{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2007:YPU6I75I44GCSRHUAGKPNHDIYW","short_pith_number":"pith:YPU6I75I","schema_version":"1.0","canonical_sha256":"c3e9e47fa8e70c2944f40194f69c68c5b92cef405b87ce8fa4d2384c2da36fc3","source":{"kind":"arxiv","id":"0705.1733","version":3},"attestation_state":"computed","paper":{"title":"The Spectrum of Gravitational Radiation from Primordial Turbulence","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Arthur Kosowsky, Grigol Gogoberidze, Tina Kahniashvili","submitted_at":"2007-05-11T21:40:08Z","abstract_excerpt":"Energy injection into the early universe can induce turbulent motions of the primordial plasma, which in turn act as a source for gravitational radiation. Earlier work computed the amplitude and characteristic frequency of the relic gravitational wave background, as a function of the total energy injected and the stirring scale of the turbulence. This paper computes the frequency spectrum of relic gravitational radiation from a turbulent source of the stationary Kolmogoroff form which acts for a given duration, making no other approximations. We also show that the limit of long source waveleng"},"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":"0705.1733","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph","submitted_at":"2007-05-11T21:40:08Z","cross_cats_sorted":[],"title_canon_sha256":"7cd050233f1c91160742a96603a268a62a1fc7e953a4b219b2b2ba29d3b4a9a0","abstract_canon_sha256":"42b37a72e0c3c939caeff17b3f35a2ad28af1659cf1912a71de6c060f5d5ac4c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:41:50.987476Z","signature_b64":"26eRzCxXJJgf/qP8LxD9UWTcvH9MMNwtdoAhuE9x9PjGN63vtZQ3uPHOMrLSh1rEjtynYndT2lRGZLociBVfCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c3e9e47fa8e70c2944f40194f69c68c5b92cef405b87ce8fa4d2384c2da36fc3","last_reissued_at":"2026-07-04T15:41:50.987102Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:41:50.987102Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Spectrum of Gravitational Radiation from Primordial Turbulence","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Arthur Kosowsky, Grigol Gogoberidze, Tina Kahniashvili","submitted_at":"2007-05-11T21:40:08Z","abstract_excerpt":"Energy injection into the early universe can induce turbulent motions of the primordial plasma, which in turn act as a source for gravitational radiation. Earlier work computed the amplitude and characteristic frequency of the relic gravitational wave background, as a function of the total energy injected and the stirring scale of the turbulence. This paper computes the frequency spectrum of relic gravitational radiation from a turbulent source of the stationary Kolmogoroff form which acts for a given duration, making no other approximations. We also show that the limit of long source waveleng"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0705.1733","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/0705.1733/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":"0705.1733","created_at":"2026-07-04T15:41:50.987170+00:00"},{"alias_kind":"arxiv_version","alias_value":"0705.1733v3","created_at":"2026-07-04T15:41:50.987170+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0705.1733","created_at":"2026-07-04T15:41:50.987170+00:00"},{"alias_kind":"pith_short_12","alias_value":"YPU6I75I44GC","created_at":"2026-07-04T15:41:50.987170+00:00"},{"alias_kind":"pith_short_16","alias_value":"YPU6I75I44GCSRHU","created_at":"2026-07-04T15:41:50.987170+00:00"},{"alias_kind":"pith_short_8","alias_value":"YPU6I75I","created_at":"2026-07-04T15:41:50.987170+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":5,"internal_anchor_count":5,"sample":[{"citing_arxiv_id":"2605.27519","citing_title":"Probing Dynamical Inverse Seesaw with Low-frequency Gravitational Waves","ref_index":113,"is_internal_anchor":true},{"citing_arxiv_id":"1910.13125","citing_title":"Detecting gravitational waves from cosmological phase transitions with LISA: an update","ref_index":58,"is_internal_anchor":true},{"citing_arxiv_id":"2509.07070","citing_title":"Reviving WIMP dark matter with temperature-dependent couplings","ref_index":60,"is_internal_anchor":true},{"citing_arxiv_id":"2511.00996","citing_title":"Measuring gravitational wave spectrum from electroweak phase transition and Higgs self-couplings","ref_index":84,"is_internal_anchor":true},{"citing_arxiv_id":"1912.02622","citing_title":"Science Case for the Einstein Telescope","ref_index":225,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/YPU6I75I44GCSRHUAGKPNHDIYW","json":"https://pith.science/pith/YPU6I75I44GCSRHUAGKPNHDIYW.json","graph_json":"https://pith.science/api/pith-number/YPU6I75I44GCSRHUAGKPNHDIYW/graph.json","events_json":"https://pith.science/api/pith-number/YPU6I75I44GCSRHUAGKPNHDIYW/events.json","paper":"https://pith.science/paper/YPU6I75I"},"agent_actions":{"view_html":"https://pith.science/pith/YPU6I75I44GCSRHUAGKPNHDIYW","download_json":"https://pith.science/pith/YPU6I75I44GCSRHUAGKPNHDIYW.json","view_paper":"https://pith.science/paper/YPU6I75I","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0705.1733&json=true","fetch_graph":"https://pith.science/api/pith-number/YPU6I75I44GCSRHUAGKPNHDIYW/graph.json","fetch_events":"https://pith.science/api/pith-number/YPU6I75I44GCSRHUAGKPNHDIYW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YPU6I75I44GCSRHUAGKPNHDIYW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YPU6I75I44GCSRHUAGKPNHDIYW/action/storage_attestation","attest_author":"https://pith.science/pith/YPU6I75I44GCSRHUAGKPNHDIYW/action/author_attestation","sign_citation":"https://pith.science/pith/YPU6I75I44GCSRHUAGKPNHDIYW/action/citation_signature","submit_replication":"https://pith.science/pith/YPU6I75I44GCSRHUAGKPNHDIYW/action/replication_record"}},"created_at":"2026-07-04T15:41:50.987170+00:00","updated_at":"2026-07-04T15:41:50.987170+00:00"}