{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:AGEQFETUCBHCVEKY5E74Y4UFQZ","short_pith_number":"pith:AGEQFETU","schema_version":"1.0","canonical_sha256":"0189029274104e2a9158e93fcc7285864b0592a8efb82a0645bc50f2131c429d","source":{"kind":"arxiv","id":"2312.16316","version":1},"attestation_state":"computed","paper":{"title":"Imprints of primordial magnetic fields on intrinsic alignments of galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.CO","authors_text":"Kazuyuki Akitsu, Maresuke Shiraishi, Shohei Saga, Teppei Okumura","submitted_at":"2023-12-26T19:49:43Z","abstract_excerpt":"Primordial magnetic fields (PMFs) are one of the plausible candidates for the origin of the observed large-scale magnetic fields. While many proposals have been made for the generation mechanism of PMFs by earlier studies, it remains a subject of debate. In this paper, to obtain new insights into PMFs, we focus on the intrinsic alignments (IAs) of galaxies induced by the vector and tensor modes of the anisotropic stress of PMFs. The long-wavelength vector and tensor modes locally induce the tidal gravitational fields, leading to the characteristic distortions of the intrinsic ellipticity of ga"},"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":"2312.16316","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2023-12-26T19:49:43Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"876060165f17d9ca08b98c608dfd1eaa724874a438e3a05a2a0e9fc7bc0db5fa","abstract_canon_sha256":"583e4e8d303ce2985bbe44f0887aed5dbb7e1dcfaade192a57b226a1b1eb91b8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:06:45.583208Z","signature_b64":"vO4u6zScWFXwijW+EjWvubzZYm2poMhoWeRikRBlG+QTol+8eaiP60cUR8c6gZhuwwvL9WhPdiHvdolOEhkWCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0189029274104e2a9158e93fcc7285864b0592a8efb82a0645bc50f2131c429d","last_reissued_at":"2026-07-05T08:06:45.582640Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:06:45.582640Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Imprints of primordial magnetic fields on intrinsic alignments of galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.CO","authors_text":"Kazuyuki Akitsu, Maresuke Shiraishi, Shohei Saga, Teppei Okumura","submitted_at":"2023-12-26T19:49:43Z","abstract_excerpt":"Primordial magnetic fields (PMFs) are one of the plausible candidates for the origin of the observed large-scale magnetic fields. While many proposals have been made for the generation mechanism of PMFs by earlier studies, it remains a subject of debate. In this paper, to obtain new insights into PMFs, we focus on the intrinsic alignments (IAs) of galaxies induced by the vector and tensor modes of the anisotropic stress of PMFs. The long-wavelength vector and tensor modes locally induce the tidal gravitational fields, leading to the characteristic distortions of the intrinsic ellipticity of ga"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2312.16316","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2312.16316/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":"2312.16316","created_at":"2026-07-05T08:06:45.582706+00:00"},{"alias_kind":"arxiv_version","alias_value":"2312.16316v1","created_at":"2026-07-05T08:06:45.582706+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2312.16316","created_at":"2026-07-05T08:06:45.582706+00:00"},{"alias_kind":"pith_short_12","alias_value":"AGEQFETUCBHC","created_at":"2026-07-05T08:06:45.582706+00:00"},{"alias_kind":"pith_short_16","alias_value":"AGEQFETUCBHCVEKY","created_at":"2026-07-05T08:06:45.582706+00:00"},{"alias_kind":"pith_short_8","alias_value":"AGEQFETU","created_at":"2026-07-05T08:06:45.582706+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.25171","citing_title":"Symbiotic Magnetogenesis during Radiation Domination","ref_index":60,"is_internal_anchor":false},{"citing_arxiv_id":"2605.13016","citing_title":"Revisiting constraints on primordial vector modes and implications for sourced magnetic fields and observed $EB$ power spectrum","ref_index":8,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/AGEQFETUCBHCVEKY5E74Y4UFQZ","json":"https://pith.science/pith/AGEQFETUCBHCVEKY5E74Y4UFQZ.json","graph_json":"https://pith.science/api/pith-number/AGEQFETUCBHCVEKY5E74Y4UFQZ/graph.json","events_json":"https://pith.science/api/pith-number/AGEQFETUCBHCVEKY5E74Y4UFQZ/events.json","paper":"https://pith.science/paper/AGEQFETU"},"agent_actions":{"view_html":"https://pith.science/pith/AGEQFETUCBHCVEKY5E74Y4UFQZ","download_json":"https://pith.science/pith/AGEQFETUCBHCVEKY5E74Y4UFQZ.json","view_paper":"https://pith.science/paper/AGEQFETU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2312.16316&json=true","fetch_graph":"https://pith.science/api/pith-number/AGEQFETUCBHCVEKY5E74Y4UFQZ/graph.json","fetch_events":"https://pith.science/api/pith-number/AGEQFETUCBHCVEKY5E74Y4UFQZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AGEQFETUCBHCVEKY5E74Y4UFQZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AGEQFETUCBHCVEKY5E74Y4UFQZ/action/storage_attestation","attest_author":"https://pith.science/pith/AGEQFETUCBHCVEKY5E74Y4UFQZ/action/author_attestation","sign_citation":"https://pith.science/pith/AGEQFETUCBHCVEKY5E74Y4UFQZ/action/citation_signature","submit_replication":"https://pith.science/pith/AGEQFETUCBHCVEKY5E74Y4UFQZ/action/replication_record"}},"created_at":"2026-07-05T08:06:45.582706+00:00","updated_at":"2026-07-05T08:06:45.582706+00:00"}