{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2006:LMREAJGGR2GDVVPBYZ2TPB7WE5","short_pith_number":"pith:LMREAJGG","schema_version":"1.0","canonical_sha256":"5b224024c68e8c3ad5e1c6753787f62766bc42e70f6932aa9036ffae56484510","source":{"kind":"arxiv","id":"hep-th/0606036","version":2},"attestation_state":"computed","paper":{"title":"Cosmic D-Strings and Vortons in Supergravity","license":"","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"A. C. Davis, C. van de Bruck, Ph. Brax, Stephen C. Davis","submitted_at":"2006-06-05T15:31:29Z","abstract_excerpt":"Recent developments in string inspired models of inflation suggest that D-strings are formed at the end of inflation. Within the supergravity model of D-strings there are 2(n-1) chiral fermion zero modes for a D-string of winding n. Using the bounds on the relic vorton density, we show that D-strings with winding number n>1 are more strongly constrained than cosmic strings arising in cosmological phase transitions. The D-string tension of such vortons, if they survive until the present, has to satisfy 8\\pi G_N \\mu \\lesssim p 10^{-26} where p is the intercommutation probability. Similarly, D-st"},"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":"hep-th/0606036","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"hep-th","submitted_at":"2006-06-05T15:31:29Z","cross_cats_sorted":[],"title_canon_sha256":"88b3717665d30ac17a31a63cf5862b7e1a75d17b168cb8745011dfc9885ba9e9","abstract_canon_sha256":"a6dc363bdafba2cad909fbfda87457b9a059003df9845de4447921efd2aa2953"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:22:39.805456Z","signature_b64":"ZT+/KwdaeOpRFvHAKCQ/sdZ3OLGw3tp/Pz2tJ1kR+56Jcj8EnJhMGU/Ll1hYUF3NUmRHK8+d+0Sp0h7Z1lbnAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5b224024c68e8c3ad5e1c6753787f62766bc42e70f6932aa9036ffae56484510","last_reissued_at":"2026-07-04T15:22:39.805105Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:22:39.805105Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cosmic D-Strings and Vortons in Supergravity","license":"","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"A. C. Davis, C. van de Bruck, Ph. Brax, Stephen C. Davis","submitted_at":"2006-06-05T15:31:29Z","abstract_excerpt":"Recent developments in string inspired models of inflation suggest that D-strings are formed at the end of inflation. Within the supergravity model of D-strings there are 2(n-1) chiral fermion zero modes for a D-string of winding n. Using the bounds on the relic vorton density, we show that D-strings with winding number n>1 are more strongly constrained than cosmic strings arising in cosmological phase transitions. The D-string tension of such vortons, if they survive until the present, has to satisfy 8\\pi G_N \\mu \\lesssim p 10^{-26} where p is the intercommutation probability. Similarly, D-st"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-th/0606036","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/hep-th/0606036/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":"hep-th/0606036","created_at":"2026-07-04T15:22:39.805165+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-th/0606036v2","created_at":"2026-07-04T15:22:39.805165+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-th/0606036","created_at":"2026-07-04T15:22:39.805165+00:00"},{"alias_kind":"pith_short_12","alias_value":"LMREAJGGR2GD","created_at":"2026-07-04T15:22:39.805165+00:00"},{"alias_kind":"pith_short_16","alias_value":"LMREAJGGR2GDVVPB","created_at":"2026-07-04T15:22:39.805165+00:00"},{"alias_kind":"pith_short_8","alias_value":"LMREAJGG","created_at":"2026-07-04T15:22:39.805165+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/LMREAJGGR2GDVVPBYZ2TPB7WE5","json":"https://pith.science/pith/LMREAJGGR2GDVVPBYZ2TPB7WE5.json","graph_json":"https://pith.science/api/pith-number/LMREAJGGR2GDVVPBYZ2TPB7WE5/graph.json","events_json":"https://pith.science/api/pith-number/LMREAJGGR2GDVVPBYZ2TPB7WE5/events.json","paper":"https://pith.science/paper/LMREAJGG"},"agent_actions":{"view_html":"https://pith.science/pith/LMREAJGGR2GDVVPBYZ2TPB7WE5","download_json":"https://pith.science/pith/LMREAJGGR2GDVVPBYZ2TPB7WE5.json","view_paper":"https://pith.science/paper/LMREAJGG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-th/0606036&json=true","fetch_graph":"https://pith.science/api/pith-number/LMREAJGGR2GDVVPBYZ2TPB7WE5/graph.json","fetch_events":"https://pith.science/api/pith-number/LMREAJGGR2GDVVPBYZ2TPB7WE5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LMREAJGGR2GDVVPBYZ2TPB7WE5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LMREAJGGR2GDVVPBYZ2TPB7WE5/action/storage_attestation","attest_author":"https://pith.science/pith/LMREAJGGR2GDVVPBYZ2TPB7WE5/action/author_attestation","sign_citation":"https://pith.science/pith/LMREAJGGR2GDVVPBYZ2TPB7WE5/action/citation_signature","submit_replication":"https://pith.science/pith/LMREAJGGR2GDVVPBYZ2TPB7WE5/action/replication_record"}},"created_at":"2026-07-04T15:22:39.805165+00:00","updated_at":"2026-07-04T15:22:39.805165+00:00"}