{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:ZTRUPYJXPTR5KEAFJGXOKXUHBL","short_pith_number":"pith:ZTRUPYJX","schema_version":"1.0","canonical_sha256":"cce347e1377ce3d5100549aee55e870acd20f2bd3aa3a559f9ef6c7da948de42","source":{"kind":"arxiv","id":"1809.04994","version":1},"attestation_state":"computed","paper":{"title":"Fingerprinting models of first-order phase transitions by the synergy between collider and gravitational-wave experiments","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Katsuya Hashino, Masahiro Takimoto, Mitsuru Kakizaki, Ryusuke Jinno, Shinya Kanemura, Tomo Takahashi","submitted_at":"2018-09-13T14:45:02Z","abstract_excerpt":"We investigate the sensitivity of future space-based interferometers such as LISA and DECIGO to the parameters of new particle physics models which drive a first-order phase transition in the early Universe. We first perform a Fisher matrix analysis on the quantities characterizing the gravitational wave spectrum resulting from the phase transition, such as the peak frequency and amplitude. We next perform a Fisher analysis for the quantities which determine the properties of the phase transition, such as the latent heat and the time dependence of the bubble nucleation rate. Since these quanti"},"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":"1809.04994","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2018-09-13T14:45:02Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"34f712619b79a3578aee7a3b70587354647df3044b047a95c83dc5648ed20505","abstract_canon_sha256":"128eaa3d7208df51edf3d3faf745bd7fce6c25ea7ad77f19b19b687c8e5f8468"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:48:33.836941Z","signature_b64":"wKx7WNI+rdme5f/Vd97ysCohcnBAg4JhtKhKfev/X+A+Kq6XIh4UlnaIFJyTBvnc+44W34roNhg5RqIV5G76Cg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cce347e1377ce3d5100549aee55e870acd20f2bd3aa3a559f9ef6c7da948de42","last_reissued_at":"2026-05-17T23:48:33.836301Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:48:33.836301Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Fingerprinting models of first-order phase transitions by the synergy between collider and gravitational-wave experiments","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Katsuya Hashino, Masahiro Takimoto, Mitsuru Kakizaki, Ryusuke Jinno, Shinya Kanemura, Tomo Takahashi","submitted_at":"2018-09-13T14:45:02Z","abstract_excerpt":"We investigate the sensitivity of future space-based interferometers such as LISA and DECIGO to the parameters of new particle physics models which drive a first-order phase transition in the early Universe. We first perform a Fisher matrix analysis on the quantities characterizing the gravitational wave spectrum resulting from the phase transition, such as the peak frequency and amplitude. We next perform a Fisher analysis for the quantities which determine the properties of the phase transition, such as the latent heat and the time dependence of the bubble nucleation rate. Since these quanti"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1809.04994","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":""},"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":"1809.04994","created_at":"2026-05-17T23:48:33.836409+00:00"},{"alias_kind":"arxiv_version","alias_value":"1809.04994v1","created_at":"2026-05-17T23:48:33.836409+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1809.04994","created_at":"2026-05-17T23:48:33.836409+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZTRUPYJXPTR5","created_at":"2026-05-18T12:33:07.085635+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZTRUPYJXPTR5KEAF","created_at":"2026-05-18T12:33:07.085635+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZTRUPYJX","created_at":"2026-05-18T12:33:07.085635+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2002.04615","citing_title":"New Sensitivity Curves for Gravitational-Wave Signals from Cosmological Phase Transitions","ref_index":87,"is_internal_anchor":true},{"citing_arxiv_id":"2604.21492","citing_title":"Solving Cosmological Puzzles using Finite Temperature $\\nu$SMEFT","ref_index":40,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/ZTRUPYJXPTR5KEAFJGXOKXUHBL","json":"https://pith.science/pith/ZTRUPYJXPTR5KEAFJGXOKXUHBL.json","graph_json":"https://pith.science/api/pith-number/ZTRUPYJXPTR5KEAFJGXOKXUHBL/graph.json","events_json":"https://pith.science/api/pith-number/ZTRUPYJXPTR5KEAFJGXOKXUHBL/events.json","paper":"https://pith.science/paper/ZTRUPYJX"},"agent_actions":{"view_html":"https://pith.science/pith/ZTRUPYJXPTR5KEAFJGXOKXUHBL","download_json":"https://pith.science/pith/ZTRUPYJXPTR5KEAFJGXOKXUHBL.json","view_paper":"https://pith.science/paper/ZTRUPYJX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1809.04994&json=true","fetch_graph":"https://pith.science/api/pith-number/ZTRUPYJXPTR5KEAFJGXOKXUHBL/graph.json","fetch_events":"https://pith.science/api/pith-number/ZTRUPYJXPTR5KEAFJGXOKXUHBL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZTRUPYJXPTR5KEAFJGXOKXUHBL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZTRUPYJXPTR5KEAFJGXOKXUHBL/action/storage_attestation","attest_author":"https://pith.science/pith/ZTRUPYJXPTR5KEAFJGXOKXUHBL/action/author_attestation","sign_citation":"https://pith.science/pith/ZTRUPYJXPTR5KEAFJGXOKXUHBL/action/citation_signature","submit_replication":"https://pith.science/pith/ZTRUPYJXPTR5KEAFJGXOKXUHBL/action/replication_record"}},"created_at":"2026-05-17T23:48:33.836409+00:00","updated_at":"2026-05-17T23:48:33.836409+00:00"}