{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:KSTH2EH3WROTXBTGRUTDTF7FOA","short_pith_number":"pith:KSTH2EH3","schema_version":"1.0","canonical_sha256":"54a67d10fbb45d3b86668d263997e570260a5772303afc30d50ce2cb669a25f9","source":{"kind":"arxiv","id":"1202.2474","version":2},"attestation_state":"computed","paper":{"title":"CMB Distortions from Superconducting Cosmic Strings","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph","hep-th"],"primary_cat":"astro-ph.CO","authors_text":"Eray Sabancilar, Hiroyuki Tashiro, Tanmay Vachaspati","submitted_at":"2012-02-11T20:54:37Z","abstract_excerpt":"We reconsider the effect of electromagnetic radiation from superconducting strings on cosmic microwave background (CMB) mu- and y-distortions and derive present (COBE-FIRAS) and future (PIXIE) constraints on the string tension, mu_s, and electric current, I. We show that absence of distortions of the CMB in PIXIE will impose strong constraints on mu_s and I, leaving the possibility of light strings (G mu_s < 10^{-18}) or relatively weak currents (I < 10 TeV)."},"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":"1202.2474","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-02-11T20:54:37Z","cross_cats_sorted":["hep-ph","hep-th"],"title_canon_sha256":"8772ceccde38122462b0354b467592a4c7c801103bdb8ad1f10cd49d94a6bfc6","abstract_canon_sha256":"da600dfd574a2d6efdbee4de180e85dd6f9cc8cec50288c41da6e25be660f491"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:38:23.716807Z","signature_b64":"5kUMtcPEXwjU5/hoX44ARXyQNwwZ2eu169qGkbPUeAn080wvMfkhE+8BSA84vDy8DWbelDctTHVw0IWtVOADCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"54a67d10fbb45d3b86668d263997e570260a5772303afc30d50ce2cb669a25f9","last_reissued_at":"2026-05-18T03:38:23.715982Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:38:23.715982Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"CMB Distortions from Superconducting Cosmic Strings","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph","hep-th"],"primary_cat":"astro-ph.CO","authors_text":"Eray Sabancilar, Hiroyuki Tashiro, Tanmay Vachaspati","submitted_at":"2012-02-11T20:54:37Z","abstract_excerpt":"We reconsider the effect of electromagnetic radiation from superconducting strings on cosmic microwave background (CMB) mu- and y-distortions and derive present (COBE-FIRAS) and future (PIXIE) constraints on the string tension, mu_s, and electric current, I. We show that absence of distortions of the CMB in PIXIE will impose strong constraints on mu_s and I, leaving the possibility of light strings (G mu_s < 10^{-18}) or relatively weak currents (I < 10 TeV)."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1202.2474","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":"1202.2474","created_at":"2026-05-18T03:38:23.716114+00:00"},{"alias_kind":"arxiv_version","alias_value":"1202.2474v2","created_at":"2026-05-18T03:38:23.716114+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1202.2474","created_at":"2026-05-18T03:38:23.716114+00:00"},{"alias_kind":"pith_short_12","alias_value":"KSTH2EH3WROT","created_at":"2026-05-18T12:27:11.947152+00:00"},{"alias_kind":"pith_short_16","alias_value":"KSTH2EH3WROTXBTG","created_at":"2026-05-18T12:27:11.947152+00:00"},{"alias_kind":"pith_short_8","alias_value":"KSTH2EH3","created_at":"2026-05-18T12:27:11.947152+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/KSTH2EH3WROTXBTGRUTDTF7FOA","json":"https://pith.science/pith/KSTH2EH3WROTXBTGRUTDTF7FOA.json","graph_json":"https://pith.science/api/pith-number/KSTH2EH3WROTXBTGRUTDTF7FOA/graph.json","events_json":"https://pith.science/api/pith-number/KSTH2EH3WROTXBTGRUTDTF7FOA/events.json","paper":"https://pith.science/paper/KSTH2EH3"},"agent_actions":{"view_html":"https://pith.science/pith/KSTH2EH3WROTXBTGRUTDTF7FOA","download_json":"https://pith.science/pith/KSTH2EH3WROTXBTGRUTDTF7FOA.json","view_paper":"https://pith.science/paper/KSTH2EH3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1202.2474&json=true","fetch_graph":"https://pith.science/api/pith-number/KSTH2EH3WROTXBTGRUTDTF7FOA/graph.json","fetch_events":"https://pith.science/api/pith-number/KSTH2EH3WROTXBTGRUTDTF7FOA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KSTH2EH3WROTXBTGRUTDTF7FOA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KSTH2EH3WROTXBTGRUTDTF7FOA/action/storage_attestation","attest_author":"https://pith.science/pith/KSTH2EH3WROTXBTGRUTDTF7FOA/action/author_attestation","sign_citation":"https://pith.science/pith/KSTH2EH3WROTXBTGRUTDTF7FOA/action/citation_signature","submit_replication":"https://pith.science/pith/KSTH2EH3WROTXBTGRUTDTF7FOA/action/replication_record"}},"created_at":"2026-05-18T03:38:23.716114+00:00","updated_at":"2026-05-18T03:38:23.716114+00:00"}