{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:HLMBBM46HJRRDJXOPDGVES3VRS","short_pith_number":"pith:HLMBBM46","schema_version":"1.0","canonical_sha256":"3ad810b39e3a6311a6ee78cd524b758c828bffe44f0fc1e22167d153e05be64f","source":{"kind":"arxiv","id":"1708.01411","version":3},"attestation_state":"computed","paper":{"title":"On the thermodynamics of the black hole and hairy black hole transitions in the asymptotically flat spacetime with a box","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Bin Wang, Yan Peng, Yunqi Liu","submitted_at":"2017-08-04T08:10:26Z","abstract_excerpt":"We study the asymptotically flat quasi-local black hole/hairy black hole model with nonzero mass of the scalar filed. We disclose effects of the scalar mass on transitions in a grand canonical ensemble with condensation behaviors of a parameter $\\psi_{2}$, which is similar to approaches in holographic theories. We find that more negative scalar mass makes the phase transition easier to happen. We also obtain an analytical relation $\\psi_{2}\\varpropto(T_{c}-T)^{1/2}$ around the critical phase transition points implying a second order phase transition. Besides the parameter $\\psi_{2}$, we show t"},"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":"1708.01411","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2017-08-04T08:10:26Z","cross_cats_sorted":[],"title_canon_sha256":"ef1e782a833bd11e5e0f2be701e2ea4f8b6ee2c5ae7c56da0bb019f14370a16c","abstract_canon_sha256":"0cd9442a0280944f59002b717ae4ffbad11c34160da4f0c2c4f737cceb89e1c0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:19:35.527725Z","signature_b64":"uKYeVeT2ZW8xfRgFTEpCf3c4VseP60IeJBiKejvx6I8+vZ3tdS4aE+/4IAuttSK/aD26EriZQ0Mxs/kbTqq6Aw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3ad810b39e3a6311a6ee78cd524b758c828bffe44f0fc1e22167d153e05be64f","last_reissued_at":"2026-05-18T00:19:35.527260Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:19:35.527260Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On the thermodynamics of the black hole and hairy black hole transitions in the asymptotically flat spacetime with a box","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Bin Wang, Yan Peng, Yunqi Liu","submitted_at":"2017-08-04T08:10:26Z","abstract_excerpt":"We study the asymptotically flat quasi-local black hole/hairy black hole model with nonzero mass of the scalar filed. We disclose effects of the scalar mass on transitions in a grand canonical ensemble with condensation behaviors of a parameter $\\psi_{2}$, which is similar to approaches in holographic theories. We find that more negative scalar mass makes the phase transition easier to happen. We also obtain an analytical relation $\\psi_{2}\\varpropto(T_{c}-T)^{1/2}$ around the critical phase transition points implying a second order phase transition. Besides the parameter $\\psi_{2}$, we show t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1708.01411","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":"1708.01411","created_at":"2026-05-18T00:19:35.527335+00:00"},{"alias_kind":"arxiv_version","alias_value":"1708.01411v3","created_at":"2026-05-18T00:19:35.527335+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1708.01411","created_at":"2026-05-18T00:19:35.527335+00:00"},{"alias_kind":"pith_short_12","alias_value":"HLMBBM46HJRR","created_at":"2026-05-18T12:31:18.294218+00:00"},{"alias_kind":"pith_short_16","alias_value":"HLMBBM46HJRRDJXO","created_at":"2026-05-18T12:31:18.294218+00:00"},{"alias_kind":"pith_short_8","alias_value":"HLMBBM46","created_at":"2026-05-18T12:31:18.294218+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2512.14921","citing_title":"$\\ell$-Boson stars in anti-de Sitter spacetime","ref_index":54,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/HLMBBM46HJRRDJXOPDGVES3VRS","json":"https://pith.science/pith/HLMBBM46HJRRDJXOPDGVES3VRS.json","graph_json":"https://pith.science/api/pith-number/HLMBBM46HJRRDJXOPDGVES3VRS/graph.json","events_json":"https://pith.science/api/pith-number/HLMBBM46HJRRDJXOPDGVES3VRS/events.json","paper":"https://pith.science/paper/HLMBBM46"},"agent_actions":{"view_html":"https://pith.science/pith/HLMBBM46HJRRDJXOPDGVES3VRS","download_json":"https://pith.science/pith/HLMBBM46HJRRDJXOPDGVES3VRS.json","view_paper":"https://pith.science/paper/HLMBBM46","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1708.01411&json=true","fetch_graph":"https://pith.science/api/pith-number/HLMBBM46HJRRDJXOPDGVES3VRS/graph.json","fetch_events":"https://pith.science/api/pith-number/HLMBBM46HJRRDJXOPDGVES3VRS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HLMBBM46HJRRDJXOPDGVES3VRS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HLMBBM46HJRRDJXOPDGVES3VRS/action/storage_attestation","attest_author":"https://pith.science/pith/HLMBBM46HJRRDJXOPDGVES3VRS/action/author_attestation","sign_citation":"https://pith.science/pith/HLMBBM46HJRRDJXOPDGVES3VRS/action/citation_signature","submit_replication":"https://pith.science/pith/HLMBBM46HJRRDJXOPDGVES3VRS/action/replication_record"}},"created_at":"2026-05-18T00:19:35.527335+00:00","updated_at":"2026-05-18T00:19:35.527335+00:00"}