{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:47YPDGIT4AMPJM2RGQQZ7VFYLK","short_pith_number":"pith:47YPDGIT","schema_version":"1.0","canonical_sha256":"e7f0f19913e018f4b35134219fd4b85abe19b53fa66f5a002246daab1d96aa2f","source":{"kind":"arxiv","id":"1912.00785","version":3},"attestation_state":"computed","paper":{"title":"Gauge Independence of Induced Gravitational Waves","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph"],"primary_cat":"gr-qc","authors_text":"Keisuke Inomata, Takahiro Terada","submitted_at":"2019-12-02T13:53:09Z","abstract_excerpt":"We study gauge (in)dependence of the gravitational waves (GWs) induced from curvature perturbations. For the GWs produced in a radiation-dominated era, we find that the observable (late-time) GWs in the TT gauge and in the Newtonian gauge are the same in contrast to a claim in the literature. We also mention the interpretation of the gauge dependence of the tensor perturbations which appears in the context of the induced GWs."},"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":"1912.00785","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2019-12-02T13:53:09Z","cross_cats_sorted":["astro-ph.CO","hep-ph"],"title_canon_sha256":"ca3a3fed081c4d3be3b37aafcc23b319462b501f1bd1baa6a1fd662aba420383","abstract_canon_sha256":"09d11fe055c103b5ef081e34762c845b1c2195a25b64dba6f83d3dfbf7487425"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:36:43.925944Z","signature_b64":"26gekUNE+Dc93Y1q+ASiYdoonPKricEA08kvT4LWFy5xthGK2uPTx0a+6sRzW/74ssigA5FaoA2lkYaTzP/ZBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e7f0f19913e018f4b35134219fd4b85abe19b53fa66f5a002246daab1d96aa2f","last_reissued_at":"2026-07-05T00:36:43.925511Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:36:43.925511Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gauge Independence of Induced Gravitational Waves","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph"],"primary_cat":"gr-qc","authors_text":"Keisuke Inomata, Takahiro Terada","submitted_at":"2019-12-02T13:53:09Z","abstract_excerpt":"We study gauge (in)dependence of the gravitational waves (GWs) induced from curvature perturbations. For the GWs produced in a radiation-dominated era, we find that the observable (late-time) GWs in the TT gauge and in the Newtonian gauge are the same in contrast to a claim in the literature. We also mention the interpretation of the gauge dependence of the tensor perturbations which appears in the context of the induced GWs."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1912.00785","kind":"arxiv","version":3},"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/1912.00785/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":"1912.00785","created_at":"2026-07-05T00:36:43.925566+00:00"},{"alias_kind":"arxiv_version","alias_value":"1912.00785v3","created_at":"2026-07-05T00:36:43.925566+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1912.00785","created_at":"2026-07-05T00:36:43.925566+00:00"},{"alias_kind":"pith_short_12","alias_value":"47YPDGIT4AMP","created_at":"2026-07-05T00:36:43.925566+00:00"},{"alias_kind":"pith_short_16","alias_value":"47YPDGIT4AMPJM2R","created_at":"2026-07-05T00:36:43.925566+00:00"},{"alias_kind":"pith_short_8","alias_value":"47YPDGIT","created_at":"2026-07-05T00:36:43.925566+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2507.09552","citing_title":"Probing the scalar-induced gravitational waves with the Five-hundred-meter Aperture Spherical radio Telescope and the Square Kilometer Array","ref_index":71,"is_internal_anchor":false},{"citing_arxiv_id":"2109.01398","citing_title":"Scalar induced gravitational waves review","ref_index":154,"is_internal_anchor":false},{"citing_arxiv_id":"2604.20063","citing_title":"Purely quadratic non-Gaussianity from tachyonic instability: Primordial black holes and scalar-induced gravitational waves","ref_index":156,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/47YPDGIT4AMPJM2RGQQZ7VFYLK","json":"https://pith.science/pith/47YPDGIT4AMPJM2RGQQZ7VFYLK.json","graph_json":"https://pith.science/api/pith-number/47YPDGIT4AMPJM2RGQQZ7VFYLK/graph.json","events_json":"https://pith.science/api/pith-number/47YPDGIT4AMPJM2RGQQZ7VFYLK/events.json","paper":"https://pith.science/paper/47YPDGIT"},"agent_actions":{"view_html":"https://pith.science/pith/47YPDGIT4AMPJM2RGQQZ7VFYLK","download_json":"https://pith.science/pith/47YPDGIT4AMPJM2RGQQZ7VFYLK.json","view_paper":"https://pith.science/paper/47YPDGIT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1912.00785&json=true","fetch_graph":"https://pith.science/api/pith-number/47YPDGIT4AMPJM2RGQQZ7VFYLK/graph.json","fetch_events":"https://pith.science/api/pith-number/47YPDGIT4AMPJM2RGQQZ7VFYLK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/47YPDGIT4AMPJM2RGQQZ7VFYLK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/47YPDGIT4AMPJM2RGQQZ7VFYLK/action/storage_attestation","attest_author":"https://pith.science/pith/47YPDGIT4AMPJM2RGQQZ7VFYLK/action/author_attestation","sign_citation":"https://pith.science/pith/47YPDGIT4AMPJM2RGQQZ7VFYLK/action/citation_signature","submit_replication":"https://pith.science/pith/47YPDGIT4AMPJM2RGQQZ7VFYLK/action/replication_record"}},"created_at":"2026-07-05T00:36:43.925566+00:00","updated_at":"2026-07-05T00:36:43.925566+00:00"}