{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:TSDPGAR4YPKE5SP3XMC75WSXQV","short_pith_number":"pith:TSDPGAR4","schema_version":"1.0","canonical_sha256":"9c86f3023cc3d44ec9fbbb05feda57857a0d0b969e28bfdbbd87296dd1c3eafa","source":{"kind":"arxiv","id":"2402.14092","version":2},"attestation_state":"computed","paper":{"title":"High Frequency Gravitational Wave Bounds from Galactic Neutron Stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-ph"],"primary_cat":"gr-qc","authors_text":"Francesco Costa, Toni Bert\\'olez-Mart\\'inez, Virgile Dandoy","submitted_at":"2024-02-21T19:39:56Z","abstract_excerpt":"High-Frequency Gravitational Waves (HFGWs) constitute a unique window on the early Universe as well as exotic astrophysical objects. If the current gravitational wave experiments are more dedicated to the low frequency regime, the graviton conversion into photons in a strong magnetic field constitutes a powerful tool to probe HFGWs. In this paper, we show that neutron stars, due to their extreme magnetic field, are a perfect laboratory to study the conversion of HFGWs into photons. Using realistic models for the galactic neutron star population, we calculate for the first time the expected pho"},"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":"2402.14092","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2024-02-21T19:39:56Z","cross_cats_sorted":["astro-ph.HE","hep-ph"],"title_canon_sha256":"68b09ca595f0d71e2f04ee9e15f1a8ac8ef4ed5e0fef02cf6927a5af6116ca55","abstract_canon_sha256":"ff32e4f06feed393848aa634e2db20088dd93c343766ef7d34d328e90f670fbb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:06:03.075542Z","signature_b64":"zEZkrnQdzhMsGOu5H2BiStHnNWFKdRsdY1R2GqNwcugH69FB2yXPzSfAjIS+vBPMXRSKUiNTD3aK3UCHnVmCAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9c86f3023cc3d44ec9fbbb05feda57857a0d0b969e28bfdbbd87296dd1c3eafa","last_reissued_at":"2026-07-05T10:06:03.075055Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:06:03.075055Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"High Frequency Gravitational Wave Bounds from Galactic Neutron Stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-ph"],"primary_cat":"gr-qc","authors_text":"Francesco Costa, Toni Bert\\'olez-Mart\\'inez, Virgile Dandoy","submitted_at":"2024-02-21T19:39:56Z","abstract_excerpt":"High-Frequency Gravitational Waves (HFGWs) constitute a unique window on the early Universe as well as exotic astrophysical objects. If the current gravitational wave experiments are more dedicated to the low frequency regime, the graviton conversion into photons in a strong magnetic field constitutes a powerful tool to probe HFGWs. In this paper, we show that neutron stars, due to their extreme magnetic field, are a perfect laboratory to study the conversion of HFGWs into photons. Using realistic models for the galactic neutron star population, we calculate for the first time the expected pho"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2402.14092","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/2402.14092/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":"2402.14092","created_at":"2026-07-05T10:06:03.075109+00:00"},{"alias_kind":"arxiv_version","alias_value":"2402.14092v2","created_at":"2026-07-05T10:06:03.075109+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2402.14092","created_at":"2026-07-05T10:06:03.075109+00:00"},{"alias_kind":"pith_short_12","alias_value":"TSDPGAR4YPKE","created_at":"2026-07-05T10:06:03.075109+00:00"},{"alias_kind":"pith_short_16","alias_value":"TSDPGAR4YPKE5SP3","created_at":"2026-07-05T10:06:03.075109+00:00"},{"alias_kind":"pith_short_8","alias_value":"TSDPGAR4","created_at":"2026-07-05T10:06:03.075109+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.19757","citing_title":"Graviton Floor","ref_index":11,"is_internal_anchor":false},{"citing_arxiv_id":"2606.13642","citing_title":"Search for High-Frequency Gravitational Waves via Geomagnetic Conversion with Radio Telescopes","ref_index":61,"is_internal_anchor":false},{"citing_arxiv_id":"2606.12546","citing_title":"Polarization Formalism for Photon-Gravitational Wave Mixing Around Magnetars","ref_index":46,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TSDPGAR4YPKE5SP3XMC75WSXQV","json":"https://pith.science/pith/TSDPGAR4YPKE5SP3XMC75WSXQV.json","graph_json":"https://pith.science/api/pith-number/TSDPGAR4YPKE5SP3XMC75WSXQV/graph.json","events_json":"https://pith.science/api/pith-number/TSDPGAR4YPKE5SP3XMC75WSXQV/events.json","paper":"https://pith.science/paper/TSDPGAR4"},"agent_actions":{"view_html":"https://pith.science/pith/TSDPGAR4YPKE5SP3XMC75WSXQV","download_json":"https://pith.science/pith/TSDPGAR4YPKE5SP3XMC75WSXQV.json","view_paper":"https://pith.science/paper/TSDPGAR4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2402.14092&json=true","fetch_graph":"https://pith.science/api/pith-number/TSDPGAR4YPKE5SP3XMC75WSXQV/graph.json","fetch_events":"https://pith.science/api/pith-number/TSDPGAR4YPKE5SP3XMC75WSXQV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TSDPGAR4YPKE5SP3XMC75WSXQV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TSDPGAR4YPKE5SP3XMC75WSXQV/action/storage_attestation","attest_author":"https://pith.science/pith/TSDPGAR4YPKE5SP3XMC75WSXQV/action/author_attestation","sign_citation":"https://pith.science/pith/TSDPGAR4YPKE5SP3XMC75WSXQV/action/citation_signature","submit_replication":"https://pith.science/pith/TSDPGAR4YPKE5SP3XMC75WSXQV/action/replication_record"}},"created_at":"2026-07-05T10:06:03.075109+00:00","updated_at":"2026-07-05T10:06:03.075109+00:00"}