{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:VHMHKNCRBND3LH3VKPZRJC6OVK","short_pith_number":"pith:VHMHKNCR","schema_version":"1.0","canonical_sha256":"a9d87534510b47b59f7553f3148bceaa883e6cf051f4c87568fe80d8495f3313","source":{"kind":"arxiv","id":"1506.05722","version":1},"attestation_state":"computed","paper":{"title":"Stability Bounds on Compact Astrophysical Objects from Information-Entropic Measure","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR","hep-th"],"primary_cat":"gr-qc","authors_text":"Marcelo Gleiser, Nan Jiang","submitted_at":"2015-06-18T15:41:32Z","abstract_excerpt":"We obtain bounds on the stability of various self-gravitating astrophysical objects using a new measure of shape complexity known as configurational entropy. We apply the method to Newtonian polytropes, neutron stars with an Oppenheimer-Volkoff equation of state, and to self-gravitating configurations of complex scalar field (boson stars) with different self-couplings, showing that the critical stability region of these stellar configurations obtained from traditional perturbation methods correlates well with critical points of the configurational entropy with accuracy of a few percent or bett"},"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":"1506.05722","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2015-06-18T15:41:32Z","cross_cats_sorted":["astro-ph.SR","hep-th"],"title_canon_sha256":"207d231f28eb61dc8c39bcb5d42aad412fa1e8a676d30c8af1de26b5b11e152e","abstract_canon_sha256":"38215e5ca3eb867a4c164e78d4970619045a85071050dd1d1d82010fe1611d21"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:11:33.513167Z","signature_b64":"2dZouVCDquR6JJqNwulRimSFZSdqWhfs1lFU+ulm5SXkBBzyhMtWlZEVdaUPVJynn1wq2OD4cPute/MKGEpKAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a9d87534510b47b59f7553f3148bceaa883e6cf051f4c87568fe80d8495f3313","last_reissued_at":"2026-05-18T01:11:33.512578Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:11:33.512578Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Stability Bounds on Compact Astrophysical Objects from Information-Entropic Measure","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR","hep-th"],"primary_cat":"gr-qc","authors_text":"Marcelo Gleiser, Nan Jiang","submitted_at":"2015-06-18T15:41:32Z","abstract_excerpt":"We obtain bounds on the stability of various self-gravitating astrophysical objects using a new measure of shape complexity known as configurational entropy. We apply the method to Newtonian polytropes, neutron stars with an Oppenheimer-Volkoff equation of state, and to self-gravitating configurations of complex scalar field (boson stars) with different self-couplings, showing that the critical stability region of these stellar configurations obtained from traditional perturbation methods correlates well with critical points of the configurational entropy with accuracy of a few percent or bett"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1506.05722","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":"1506.05722","created_at":"2026-05-18T01:11:33.512655+00:00"},{"alias_kind":"arxiv_version","alias_value":"1506.05722v1","created_at":"2026-05-18T01:11:33.512655+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1506.05722","created_at":"2026-05-18T01:11:33.512655+00:00"},{"alias_kind":"pith_short_12","alias_value":"VHMHKNCRBND3","created_at":"2026-05-18T12:29:44.643036+00:00"},{"alias_kind":"pith_short_16","alias_value":"VHMHKNCRBND3LH3V","created_at":"2026-05-18T12:29:44.643036+00:00"},{"alias_kind":"pith_short_8","alias_value":"VHMHKNCR","created_at":"2026-05-18T12:29:44.643036+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"1202.5809","citing_title":"Dynamical Boson Stars","ref_index":212,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/VHMHKNCRBND3LH3VKPZRJC6OVK","json":"https://pith.science/pith/VHMHKNCRBND3LH3VKPZRJC6OVK.json","graph_json":"https://pith.science/api/pith-number/VHMHKNCRBND3LH3VKPZRJC6OVK/graph.json","events_json":"https://pith.science/api/pith-number/VHMHKNCRBND3LH3VKPZRJC6OVK/events.json","paper":"https://pith.science/paper/VHMHKNCR"},"agent_actions":{"view_html":"https://pith.science/pith/VHMHKNCRBND3LH3VKPZRJC6OVK","download_json":"https://pith.science/pith/VHMHKNCRBND3LH3VKPZRJC6OVK.json","view_paper":"https://pith.science/paper/VHMHKNCR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1506.05722&json=true","fetch_graph":"https://pith.science/api/pith-number/VHMHKNCRBND3LH3VKPZRJC6OVK/graph.json","fetch_events":"https://pith.science/api/pith-number/VHMHKNCRBND3LH3VKPZRJC6OVK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VHMHKNCRBND3LH3VKPZRJC6OVK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VHMHKNCRBND3LH3VKPZRJC6OVK/action/storage_attestation","attest_author":"https://pith.science/pith/VHMHKNCRBND3LH3VKPZRJC6OVK/action/author_attestation","sign_citation":"https://pith.science/pith/VHMHKNCRBND3LH3VKPZRJC6OVK/action/citation_signature","submit_replication":"https://pith.science/pith/VHMHKNCRBND3LH3VKPZRJC6OVK/action/replication_record"}},"created_at":"2026-05-18T01:11:33.512655+00:00","updated_at":"2026-05-18T01:11:33.512655+00:00"}