{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:OTHVTAVDB42W2ALTREEOI6I4HM","short_pith_number":"pith:OTHVTAVD","schema_version":"1.0","canonical_sha256":"74cf5982a30f356d01738908e4791c3b053fda5138368ba0650b33b47b783724","source":{"kind":"arxiv","id":"1512.01964","version":3},"attestation_state":"computed","paper":{"title":"Nilpotent chiral superfield in N=2 supergravity and partial rigid supersymmetry breaking","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Gabriele Tartaglino-Mazzucchelli, Sergei M. Kuzenko","submitted_at":"2015-12-07T10:19:30Z","abstract_excerpt":"In the framework of N=2 conformal supergravity in four dimensions, we introduce a nilpotent chiral superfield suitable for the description of partial supersymmetry breaking in maximally supersymmetric spacetimes. As an application, we construct Maxwell-Goldstone multiplet actions for partial N=2 --> N=1 supersymmetry breaking on R x S^3, AdS_3 x S^1 (or its covering AdS_3 x R), and a pp-wave spacetime. In each of these cases, the action coincides with a unique curved-superspace extension of the N=1 supersymmetric Born-Infeld action, which is singled out by the requirement of U(1) duality invar"},"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":"1512.01964","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2015-12-07T10:19:30Z","cross_cats_sorted":[],"title_canon_sha256":"977a4d7679f0ba285fd60aaad03f7ea99e000244b809cf11c9c87f0c4baf9db6","abstract_canon_sha256":"0f231b591d795d4d359acadb71819db91d61075f75c0531fa30552c3d58c75fe"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:16:44.959499Z","signature_b64":"Jd8RHN6KOiQyIzQsribQkeA06NpjIWx6HQYXl3XtOiKi2GZ4nWhWwcNwHsxGxX1GgyBTN5hxInib8FP0BVtQBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"74cf5982a30f356d01738908e4791c3b053fda5138368ba0650b33b47b783724","last_reissued_at":"2026-05-18T01:16:44.958831Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:16:44.958831Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Nilpotent chiral superfield in N=2 supergravity and partial rigid supersymmetry breaking","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Gabriele Tartaglino-Mazzucchelli, Sergei M. Kuzenko","submitted_at":"2015-12-07T10:19:30Z","abstract_excerpt":"In the framework of N=2 conformal supergravity in four dimensions, we introduce a nilpotent chiral superfield suitable for the description of partial supersymmetry breaking in maximally supersymmetric spacetimes. As an application, we construct Maxwell-Goldstone multiplet actions for partial N=2 --> N=1 supersymmetry breaking on R x S^3, AdS_3 x S^1 (or its covering AdS_3 x R), and a pp-wave spacetime. In each of these cases, the action coincides with a unique curved-superspace extension of the N=1 supersymmetric Born-Infeld action, which is singled out by the requirement of U(1) duality invar"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1512.01964","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":"1512.01964","created_at":"2026-05-18T01:16:44.958925+00:00"},{"alias_kind":"arxiv_version","alias_value":"1512.01964v3","created_at":"2026-05-18T01:16:44.958925+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1512.01964","created_at":"2026-05-18T01:16:44.958925+00:00"},{"alias_kind":"pith_short_12","alias_value":"OTHVTAVDB42W","created_at":"2026-05-18T12:29:34.919912+00:00"},{"alias_kind":"pith_short_16","alias_value":"OTHVTAVDB42W2ALT","created_at":"2026-05-18T12:29:34.919912+00:00"},{"alias_kind":"pith_short_8","alias_value":"OTHVTAVD","created_at":"2026-05-18T12:29:34.919912+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.06193","citing_title":"Causal self-dual nonlinear electrodynamics from the Born-Infeld theory","ref_index":41,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/OTHVTAVDB42W2ALTREEOI6I4HM","json":"https://pith.science/pith/OTHVTAVDB42W2ALTREEOI6I4HM.json","graph_json":"https://pith.science/api/pith-number/OTHVTAVDB42W2ALTREEOI6I4HM/graph.json","events_json":"https://pith.science/api/pith-number/OTHVTAVDB42W2ALTREEOI6I4HM/events.json","paper":"https://pith.science/paper/OTHVTAVD"},"agent_actions":{"view_html":"https://pith.science/pith/OTHVTAVDB42W2ALTREEOI6I4HM","download_json":"https://pith.science/pith/OTHVTAVDB42W2ALTREEOI6I4HM.json","view_paper":"https://pith.science/paper/OTHVTAVD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1512.01964&json=true","fetch_graph":"https://pith.science/api/pith-number/OTHVTAVDB42W2ALTREEOI6I4HM/graph.json","fetch_events":"https://pith.science/api/pith-number/OTHVTAVDB42W2ALTREEOI6I4HM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OTHVTAVDB42W2ALTREEOI6I4HM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OTHVTAVDB42W2ALTREEOI6I4HM/action/storage_attestation","attest_author":"https://pith.science/pith/OTHVTAVDB42W2ALTREEOI6I4HM/action/author_attestation","sign_citation":"https://pith.science/pith/OTHVTAVDB42W2ALTREEOI6I4HM/action/citation_signature","submit_replication":"https://pith.science/pith/OTHVTAVDB42W2ALTREEOI6I4HM/action/replication_record"}},"created_at":"2026-05-18T01:16:44.958925+00:00","updated_at":"2026-05-18T01:16:44.958925+00:00"}