{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:TVI3P54WL7BJ7K6ACXPDKANZOZ","short_pith_number":"pith:TVI3P54W","schema_version":"1.0","canonical_sha256":"9d51b7f7965fc29fabc015de3501b97644e88c5a32d118dc16f7cabff1689144","source":{"kind":"arxiv","id":"2208.02768","version":1},"attestation_state":"computed","paper":{"title":"Chiral loop quantum supergravity and black hole entropy","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Hanno Sahlmann, Konstantin Eder","submitted_at":"2022-08-04T16:58:30Z","abstract_excerpt":"Recent work has shown that local supersymmetry on a spacetime boundary in $\\mathcal{N}$-extended AdS supergravity in chiral variables implies coupling to a boundary $\\mathrm{OSp}(\\mathcal{N}|2)_{\\mathbb{C}}$ super Chern-Simons theory. We propose a way to calculate the entropy $S$ for the boundary, in the supersymmetric version of loop quantum gravity, for the minimal case $\\mathcal{N}=1$. We calculate the dimensions of the quantum state spaces of $\\mathrm{UOSp}(1|2)$ super Chern-Simons theory with punctures, and analytically continue, for fixed quantum super area of the surface, to $\\mathrm{OS"},"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":"2208.02768","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2022-08-04T16:58:30Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"154688ce1a1a6efc81c099383309d1df0fe2ae1b768a407de400f7c1349e97ac","abstract_canon_sha256":"a66212bff4bed84b33f95a0dda53bfa682edbf932a593d38458495a3c55112a6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:46:08.319684Z","signature_b64":"pGUiLUQTavtA7sd+JSfAOaKMLXhKQheBukjALQ4SUH/d/wlD1Cc1YinuxgcHpNlL94GuKM3w4CJ8VTqtspRjDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9d51b7f7965fc29fabc015de3501b97644e88c5a32d118dc16f7cabff1689144","last_reissued_at":"2026-07-05T04:46:08.319246Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:46:08.319246Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Chiral loop quantum supergravity and black hole entropy","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Hanno Sahlmann, Konstantin Eder","submitted_at":"2022-08-04T16:58:30Z","abstract_excerpt":"Recent work has shown that local supersymmetry on a spacetime boundary in $\\mathcal{N}$-extended AdS supergravity in chiral variables implies coupling to a boundary $\\mathrm{OSp}(\\mathcal{N}|2)_{\\mathbb{C}}$ super Chern-Simons theory. We propose a way to calculate the entropy $S$ for the boundary, in the supersymmetric version of loop quantum gravity, for the minimal case $\\mathcal{N}=1$. We calculate the dimensions of the quantum state spaces of $\\mathrm{UOSp}(1|2)$ super Chern-Simons theory with punctures, and analytically continue, for fixed quantum super area of the surface, to $\\mathrm{OS"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2208.02768","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2208.02768/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":"2208.02768","created_at":"2026-07-05T04:46:08.319302+00:00"},{"alias_kind":"arxiv_version","alias_value":"2208.02768v1","created_at":"2026-07-05T04:46:08.319302+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2208.02768","created_at":"2026-07-05T04:46:08.319302+00:00"},{"alias_kind":"pith_short_12","alias_value":"TVI3P54WL7BJ","created_at":"2026-07-05T04:46:08.319302+00:00"},{"alias_kind":"pith_short_16","alias_value":"TVI3P54WL7BJ7K6A","created_at":"2026-07-05T04:46:08.319302+00:00"},{"alias_kind":"pith_short_8","alias_value":"TVI3P54W","created_at":"2026-07-05T04:46:08.319302+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.24945","citing_title":"Toller matrices and the Feynman $i\\varepsilon$ in spinfoams","ref_index":119,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TVI3P54WL7BJ7K6ACXPDKANZOZ","json":"https://pith.science/pith/TVI3P54WL7BJ7K6ACXPDKANZOZ.json","graph_json":"https://pith.science/api/pith-number/TVI3P54WL7BJ7K6ACXPDKANZOZ/graph.json","events_json":"https://pith.science/api/pith-number/TVI3P54WL7BJ7K6ACXPDKANZOZ/events.json","paper":"https://pith.science/paper/TVI3P54W"},"agent_actions":{"view_html":"https://pith.science/pith/TVI3P54WL7BJ7K6ACXPDKANZOZ","download_json":"https://pith.science/pith/TVI3P54WL7BJ7K6ACXPDKANZOZ.json","view_paper":"https://pith.science/paper/TVI3P54W","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2208.02768&json=true","fetch_graph":"https://pith.science/api/pith-number/TVI3P54WL7BJ7K6ACXPDKANZOZ/graph.json","fetch_events":"https://pith.science/api/pith-number/TVI3P54WL7BJ7K6ACXPDKANZOZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TVI3P54WL7BJ7K6ACXPDKANZOZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TVI3P54WL7BJ7K6ACXPDKANZOZ/action/storage_attestation","attest_author":"https://pith.science/pith/TVI3P54WL7BJ7K6ACXPDKANZOZ/action/author_attestation","sign_citation":"https://pith.science/pith/TVI3P54WL7BJ7K6ACXPDKANZOZ/action/citation_signature","submit_replication":"https://pith.science/pith/TVI3P54WL7BJ7K6ACXPDKANZOZ/action/replication_record"}},"created_at":"2026-07-05T04:46:08.319302+00:00","updated_at":"2026-07-05T04:46:08.319302+00:00"}