{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:KL3443VHYHLJZAWHWJTP56HADA","short_pith_number":"pith:KL3443VH","schema_version":"1.0","canonical_sha256":"52f7ce6ea7c1d69c82c7b266fef8e01805bbc60c65c8506d47189a768a71ce80","source":{"kind":"arxiv","id":"1805.10650","version":5},"attestation_state":"computed","paper":{"title":"White dwarfs in de Rham-Gabadadze-Tolley like massive gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-th"],"primary_cat":"gr-qc","authors_text":"B. Eslam Panah, H.L. Liu","submitted_at":"2018-05-27T16:41:52Z","abstract_excerpt":"The existence of possible massive white dwarfs more than the Chandrasekhar limit ($1.45M_{\\odot }$, in which $M_{\\odot }$ is mass of the sun) is a challenging topic. In this regard and motivated by the important effect of massive graviton on the structure of white dwarfs we study the white dwarfs in Vegh's massive gravity which is known as one of theories of de Rham, Gabadadze and Tolley (dRGT) like massive gravity. First, we consider the modified Tolman-Oppenheimer-Volkoff equation in this theory of massive gravity and solve it numerically by using the Chandrasekhar's equation of state. Our r"},"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":"1805.10650","kind":"arxiv","version":5},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2018-05-27T16:41:52Z","cross_cats_sorted":["astro-ph.HE","hep-th"],"title_canon_sha256":"d67ba5ecb51813059006b3df0ca9d18110bc7f15380a420871f3f43a2689ba76","abstract_canon_sha256":"97144896a3309308e9d02894cff4e541c8150cd655720f3db96d22892e5b6972"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:44:13.399197Z","signature_b64":"sQwfg4ozthOzRtA0M9gPEfdgLqJl3y3Ya9AH0xs0lPCGsA1p1G4CLDtm5U/KESLB7drxK94JlbwVSkq4/Jf8AA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"52f7ce6ea7c1d69c82c7b266fef8e01805bbc60c65c8506d47189a768a71ce80","last_reissued_at":"2026-05-17T23:44:13.398498Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:44:13.398498Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"White dwarfs in de Rham-Gabadadze-Tolley like massive gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-th"],"primary_cat":"gr-qc","authors_text":"B. Eslam Panah, H.L. Liu","submitted_at":"2018-05-27T16:41:52Z","abstract_excerpt":"The existence of possible massive white dwarfs more than the Chandrasekhar limit ($1.45M_{\\odot }$, in which $M_{\\odot }$ is mass of the sun) is a challenging topic. In this regard and motivated by the important effect of massive graviton on the structure of white dwarfs we study the white dwarfs in Vegh's massive gravity which is known as one of theories of de Rham, Gabadadze and Tolley (dRGT) like massive gravity. First, we consider the modified Tolman-Oppenheimer-Volkoff equation in this theory of massive gravity and solve it numerically by using the Chandrasekhar's equation of state. Our r"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1805.10650","kind":"arxiv","version":5},"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":"1805.10650","created_at":"2026-05-17T23:44:13.398615+00:00"},{"alias_kind":"arxiv_version","alias_value":"1805.10650v5","created_at":"2026-05-17T23:44:13.398615+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1805.10650","created_at":"2026-05-17T23:44:13.398615+00:00"},{"alias_kind":"pith_short_12","alias_value":"KL3443VHYHLJ","created_at":"2026-05-18T12:32:33.847187+00:00"},{"alias_kind":"pith_short_16","alias_value":"KL3443VHYHLJZAWH","created_at":"2026-05-18T12:32:33.847187+00:00"},{"alias_kind":"pith_short_8","alias_value":"KL3443VH","created_at":"2026-05-18T12:32:33.847187+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2509.04261","citing_title":"Topological charge and black hole photon spheres in massive gravity","ref_index":93,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/KL3443VHYHLJZAWHWJTP56HADA","json":"https://pith.science/pith/KL3443VHYHLJZAWHWJTP56HADA.json","graph_json":"https://pith.science/api/pith-number/KL3443VHYHLJZAWHWJTP56HADA/graph.json","events_json":"https://pith.science/api/pith-number/KL3443VHYHLJZAWHWJTP56HADA/events.json","paper":"https://pith.science/paper/KL3443VH"},"agent_actions":{"view_html":"https://pith.science/pith/KL3443VHYHLJZAWHWJTP56HADA","download_json":"https://pith.science/pith/KL3443VHYHLJZAWHWJTP56HADA.json","view_paper":"https://pith.science/paper/KL3443VH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1805.10650&json=true","fetch_graph":"https://pith.science/api/pith-number/KL3443VHYHLJZAWHWJTP56HADA/graph.json","fetch_events":"https://pith.science/api/pith-number/KL3443VHYHLJZAWHWJTP56HADA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KL3443VHYHLJZAWHWJTP56HADA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KL3443VHYHLJZAWHWJTP56HADA/action/storage_attestation","attest_author":"https://pith.science/pith/KL3443VHYHLJZAWHWJTP56HADA/action/author_attestation","sign_citation":"https://pith.science/pith/KL3443VHYHLJZAWHWJTP56HADA/action/citation_signature","submit_replication":"https://pith.science/pith/KL3443VHYHLJZAWHWJTP56HADA/action/replication_record"}},"created_at":"2026-05-17T23:44:13.398615+00:00","updated_at":"2026-05-17T23:44:13.398615+00:00"}