{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:TPRMWU2W2PYLCFVBZDRQP46D4V","short_pith_number":"pith:TPRMWU2W","schema_version":"1.0","canonical_sha256":"9be2cb5356d3f0b116a1c8e307f3c3e55489f8f3b9c81f4728d6be5b5bbd2450","source":{"kind":"arxiv","id":"2306.17510","version":2},"attestation_state":"computed","paper":{"title":"Influence of Dark Matter on the Magnetized Neutron Star","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["nucl-th"],"primary_cat":"astro-ph.HE","authors_text":"H. C. Das, M. K. Sharma, S. K. Patra, Vishal Parmar","submitted_at":"2023-06-30T09:55:11Z","abstract_excerpt":"Over the past two decades, significant strides have been made in the study of Dark Matter (DM) admixed neutron stars and their associated properties. However, an intriguing facet regarding the effect of DM on magnetized neutron stars still remains unexplored. This study is carried out to analyze the properties of DM admixed magnetized neutron stars. The equation of state for the DM admixed neutron star is calculated using the relativistic mean-field model with the inclusion of a density-dependent magnetic field. Several macroscopic properties, such as mass, radius, particle fractions, tidal de"},"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":"2306.17510","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2023-06-30T09:55:11Z","cross_cats_sorted":["nucl-th"],"title_canon_sha256":"b0388172112439947a94fc2c9b5830b20f62240263a06330130dcf6c38e794c2","abstract_canon_sha256":"e3aa0bffd320d790a9ce068d4a1c8996afcb232addb91a7bda1f3ec71f9cd620"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:56:35.610609Z","signature_b64":"DZMw7ryNFjkURF1otnKLaludM1zy0eXGMF8sESL63rTjjgqMZRtIGw0CjgFMFiwOmY6mji3/J0nsbdqg9CCoCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9be2cb5356d3f0b116a1c8e307f3c3e55489f8f3b9c81f4728d6be5b5bbd2450","last_reissued_at":"2026-07-05T06:56:35.610116Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:56:35.610116Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Influence of Dark Matter on the Magnetized Neutron Star","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["nucl-th"],"primary_cat":"astro-ph.HE","authors_text":"H. C. Das, M. K. Sharma, S. K. Patra, Vishal Parmar","submitted_at":"2023-06-30T09:55:11Z","abstract_excerpt":"Over the past two decades, significant strides have been made in the study of Dark Matter (DM) admixed neutron stars and their associated properties. However, an intriguing facet regarding the effect of DM on magnetized neutron stars still remains unexplored. This study is carried out to analyze the properties of DM admixed magnetized neutron stars. The equation of state for the DM admixed neutron star is calculated using the relativistic mean-field model with the inclusion of a density-dependent magnetic field. Several macroscopic properties, such as mass, radius, particle fractions, tidal de"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2306.17510","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/2306.17510/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":"2306.17510","created_at":"2026-07-05T06:56:35.610174+00:00"},{"alias_kind":"arxiv_version","alias_value":"2306.17510v2","created_at":"2026-07-05T06:56:35.610174+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2306.17510","created_at":"2026-07-05T06:56:35.610174+00:00"},{"alias_kind":"pith_short_12","alias_value":"TPRMWU2W2PYL","created_at":"2026-07-05T06:56:35.610174+00:00"},{"alias_kind":"pith_short_16","alias_value":"TPRMWU2W2PYLCFVB","created_at":"2026-07-05T06:56:35.610174+00:00"},{"alias_kind":"pith_short_8","alias_value":"TPRMWU2W","created_at":"2026-07-05T06:56:35.610174+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.22680","citing_title":"Dense Matter and Compact Stars in Strong Magnetic Fields","ref_index":124,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TPRMWU2W2PYLCFVBZDRQP46D4V","json":"https://pith.science/pith/TPRMWU2W2PYLCFVBZDRQP46D4V.json","graph_json":"https://pith.science/api/pith-number/TPRMWU2W2PYLCFVBZDRQP46D4V/graph.json","events_json":"https://pith.science/api/pith-number/TPRMWU2W2PYLCFVBZDRQP46D4V/events.json","paper":"https://pith.science/paper/TPRMWU2W"},"agent_actions":{"view_html":"https://pith.science/pith/TPRMWU2W2PYLCFVBZDRQP46D4V","download_json":"https://pith.science/pith/TPRMWU2W2PYLCFVBZDRQP46D4V.json","view_paper":"https://pith.science/paper/TPRMWU2W","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2306.17510&json=true","fetch_graph":"https://pith.science/api/pith-number/TPRMWU2W2PYLCFVBZDRQP46D4V/graph.json","fetch_events":"https://pith.science/api/pith-number/TPRMWU2W2PYLCFVBZDRQP46D4V/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TPRMWU2W2PYLCFVBZDRQP46D4V/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TPRMWU2W2PYLCFVBZDRQP46D4V/action/storage_attestation","attest_author":"https://pith.science/pith/TPRMWU2W2PYLCFVBZDRQP46D4V/action/author_attestation","sign_citation":"https://pith.science/pith/TPRMWU2W2PYLCFVBZDRQP46D4V/action/citation_signature","submit_replication":"https://pith.science/pith/TPRMWU2W2PYLCFVBZDRQP46D4V/action/replication_record"}},"created_at":"2026-07-05T06:56:35.610174+00:00","updated_at":"2026-07-05T06:56:35.610174+00:00"}