{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2009:THXOVVYYNMVMJXQX6HCUIXKPEH","short_pith_number":"pith:THXOVVYY","schema_version":"1.0","canonical_sha256":"99eeead7186b2ac4de17f1c5445d4f21eeaa46d33f23c3bcf27b4b3e5e3eca4f","source":{"kind":"arxiv","id":"0904.4267","version":1},"attestation_state":"computed","paper":{"title":"Quantum Liquid Signatures in Dwarf Stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR","cond-mat.other"],"primary_cat":"hep-th","authors_text":"David Pirtskhalava, Gregory Gabadadze","submitted_at":"2009-04-28T16:35:42Z","abstract_excerpt":"We develop further the proposal of arXiv:0806.3692 that a new state of matter -- charged condensate of spin-0 nuclei -- may exist in helium-core dwarf stars. The charged condensate and its fluctuations are described by an effective field theory Lagrangian. The spectrum of bosonic fluctuations is gapped, while electrons, at temperatures of interest, give rise to gapless excitations near the Fermi surface. These properties determine the evolution of the dwarfs with condensed cores. In particular, we show that such dwarf stars would cool significantly faster than their crystallized counterparts. "},"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":"0904.4267","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2009-04-28T16:35:42Z","cross_cats_sorted":["astro-ph.SR","cond-mat.other"],"title_canon_sha256":"77790ba2e152c003a1efa3ad9bb97be638c5dfed5a6de75220e65a39bb3e180a","abstract_canon_sha256":"c7998b0d1bccadd5d86be908e917b18d726e092c59adfc195f063e629733b96b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:23:23.377460Z","signature_b64":"JnHY+H5UgaC3+zzIhR5h2I3PIwm+62XIzX/ZxNwmaOVYQGSlNlvL2ZswtP76fEU3wpkjhyoD7gtNSq61eSZ+Cw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"99eeead7186b2ac4de17f1c5445d4f21eeaa46d33f23c3bcf27b4b3e5e3eca4f","last_reissued_at":"2026-05-18T04:23:23.376783Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:23:23.376783Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Quantum Liquid Signatures in Dwarf Stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR","cond-mat.other"],"primary_cat":"hep-th","authors_text":"David Pirtskhalava, Gregory Gabadadze","submitted_at":"2009-04-28T16:35:42Z","abstract_excerpt":"We develop further the proposal of arXiv:0806.3692 that a new state of matter -- charged condensate of spin-0 nuclei -- may exist in helium-core dwarf stars. The charged condensate and its fluctuations are described by an effective field theory Lagrangian. The spectrum of bosonic fluctuations is gapped, while electrons, at temperatures of interest, give rise to gapless excitations near the Fermi surface. These properties determine the evolution of the dwarfs with condensed cores. In particular, we show that such dwarf stars would cool significantly faster than their crystallized counterparts. "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0904.4267","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":""},"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":"0904.4267","created_at":"2026-05-18T04:23:23.376870+00:00"},{"alias_kind":"arxiv_version","alias_value":"0904.4267v1","created_at":"2026-05-18T04:23:23.376870+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0904.4267","created_at":"2026-05-18T04:23:23.376870+00:00"},{"alias_kind":"pith_short_12","alias_value":"THXOVVYYNMVM","created_at":"2026-05-18T12:26:01.383474+00:00"},{"alias_kind":"pith_short_16","alias_value":"THXOVVYYNMVMJXQX","created_at":"2026-05-18T12:26:01.383474+00:00"},{"alias_kind":"pith_short_8","alias_value":"THXOVVYY","created_at":"2026-05-18T12:26:01.383474+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/THXOVVYYNMVMJXQX6HCUIXKPEH","json":"https://pith.science/pith/THXOVVYYNMVMJXQX6HCUIXKPEH.json","graph_json":"https://pith.science/api/pith-number/THXOVVYYNMVMJXQX6HCUIXKPEH/graph.json","events_json":"https://pith.science/api/pith-number/THXOVVYYNMVMJXQX6HCUIXKPEH/events.json","paper":"https://pith.science/paper/THXOVVYY"},"agent_actions":{"view_html":"https://pith.science/pith/THXOVVYYNMVMJXQX6HCUIXKPEH","download_json":"https://pith.science/pith/THXOVVYYNMVMJXQX6HCUIXKPEH.json","view_paper":"https://pith.science/paper/THXOVVYY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0904.4267&json=true","fetch_graph":"https://pith.science/api/pith-number/THXOVVYYNMVMJXQX6HCUIXKPEH/graph.json","fetch_events":"https://pith.science/api/pith-number/THXOVVYYNMVMJXQX6HCUIXKPEH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/THXOVVYYNMVMJXQX6HCUIXKPEH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/THXOVVYYNMVMJXQX6HCUIXKPEH/action/storage_attestation","attest_author":"https://pith.science/pith/THXOVVYYNMVMJXQX6HCUIXKPEH/action/author_attestation","sign_citation":"https://pith.science/pith/THXOVVYYNMVMJXQX6HCUIXKPEH/action/citation_signature","submit_replication":"https://pith.science/pith/THXOVVYYNMVMJXQX6HCUIXKPEH/action/replication_record"}},"created_at":"2026-05-18T04:23:23.376870+00:00","updated_at":"2026-05-18T04:23:23.376870+00:00"}