{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:TNCRWRIEKPPNGONQOWRR2QTUNZ","short_pith_number":"pith:TNCRWRIE","schema_version":"1.0","canonical_sha256":"9b451b450453ded339b075a31d42746e5518d40e323ceff129a5ee843bcbff21","source":{"kind":"arxiv","id":"2310.13060","version":2},"attestation_state":"computed","paper":{"title":"Gravitational Wave Symphony from Oscillating Spectator Scalar Fields","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc"],"primary_cat":"hep-ph","authors_text":"Evangelos I. Sfakianakis, Pankaj Saha, Yanou Cui","submitted_at":"2023-10-19T18:00:45Z","abstract_excerpt":"We investigate a generic source of stochastic gravitational wave background due to the parametric resonance of oscillating scalar fields in the early Universe. By systematically analyzing benchmark models through lattice simulations and considering a wide range of parameters, we demonstrate that such a scenario can lead to detectable signals in gravitational wave detectors over a broad frequency range and potentially address the recent findings by pulsar timing array experiments. Furthermore, these models naturally yield ultralight dark matter candidates or dark radiation detectable by cosmic "},"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":"2310.13060","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2023-10-19T18:00:45Z","cross_cats_sorted":["astro-ph.CO","gr-qc"],"title_canon_sha256":"6717618556e257a0d3154f5bedda6df14be3ea19b19336adf1e2986fdee8cff0","abstract_canon_sha256":"30b4c79be01c8c91765b228836ab715dc77889d13e4dcf3a71f95f4f2966657b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:45:22.915448Z","signature_b64":"GomaS3b6nSGkddIkOJ7QMEhtO4RDqiR1N7t/Mr09mxL7dxgh7lm19YeaN0Nf8NvT+IqsgCS+8z25WSgJaw5ADA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9b451b450453ded339b075a31d42746e5518d40e323ceff129a5ee843bcbff21","last_reissued_at":"2026-07-05T08:45:22.915028Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:45:22.915028Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gravitational Wave Symphony from Oscillating Spectator Scalar Fields","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc"],"primary_cat":"hep-ph","authors_text":"Evangelos I. Sfakianakis, Pankaj Saha, Yanou Cui","submitted_at":"2023-10-19T18:00:45Z","abstract_excerpt":"We investigate a generic source of stochastic gravitational wave background due to the parametric resonance of oscillating scalar fields in the early Universe. By systematically analyzing benchmark models through lattice simulations and considering a wide range of parameters, we demonstrate that such a scenario can lead to detectable signals in gravitational wave detectors over a broad frequency range and potentially address the recent findings by pulsar timing array experiments. Furthermore, these models naturally yield ultralight dark matter candidates or dark radiation detectable by cosmic "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2310.13060","kind":"arxiv","version":2},"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/2310.13060/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":"2310.13060","created_at":"2026-07-05T08:45:22.915081+00:00"},{"alias_kind":"arxiv_version","alias_value":"2310.13060v2","created_at":"2026-07-05T08:45:22.915081+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2310.13060","created_at":"2026-07-05T08:45:22.915081+00:00"},{"alias_kind":"pith_short_12","alias_value":"TNCRWRIEKPPN","created_at":"2026-07-05T08:45:22.915081+00:00"},{"alias_kind":"pith_short_16","alias_value":"TNCRWRIEKPPNGONQ","created_at":"2026-07-05T08:45:22.915081+00:00"},{"alias_kind":"pith_short_8","alias_value":"TNCRWRIE","created_at":"2026-07-05T08:45:22.915081+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.21092","citing_title":"Audible Axion Magnetogenesis: Linking Intergalactic Magnetic Fields and Gravitational Waves","ref_index":52,"is_internal_anchor":false},{"citing_arxiv_id":"2510.05967","citing_title":"Stochastic Gravitational Waves from Modulated Reheating","ref_index":55,"is_internal_anchor":false},{"citing_arxiv_id":"2604.05078","citing_title":"Gravitational Waves from Matter Perturbations of Spectator Scalar Fields","ref_index":49,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TNCRWRIEKPPNGONQOWRR2QTUNZ","json":"https://pith.science/pith/TNCRWRIEKPPNGONQOWRR2QTUNZ.json","graph_json":"https://pith.science/api/pith-number/TNCRWRIEKPPNGONQOWRR2QTUNZ/graph.json","events_json":"https://pith.science/api/pith-number/TNCRWRIEKPPNGONQOWRR2QTUNZ/events.json","paper":"https://pith.science/paper/TNCRWRIE"},"agent_actions":{"view_html":"https://pith.science/pith/TNCRWRIEKPPNGONQOWRR2QTUNZ","download_json":"https://pith.science/pith/TNCRWRIEKPPNGONQOWRR2QTUNZ.json","view_paper":"https://pith.science/paper/TNCRWRIE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2310.13060&json=true","fetch_graph":"https://pith.science/api/pith-number/TNCRWRIEKPPNGONQOWRR2QTUNZ/graph.json","fetch_events":"https://pith.science/api/pith-number/TNCRWRIEKPPNGONQOWRR2QTUNZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TNCRWRIEKPPNGONQOWRR2QTUNZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TNCRWRIEKPPNGONQOWRR2QTUNZ/action/storage_attestation","attest_author":"https://pith.science/pith/TNCRWRIEKPPNGONQOWRR2QTUNZ/action/author_attestation","sign_citation":"https://pith.science/pith/TNCRWRIEKPPNGONQOWRR2QTUNZ/action/citation_signature","submit_replication":"https://pith.science/pith/TNCRWRIEKPPNGONQOWRR2QTUNZ/action/replication_record"}},"created_at":"2026-07-05T08:45:22.915081+00:00","updated_at":"2026-07-05T08:45:22.915081+00:00"}