Transitions: Implications to Black Holes and Gravitational Waves","ref_index":35,"is_internal_anchor":false},{"citing_arxiv_id":"2505.09202","citing_title":"Angular momentum of vacuum bubbles in a first-order phase transition","ref_index":20,"is_internal_anchor":false},{"citing_arxiv_id":"2512.08301","citing_title":"Isocurvature Induced Gravitational Waves at Pulsar Timing Arrays","ref_index":54,"is_internal_anchor":false},{"citing_arxiv_id":"2605.15197","citing_title":"Primordial Black Hole from Tensor-induced Density Fluctuation: First-order Phase Transitions and Domain Walls","ref_index":293,"is_internal_anchor":false},{"citing_arxiv_id":"2605.11079","citing_title":"New Isocurvature Constraints from JWST UV Luminosity Function","ref_index":26,"is_internal_anchor":false},{"citing_arxiv_id":"2605.03007","citing_title":"Post-Recombination Fluctuations from a Sequestered Dark Sector","ref_index":24,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/YVCTNK5ILNAHANBPQWBNRLNBQ2","json":"https://pith.science/pith/YVCTNK5ILNAHANBPQWBNRLNBQ2.json","graph_json":"https://pith.science/api/pith-number/YVCTNK5ILNAHANBPQWBNRLNBQ2/graph.json","events_json":"https://pith.science/api/pith-number/YVCTNK5ILNAHANBPQWBNRLNBQ2/events.json","paper":"https://pith.science/paper/YVCTNK5I"},"agent_actions":{"view_html":"https://pith.science/pith/YVCTNK5ILNAHANBPQWBNRLNBQ2","download_json":"https://pith.science/pith/YVCTNK5ILNAHANBPQWBNRLNBQ2.json","view_paper":"https://pith.science/paper/YVCTNK5I","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2311.16222&json=true","fetch_graph":"https://pith.science/api/pith-number/YVCTNK5ILNAHANBPQWBNRLNBQ2/graph.json","fetch_events":"https://pith.science/api/pith-number/YVCTNK5ILNAHANBPQWBNRLNBQ2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YVCTNK5ILNAHANBPQWBNRLNBQ2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YVCTNK5ILNAHANBPQWBNRLNBQ2/action/storage_attestation","attest_author":"https://pith.science/pith/YVCTNK5ILNAHANBPQWBNRLNBQ2/action/author_attestation","sign_citation":"https://pith.science/pith/YVCTNK5ILNAHANBPQWBNRLNBQ2/action/citation_signature","submit_replication":"https://pith.science/pith/YVCTNK5ILNAHANBPQWBNRLNBQ2/action/replication_record"}},"created_at":"2026-07-05T07:17:38.053953+00:00","updated_at":"2026-07-05T07:17:38.053953+00:00"}