{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2004:DHGX2ZG66CMKGWORIFNYE5AYWR","short_pith_number":"pith:DHGX2ZG6","schema_version":"1.0","canonical_sha256":"19cd7d64def098a359d1415b827418b47317edcb1e56b1e95f7af245f59cc5fa","source":{"kind":"arxiv","id":"astro-ph/0410395","version":2},"attestation_state":"computed","paper":{"title":"Neutrino Emission from Ungapped Quark Matter","license":"","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph","authors_text":"Kai Schwenzer, Thomas Schafer","submitted_at":"2004-10-15T20:02:37Z","abstract_excerpt":"We study neutrino emission from a normal, ungapped, quark phase in the core of a compact star. Neutrino emission from non-interacting quark matter leads to an emissivity that scales as $\\epsilon\\sim T^7$. We show that the emissivity is enhanced by a combination of Fermi liquid and non-Fermi liquid effects. Fermi liquid effects lead to an emissivity that scales as $\\epsilon\\sim \\alpha_s T^6$, as originally shown by Iwamoto. We demonstrate that non-Fermi liquid effects further enhance the rate, leading to $\\epsilon\\sim \\alpha_s^3 T^6\\log(m/T)^2$, where $m$ is the electric screening scale and $m\\"},"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":"astro-ph/0410395","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2004-10-15T20:02:37Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"57b9d77701b7483b622d8a24c835185fecc47ff8f080d322e4491b33e0fb6bd1","abstract_canon_sha256":"582fce11f3d6f73d9b3bdef43afbf9701bc2406a82e1d6cc6e8c82d610085d01"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:44:59.270109Z","signature_b64":"NIxpFsbVPSXDYHBeTkuNfa3IgpWVgk+xlthi7UQYAr1LTxcTHBsUWZBU/S6tKpSb1m7bY6w1CLotf/Ymdh1EBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"19cd7d64def098a359d1415b827418b47317edcb1e56b1e95f7af245f59cc5fa","last_reissued_at":"2026-07-04T16:44:59.269768Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:44:59.269768Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Neutrino Emission from Ungapped Quark Matter","license":"","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph","authors_text":"Kai Schwenzer, Thomas Schafer","submitted_at":"2004-10-15T20:02:37Z","abstract_excerpt":"We study neutrino emission from a normal, ungapped, quark phase in the core of a compact star. Neutrino emission from non-interacting quark matter leads to an emissivity that scales as $\\epsilon\\sim T^7$. We show that the emissivity is enhanced by a combination of Fermi liquid and non-Fermi liquid effects. Fermi liquid effects lead to an emissivity that scales as $\\epsilon\\sim \\alpha_s T^6$, as originally shown by Iwamoto. We demonstrate that non-Fermi liquid effects further enhance the rate, leading to $\\epsilon\\sim \\alpha_s^3 T^6\\log(m/T)^2$, where $m$ is the electric screening scale and $m\\"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0410395","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/astro-ph/0410395/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":"astro-ph/0410395","created_at":"2026-07-04T16:44:59.269829+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0410395v2","created_at":"2026-07-04T16:44:59.269829+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0410395","created_at":"2026-07-04T16:44:59.269829+00:00"},{"alias_kind":"pith_short_12","alias_value":"DHGX2ZG66CMK","created_at":"2026-07-04T16:44:59.269829+00:00"},{"alias_kind":"pith_short_16","alias_value":"DHGX2ZG66CMKGWOR","created_at":"2026-07-04T16:44:59.269829+00:00"},{"alias_kind":"pith_short_8","alias_value":"DHGX2ZG6","created_at":"2026-07-04T16:44:59.269829+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2501.03318","citing_title":"Neutrino energy and momentum emission from magnetized dense quark matter","ref_index":23,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/DHGX2ZG66CMKGWORIFNYE5AYWR","json":"https://pith.science/pith/DHGX2ZG66CMKGWORIFNYE5AYWR.json","graph_json":"https://pith.science/api/pith-number/DHGX2ZG66CMKGWORIFNYE5AYWR/graph.json","events_json":"https://pith.science/api/pith-number/DHGX2ZG66CMKGWORIFNYE5AYWR/events.json","paper":"https://pith.science/paper/DHGX2ZG6"},"agent_actions":{"view_html":"https://pith.science/pith/DHGX2ZG66CMKGWORIFNYE5AYWR","download_json":"https://pith.science/pith/DHGX2ZG66CMKGWORIFNYE5AYWR.json","view_paper":"https://pith.science/paper/DHGX2ZG6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0410395&json=true","fetch_graph":"https://pith.science/api/pith-number/DHGX2ZG66CMKGWORIFNYE5AYWR/graph.json","fetch_events":"https://pith.science/api/pith-number/DHGX2ZG66CMKGWORIFNYE5AYWR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DHGX2ZG66CMKGWORIFNYE5AYWR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DHGX2ZG66CMKGWORIFNYE5AYWR/action/storage_attestation","attest_author":"https://pith.science/pith/DHGX2ZG66CMKGWORIFNYE5AYWR/action/author_attestation","sign_citation":"https://pith.science/pith/DHGX2ZG66CMKGWORIFNYE5AYWR/action/citation_signature","submit_replication":"https://pith.science/pith/DHGX2ZG66CMKGWORIFNYE5AYWR/action/replication_record"}},"created_at":"2026-07-04T16:44:59.269829+00:00","updated_at":"2026-07-04T16:44:59.269829+00:00"}