{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:2XOBOP473HPO5C5GZQV35O2K65","short_pith_number":"pith:2XOBOP47","schema_version":"1.0","canonical_sha256":"d5dc173f9fd9deee8ba6cc2bbebb4af75f4fe07c2117176e294125bfeb74d9b1","source":{"kind":"arxiv","id":"1507.08553","version":2},"attestation_state":"computed","paper":{"title":"Supersymmetric Casimir Energy and the Anomaly Polynomial","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Hee-Cheol Kim, Mathew Bullimore, Nikolay Bobev","submitted_at":"2015-07-30T15:46:57Z","abstract_excerpt":"We conjecture that for superconformal field theories in even dimensions, the supersymmetric Casimir energy on a space with topology $S^1\\times S^{D-1}$ is equal to an equivariant integral of the anomaly polynomial. The equivariant integration is defined with respect to the Cartan subalgebra of the global symmetry algebra that commutes with a given supercharge. We test our proposal extensively by computing the supersymmetric Casimir energy for large classes of superconformal field theories, with and without known Lagrangian descriptions, in two, four and six dimensions."},"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":"1507.08553","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2015-07-30T15:46:57Z","cross_cats_sorted":[],"title_canon_sha256":"4e00ba26ae8363bc6dfb97b4f6765ed2eb62d91e8f59dc21e81d5122d52a1212","abstract_canon_sha256":"7471ef4028b165c79a43aebc2f6a3e1ea4404d7f85c1a936e15d1e4cc3925ac9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:18:14.435300Z","signature_b64":"LzLRkvQVmFuwvhXfAvei/XCDwl/KtXB/L0hFcR0I3zOij1HlweUlufbbrZUPkjAI+jRpOnFa5qvRs3Sqr7jSDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d5dc173f9fd9deee8ba6cc2bbebb4af75f4fe07c2117176e294125bfeb74d9b1","last_reissued_at":"2026-05-18T01:18:14.434716Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:18:14.434716Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Supersymmetric Casimir Energy and the Anomaly Polynomial","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Hee-Cheol Kim, Mathew Bullimore, Nikolay Bobev","submitted_at":"2015-07-30T15:46:57Z","abstract_excerpt":"We conjecture that for superconformal field theories in even dimensions, the supersymmetric Casimir energy on a space with topology $S^1\\times S^{D-1}$ is equal to an equivariant integral of the anomaly polynomial. The equivariant integration is defined with respect to the Cartan subalgebra of the global symmetry algebra that commutes with a given supercharge. We test our proposal extensively by computing the supersymmetric Casimir energy for large classes of superconformal field theories, with and without known Lagrangian descriptions, in two, four and six dimensions."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1507.08553","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":""},"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":"1507.08553","created_at":"2026-05-18T01:18:14.434786+00:00"},{"alias_kind":"arxiv_version","alias_value":"1507.08553v2","created_at":"2026-05-18T01:18:14.434786+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1507.08553","created_at":"2026-05-18T01:18:14.434786+00:00"},{"alias_kind":"pith_short_12","alias_value":"2XOBOP473HPO","created_at":"2026-05-18T12:29:02.477457+00:00"},{"alias_kind":"pith_short_16","alias_value":"2XOBOP473HPO5C5G","created_at":"2026-05-18T12:29:02.477457+00:00"},{"alias_kind":"pith_short_8","alias_value":"2XOBOP47","created_at":"2026-05-18T12:29:02.477457+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2501.09498","citing_title":"From Weyl Anomaly to Defect Supersymmetric R\\'enyi Entropy and Casimir Energy","ref_index":38,"is_internal_anchor":true},{"citing_arxiv_id":"2604.19885","citing_title":"On non-relativistic integrable models and 4d SCFTs","ref_index":35,"is_internal_anchor":false},{"citing_arxiv_id":"2604.06343","citing_title":"Indices of M5 and M2 branes at finite $N$ from equivariant volumes, and a new duality","ref_index":8,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/2XOBOP473HPO5C5GZQV35O2K65","json":"https://pith.science/pith/2XOBOP473HPO5C5GZQV35O2K65.json","graph_json":"https://pith.science/api/pith-number/2XOBOP473HPO5C5GZQV35O2K65/graph.json","events_json":"https://pith.science/api/pith-number/2XOBOP473HPO5C5GZQV35O2K65/events.json","paper":"https://pith.science/paper/2XOBOP47"},"agent_actions":{"view_html":"https://pith.science/pith/2XOBOP473HPO5C5GZQV35O2K65","download_json":"https://pith.science/pith/2XOBOP473HPO5C5GZQV35O2K65.json","view_paper":"https://pith.science/paper/2XOBOP47","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1507.08553&json=true","fetch_graph":"https://pith.science/api/pith-number/2XOBOP473HPO5C5GZQV35O2K65/graph.json","fetch_events":"https://pith.science/api/pith-number/2XOBOP473HPO5C5GZQV35O2K65/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2XOBOP473HPO5C5GZQV35O2K65/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2XOBOP473HPO5C5GZQV35O2K65/action/storage_attestation","attest_author":"https://pith.science/pith/2XOBOP473HPO5C5GZQV35O2K65/action/author_attestation","sign_citation":"https://pith.science/pith/2XOBOP473HPO5C5GZQV35O2K65/action/citation_signature","submit_replication":"https://pith.science/pith/2XOBOP473HPO5C5GZQV35O2K65/action/replication_record"}},"created_at":"2026-05-18T01:18:14.434786+00:00","updated_at":"2026-05-18T01:18:14.434786+00:00"}