{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:7DMLNYO4JZGEZHU5DQ4K7TOJCE","short_pith_number":"pith:7DMLNYO4","schema_version":"1.0","canonical_sha256":"f8d8b6e1dc4e4c4c9e9d1c38afcdc91131a0ec6f573949eb9accf1e821448a78","source":{"kind":"arxiv","id":"2505.08741","version":1},"attestation_state":"computed","paper":{"title":"Non-factorizable Superamplitudes for Massive N = 1 Superstates","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"hep-th","authors_text":"Adam Martin, Antonio Delgado, Runqing Wang","submitted_at":"2025-05-13T16:54:19Z","abstract_excerpt":"In this paper we study non-factorizable N = 1 superamplitudes for massive chiral superstates. We demonstrate how little group scaling and the supersymmetric Ward identities determine the form of non-factorizable massless superamplitudes, then extrapolate to massive superamplitudes by requiring they reduce to the massless form when we send all masses to zero. This technique does not depend on whether or not the superstates are self-conjugate (so that the fermionic components are either Dirac or Majorana) or whether the superamplitude is dressed with a form-factor."},"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":"2505.08741","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2025-05-13T16:54:19Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"44bc382d268ff50ba0106e05bfa041f568ec64276312f30e9f6ba5f2841104d5","abstract_canon_sha256":"644a5aede3dbfcdb9de0b8dcb2608e90954c43fd131adf76519a37206b04cdd5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:02:35.626387Z","signature_b64":"4WTfznJcY5KOflc52vqGYASASj5URKfI2QP9DnxBKuUhce75ZBJ2DBYYLivNfjpUSejGf2rD1M6pPS3KXcfrAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f8d8b6e1dc4e4c4c9e9d1c38afcdc91131a0ec6f573949eb9accf1e821448a78","last_reissued_at":"2026-07-05T11:02:35.625923Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:02:35.625923Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Non-factorizable Superamplitudes for Massive N = 1 Superstates","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"hep-th","authors_text":"Adam Martin, Antonio Delgado, Runqing Wang","submitted_at":"2025-05-13T16:54:19Z","abstract_excerpt":"In this paper we study non-factorizable N = 1 superamplitudes for massive chiral superstates. We demonstrate how little group scaling and the supersymmetric Ward identities determine the form of non-factorizable massless superamplitudes, then extrapolate to massive superamplitudes by requiring they reduce to the massless form when we send all masses to zero. This technique does not depend on whether or not the superstates are self-conjugate (so that the fermionic components are either Dirac or Majorana) or whether the superamplitude is dressed with a form-factor."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2505.08741","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/2505.08741/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":"2505.08741","created_at":"2026-07-05T11:02:35.625979+00:00"},{"alias_kind":"arxiv_version","alias_value":"2505.08741v1","created_at":"2026-07-05T11:02:35.625979+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2505.08741","created_at":"2026-07-05T11:02:35.625979+00:00"},{"alias_kind":"pith_short_12","alias_value":"7DMLNYO4JZGE","created_at":"2026-07-05T11:02:35.625979+00:00"},{"alias_kind":"pith_short_16","alias_value":"7DMLNYO4JZGEZHU5","created_at":"2026-07-05T11:02:35.625979+00:00"},{"alias_kind":"pith_short_8","alias_value":"7DMLNYO4","created_at":"2026-07-05T11:02:35.625979+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.17151","citing_title":"Supersymmetric geometry in non-supersymmetric effective field theory","ref_index":85,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/7DMLNYO4JZGEZHU5DQ4K7TOJCE","json":"https://pith.science/pith/7DMLNYO4JZGEZHU5DQ4K7TOJCE.json","graph_json":"https://pith.science/api/pith-number/7DMLNYO4JZGEZHU5DQ4K7TOJCE/graph.json","events_json":"https://pith.science/api/pith-number/7DMLNYO4JZGEZHU5DQ4K7TOJCE/events.json","paper":"https://pith.science/paper/7DMLNYO4"},"agent_actions":{"view_html":"https://pith.science/pith/7DMLNYO4JZGEZHU5DQ4K7TOJCE","download_json":"https://pith.science/pith/7DMLNYO4JZGEZHU5DQ4K7TOJCE.json","view_paper":"https://pith.science/paper/7DMLNYO4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2505.08741&json=true","fetch_graph":"https://pith.science/api/pith-number/7DMLNYO4JZGEZHU5DQ4K7TOJCE/graph.json","fetch_events":"https://pith.science/api/pith-number/7DMLNYO4JZGEZHU5DQ4K7TOJCE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7DMLNYO4JZGEZHU5DQ4K7TOJCE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7DMLNYO4JZGEZHU5DQ4K7TOJCE/action/storage_attestation","attest_author":"https://pith.science/pith/7DMLNYO4JZGEZHU5DQ4K7TOJCE/action/author_attestation","sign_citation":"https://pith.science/pith/7DMLNYO4JZGEZHU5DQ4K7TOJCE/action/citation_signature","submit_replication":"https://pith.science/pith/7DMLNYO4JZGEZHU5DQ4K7TOJCE/action/replication_record"}},"created_at":"2026-07-05T11:02:35.625979+00:00","updated_at":"2026-07-05T11:02:35.625979+00:00"}