{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:LMXVEGBMIPUYSOE336IIVARQOH","short_pith_number":"pith:LMXVEGBM","schema_version":"1.0","canonical_sha256":"5b2f52182c43e989389bdf908a823071c9f650a069b71b36d22ce46f35961e59","source":{"kind":"arxiv","id":"2112.14588","version":3},"attestation_state":"computed","paper":{"title":"Correlated signals of first-order phase transitions and primordial black hole evaporation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ex"],"primary_cat":"hep-ph","authors_text":"Danny Marfatia, Po-Yan Tseng","submitted_at":"2021-12-29T14:59:28Z","abstract_excerpt":"Fermi balls produced in a cosmological first-order phase transition may collapse to primordial black holes (PBHs) if the fermion dark matter particles that comprise them interact via a sufficiently strong Yukawa force. We show that phase transitions described by a quartic thermal effective potential with vacuum energy, $0.1\\lesssim B^{1/4}/{\\rm MeV} \\lesssim 10^3$, generate PBHs of mass, $10^{-20}\\lesssim M_{\\rm PBH}/M_\\odot \\lesssim 10^{-16}$, and gravitational waves from the phase transition (at THEIA/$\\mu$Ares) can be correlated with an isotropic extragalactic X-ray/$\\gamma$-ray background "},"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":"2112.14588","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2021-12-29T14:59:28Z","cross_cats_sorted":["astro-ph.CO","hep-ex"],"title_canon_sha256":"7666bc5f61bcbdd2b63e401575bcc370e16e5f654d328827825da9a0c9893b81","abstract_canon_sha256":"a921d43f02fc934117792382645754f8ecd46e049c91bc8aa2c601f4ec31b444"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:46:34.564244Z","signature_b64":"t1+WFuaj/XMQquDhlcPUGmi0nIsorum/FLpslMe8Xbd/KZpwQ6Ibj6Nq4ZsMzmgaQRwABbd8mbTQZBgvVTPYDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5b2f52182c43e989389bdf908a823071c9f650a069b71b36d22ce46f35961e59","last_reissued_at":"2026-07-05T04:46:34.563831Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:46:34.563831Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Correlated signals of first-order phase transitions and primordial black hole evaporation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ex"],"primary_cat":"hep-ph","authors_text":"Danny Marfatia, Po-Yan Tseng","submitted_at":"2021-12-29T14:59:28Z","abstract_excerpt":"Fermi balls produced in a cosmological first-order phase transition may collapse to primordial black holes (PBHs) if the fermion dark matter particles that comprise them interact via a sufficiently strong Yukawa force. We show that phase transitions described by a quartic thermal effective potential with vacuum energy, $0.1\\lesssim B^{1/4}/{\\rm MeV} \\lesssim 10^3$, generate PBHs of mass, $10^{-20}\\lesssim M_{\\rm PBH}/M_\\odot \\lesssim 10^{-16}$, and gravitational waves from the phase transition (at THEIA/$\\mu$Ares) can be correlated with an isotropic extragalactic X-ray/$\\gamma$-ray background "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2112.14588","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/2112.14588/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":"2112.14588","created_at":"2026-07-05T04:46:34.563887+00:00"},{"alias_kind":"arxiv_version","alias_value":"2112.14588v3","created_at":"2026-07-05T04:46:34.563887+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2112.14588","created_at":"2026-07-05T04:46:34.563887+00:00"},{"alias_kind":"pith_short_12","alias_value":"LMXVEGBMIPUY","created_at":"2026-07-05T04:46:34.563887+00:00"},{"alias_kind":"pith_short_16","alias_value":"LMXVEGBMIPUYSOE3","created_at":"2026-07-05T04:46:34.563887+00:00"},{"alias_kind":"pith_short_8","alias_value":"LMXVEGBM","created_at":"2026-07-05T04:46:34.563887+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2511.01848","citing_title":"Constraining memory-burdened primordial black holes with graviton-photon conversion and binary mergers","ref_index":24,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LMXVEGBMIPUYSOE336IIVARQOH","json":"https://pith.science/pith/LMXVEGBMIPUYSOE336IIVARQOH.json","graph_json":"https://pith.science/api/pith-number/LMXVEGBMIPUYSOE336IIVARQOH/graph.json","events_json":"https://pith.science/api/pith-number/LMXVEGBMIPUYSOE336IIVARQOH/events.json","paper":"https://pith.science/paper/LMXVEGBM"},"agent_actions":{"view_html":"https://pith.science/pith/LMXVEGBMIPUYSOE336IIVARQOH","download_json":"https://pith.science/pith/LMXVEGBMIPUYSOE336IIVARQOH.json","view_paper":"https://pith.science/paper/LMXVEGBM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2112.14588&json=true","fetch_graph":"https://pith.science/api/pith-number/LMXVEGBMIPUYSOE336IIVARQOH/graph.json","fetch_events":"https://pith.science/api/pith-number/LMXVEGBMIPUYSOE336IIVARQOH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LMXVEGBMIPUYSOE336IIVARQOH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LMXVEGBMIPUYSOE336IIVARQOH/action/storage_attestation","attest_author":"https://pith.science/pith/LMXVEGBMIPUYSOE336IIVARQOH/action/author_attestation","sign_citation":"https://pith.science/pith/LMXVEGBMIPUYSOE336IIVARQOH/action/citation_signature","submit_replication":"https://pith.science/pith/LMXVEGBMIPUYSOE336IIVARQOH/action/replication_record"}},"created_at":"2026-07-05T04:46:34.563887+00:00","updated_at":"2026-07-05T04:46:34.563887+00:00"}