{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:SVEKHV2IOGPFDY3PZ63FX5RWJO","short_pith_number":"pith:SVEKHV2I","schema_version":"1.0","canonical_sha256":"9548a3d748719e51e36fcfb65bf6364ba3bc560e7e18c405caf67d50f650a65e","source":{"kind":"arxiv","id":"1201.6107","version":1},"attestation_state":"computed","paper":{"title":"A brief Review of the Scalar Field Dark Matter model","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Abril Su\\'arez, Juan Maga\\~na, Tonatiuh Matos, Victor Robles","submitted_at":"2012-01-30T05:17:24Z","abstract_excerpt":"In the last time the cold dark matter (CDM) model has suggested more and more that it is not able to describe all the properties of nearby galaxies that can be observed in great detail as well as that it has some problems in the mechanism by which matter is more rapidly gathered into large-scale structure such as galaxies and clusters of galaxies. In this work we revisit an alternative model, the scalar field dark matter (SFDM) model, which proposes that the galactic haloes form by condensation of a scalar field (SF) very early in the Universe, i.e., in this model the haloes of galaxies are as"},"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":"1201.6107","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-01-30T05:17:24Z","cross_cats_sorted":[],"title_canon_sha256":"ccbcd5d7d26aeff676192b902035bb19f7731de01dd8f83015ee2df43299c1a2","abstract_canon_sha256":"e7b49a9dddba69baf1ac2fe746ebc528b69f58db35f2130c27754f3c3437b321"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:58:38.387471Z","signature_b64":"7Q/ukNmcJFgeLyZREohxYc3mL7b5q3ZYUG7Z6AvYDelBXcEQUx4/mhWTEeB+pF2DsZXecV9x2F4/QJECae3QAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9548a3d748719e51e36fcfb65bf6364ba3bc560e7e18c405caf67d50f650a65e","last_reissued_at":"2026-05-18T01:58:38.386787Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:58:38.386787Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A brief Review of the Scalar Field Dark Matter model","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Abril Su\\'arez, Juan Maga\\~na, Tonatiuh Matos, Victor Robles","submitted_at":"2012-01-30T05:17:24Z","abstract_excerpt":"In the last time the cold dark matter (CDM) model has suggested more and more that it is not able to describe all the properties of nearby galaxies that can be observed in great detail as well as that it has some problems in the mechanism by which matter is more rapidly gathered into large-scale structure such as galaxies and clusters of galaxies. In this work we revisit an alternative model, the scalar field dark matter (SFDM) model, which proposes that the galactic haloes form by condensation of a scalar field (SF) very early in the Universe, i.e., in this model the haloes of galaxies are as"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1201.6107","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":"1201.6107","created_at":"2026-05-18T01:58:38.386895+00:00"},{"alias_kind":"arxiv_version","alias_value":"1201.6107v1","created_at":"2026-05-18T01:58:38.386895+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1201.6107","created_at":"2026-05-18T01:58:38.386895+00:00"},{"alias_kind":"pith_short_12","alias_value":"SVEKHV2IOGPF","created_at":"2026-05-18T12:27:23.164592+00:00"},{"alias_kind":"pith_short_16","alias_value":"SVEKHV2IOGPFDY3P","created_at":"2026-05-18T12:27:23.164592+00:00"},{"alias_kind":"pith_short_8","alias_value":"SVEKHV2I","created_at":"2026-05-18T12:27:23.164592+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2507.05207","citing_title":"Interacting Scalar Fields as Dark Energy and Dark Matter in Einstein scalar Gauss Bonnet Gravity","ref_index":86,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/SVEKHV2IOGPFDY3PZ63FX5RWJO","json":"https://pith.science/pith/SVEKHV2IOGPFDY3PZ63FX5RWJO.json","graph_json":"https://pith.science/api/pith-number/SVEKHV2IOGPFDY3PZ63FX5RWJO/graph.json","events_json":"https://pith.science/api/pith-number/SVEKHV2IOGPFDY3PZ63FX5RWJO/events.json","paper":"https://pith.science/paper/SVEKHV2I"},"agent_actions":{"view_html":"https://pith.science/pith/SVEKHV2IOGPFDY3PZ63FX5RWJO","download_json":"https://pith.science/pith/SVEKHV2IOGPFDY3PZ63FX5RWJO.json","view_paper":"https://pith.science/paper/SVEKHV2I","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1201.6107&json=true","fetch_graph":"https://pith.science/api/pith-number/SVEKHV2IOGPFDY3PZ63FX5RWJO/graph.json","fetch_events":"https://pith.science/api/pith-number/SVEKHV2IOGPFDY3PZ63FX5RWJO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SVEKHV2IOGPFDY3PZ63FX5RWJO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SVEKHV2IOGPFDY3PZ63FX5RWJO/action/storage_attestation","attest_author":"https://pith.science/pith/SVEKHV2IOGPFDY3PZ63FX5RWJO/action/author_attestation","sign_citation":"https://pith.science/pith/SVEKHV2IOGPFDY3PZ63FX5RWJO/action/citation_signature","submit_replication":"https://pith.science/pith/SVEKHV2IOGPFDY3PZ63FX5RWJO/action/replication_record"}},"created_at":"2026-05-18T01:58:38.386895+00:00","updated_at":"2026-05-18T01:58:38.386895+00:00"}