{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2009:PTE66DVEC6CGQRB6XEUN42U643","short_pith_number":"pith:PTE66DVE","schema_version":"1.0","canonical_sha256":"7cc9ef0ea4178468443eb928de6a9ee6ef7425e699bc4750745e141546e1ee54","source":{"kind":"arxiv","id":"0912.4039","version":3},"attestation_state":"computed","paper":{"title":"Scalar-field Pressure in Induced Gravity with Higgs Potential and Dark Matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"gr-qc","authors_text":"Heinz Dehnen, Hemwati Nandan, Nils M. Bezares-Roder","submitted_at":"2009-12-20T18:40:06Z","abstract_excerpt":"A model of induced gravity with a Higgs potential is investigated in detail in view of the pressure components related to the scalar-field excitations. The physical consequences emerging as an artifact due to the presence of these pressure terms are analysed in terms of the constraints parting from energy density, solar-relativistic effects and galactic dynamics along with the dark matter halos."},"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":"0912.4039","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2009-12-20T18:40:06Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"5840715fa70c145419e91e555857b8d4c60a9287730ca3e20a22d9792689db59","abstract_canon_sha256":"bcb463e3d527de9bfe663d5dfd0ac3112dd68e093fd066bd29ce5f14fd79733c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:34:46.226223Z","signature_b64":"6OOJuFbw3cqfr5tqIwtove6m4SOS7Zs90SihIGGTIjI8sOigXiDs+TMx4M8vf8xyjmi4Rc+ZXBPHtDPDjGTKCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7cc9ef0ea4178468443eb928de6a9ee6ef7425e699bc4750745e141546e1ee54","last_reissued_at":"2026-05-18T04:34:46.225781Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:34:46.225781Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Scalar-field Pressure in Induced Gravity with Higgs Potential and Dark Matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"gr-qc","authors_text":"Heinz Dehnen, Hemwati Nandan, Nils M. Bezares-Roder","submitted_at":"2009-12-20T18:40:06Z","abstract_excerpt":"A model of induced gravity with a Higgs potential is investigated in detail in view of the pressure components related to the scalar-field excitations. The physical consequences emerging as an artifact due to the presence of these pressure terms are analysed in terms of the constraints parting from energy density, solar-relativistic effects and galactic dynamics along with the dark matter halos."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0912.4039","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":""},"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":"0912.4039","created_at":"2026-05-18T04:34:46.225839+00:00"},{"alias_kind":"arxiv_version","alias_value":"0912.4039v3","created_at":"2026-05-18T04:34:46.225839+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0912.4039","created_at":"2026-05-18T04:34:46.225839+00:00"},{"alias_kind":"pith_short_12","alias_value":"PTE66DVEC6CG","created_at":"2026-05-18T12:26:01.383474+00:00"},{"alias_kind":"pith_short_16","alias_value":"PTE66DVEC6CGQRB6","created_at":"2026-05-18T12:26:01.383474+00:00"},{"alias_kind":"pith_short_8","alias_value":"PTE66DVE","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/PTE66DVEC6CGQRB6XEUN42U643","json":"https://pith.science/pith/PTE66DVEC6CGQRB6XEUN42U643.json","graph_json":"https://pith.science/api/pith-number/PTE66DVEC6CGQRB6XEUN42U643/graph.json","events_json":"https://pith.science/api/pith-number/PTE66DVEC6CGQRB6XEUN42U643/events.json","paper":"https://pith.science/paper/PTE66DVE"},"agent_actions":{"view_html":"https://pith.science/pith/PTE66DVEC6CGQRB6XEUN42U643","download_json":"https://pith.science/pith/PTE66DVEC6CGQRB6XEUN42U643.json","view_paper":"https://pith.science/paper/PTE66DVE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0912.4039&json=true","fetch_graph":"https://pith.science/api/pith-number/PTE66DVEC6CGQRB6XEUN42U643/graph.json","fetch_events":"https://pith.science/api/pith-number/PTE66DVEC6CGQRB6XEUN42U643/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PTE66DVEC6CGQRB6XEUN42U643/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PTE66DVEC6CGQRB6XEUN42U643/action/storage_attestation","attest_author":"https://pith.science/pith/PTE66DVEC6CGQRB6XEUN42U643/action/author_attestation","sign_citation":"https://pith.science/pith/PTE66DVEC6CGQRB6XEUN42U643/action/citation_signature","submit_replication":"https://pith.science/pith/PTE66DVEC6CGQRB6XEUN42U643/action/replication_record"}},"created_at":"2026-05-18T04:34:46.225839+00:00","updated_at":"2026-05-18T04:34:46.225839+00:00"}