{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:WRLQA54K3WBVF2ASD42SC7T52Q","short_pith_number":"pith:WRLQA54K","schema_version":"1.0","canonical_sha256":"b45700778add8352e8121f35217e7dd43294e4dec3ed509f9005a0d3ee63f35c","source":{"kind":"arxiv","id":"2504.13115","version":2},"attestation_state":"computed","paper":{"title":"Polarization Properties of the Electromagnetic Response to High-frequency Gravitational Wave","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Jian-Kang Li, Tong-Jie Zhang, Wei Hong","submitted_at":"2025-04-17T17:30:35Z","abstract_excerpt":"Electromagnetic waves (EMWs) can be generated by gravitational waves (GWs) within a magnetic field via the Gertsenshtein effect. The conversion probability between GWs and EMWs can be enhanced by inhomogeneities in the electron density and magnetic field within the magnetized plasma of both the Milky Way (MW) and the intergalactic medium in the expanding Universe. Polarized GWs can induce polarized EMWs, and the polarization properties of these EMWs can be altered by Faraday rotation as they propagate through magnetized plasma. Additionally, the polarization intensity of the EMWs may be weaken"},"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":"2504.13115","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2025-04-17T17:30:35Z","cross_cats_sorted":[],"title_canon_sha256":"5bd8baceee478a60d9e993b128be74a875385aa81dbdc60128a3e72e316c8408","abstract_canon_sha256":"42d831f399771fc743c1150c2b122499eff894c71fbdc914684a0029ce8797ce"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:16:57.469052Z","signature_b64":"KMtptloNP+reNCFx9rv2KfUqSr59eQUSa09MBmshbwqGuJjqB3QKsnH/0maQb5gTD7Pab3SQWbmoxCmcOTp/Ag==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b45700778add8352e8121f35217e7dd43294e4dec3ed509f9005a0d3ee63f35c","last_reissued_at":"2026-07-05T11:16:57.468543Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:16:57.468543Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Polarization Properties of the Electromagnetic Response to High-frequency Gravitational Wave","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Jian-Kang Li, Tong-Jie Zhang, Wei Hong","submitted_at":"2025-04-17T17:30:35Z","abstract_excerpt":"Electromagnetic waves (EMWs) can be generated by gravitational waves (GWs) within a magnetic field via the Gertsenshtein effect. The conversion probability between GWs and EMWs can be enhanced by inhomogeneities in the electron density and magnetic field within the magnetized plasma of both the Milky Way (MW) and the intergalactic medium in the expanding Universe. Polarized GWs can induce polarized EMWs, and the polarization properties of these EMWs can be altered by Faraday rotation as they propagate through magnetized plasma. Additionally, the polarization intensity of the EMWs may be weaken"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2504.13115","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/2504.13115/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":"2504.13115","created_at":"2026-07-05T11:16:57.468604+00:00"},{"alias_kind":"arxiv_version","alias_value":"2504.13115v2","created_at":"2026-07-05T11:16:57.468604+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2504.13115","created_at":"2026-07-05T11:16:57.468604+00:00"},{"alias_kind":"pith_short_12","alias_value":"WRLQA54K3WBV","created_at":"2026-07-05T11:16:57.468604+00:00"},{"alias_kind":"pith_short_16","alias_value":"WRLQA54K3WBVF2AS","created_at":"2026-07-05T11:16:57.468604+00:00"},{"alias_kind":"pith_short_8","alias_value":"WRLQA54K","created_at":"2026-07-05T11:16:57.468604+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":16,"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":56,"is_internal_anchor":false},{"citing_arxiv_id":"2605.28663","citing_title":"First-Order Perturbations of Covariant Maxwell Equations in Gravitational Waves","ref_index":44,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/WRLQA54K3WBVF2ASD42SC7T52Q","json":"https://pith.science/pith/WRLQA54K3WBVF2ASD42SC7T52Q.json","graph_json":"https://pith.science/api/pith-number/WRLQA54K3WBVF2ASD42SC7T52Q/graph.json","events_json":"https://pith.science/api/pith-number/WRLQA54K3WBVF2ASD42SC7T52Q/events.json","paper":"https://pith.science/paper/WRLQA54K"},"agent_actions":{"view_html":"https://pith.science/pith/WRLQA54K3WBVF2ASD42SC7T52Q","download_json":"https://pith.science/pith/WRLQA54K3WBVF2ASD42SC7T52Q.json","view_paper":"https://pith.science/paper/WRLQA54K","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2504.13115&json=true","fetch_graph":"https://pith.science/api/pith-number/WRLQA54K3WBVF2ASD42SC7T52Q/graph.json","fetch_events":"https://pith.science/api/pith-number/WRLQA54K3WBVF2ASD42SC7T52Q/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/WRLQA54K3WBVF2ASD42SC7T52Q/action/timestamp_anchor","attest_storage":"https://pith.science/pith/WRLQA54K3WBVF2ASD42SC7T52Q/action/storage_attestation","attest_author":"https://pith.science/pith/WRLQA54K3WBVF2ASD42SC7T52Q/action/author_attestation","sign_citation":"https://pith.science/pith/WRLQA54K3WBVF2ASD42SC7T52Q/action/citation_signature","submit_replication":"https://pith.science/pith/WRLQA54K3WBVF2ASD42SC7T52Q/action/replication_record"}},"created_at":"2026-07-05T11:16:57.468604+00:00","updated_at":"2026-07-05T11:16:57.468604+00:00"}