{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:OV7TEMCZ42XVL7DTKQFQHN2XPT","short_pith_number":"pith:OV7TEMCZ","schema_version":"1.0","canonical_sha256":"757f323059e6af55fc73540b03b7577cc404d79d13c989a143653af951db6c3f","source":{"kind":"arxiv","id":"1611.06103","version":1},"attestation_state":"computed","paper":{"title":"Models for Small-Scale Structure on Cosmic Strings: II. Scaling and its stability","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","gr-qc","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"C.J.A.P. Martins, E.P.S. Shellard, J. P. P. Vieira","submitted_at":"2016-11-18T14:38:51Z","abstract_excerpt":"We make use of the formalism described in a previous paper [Martins {\\it et al.} Phys. Rev. D90 (2014) 043518] to address general features of wiggly cosmic string evolution. In particular, we highlight the important role played by poorly understood energy loss mechanisms and propose a simple ansatz which tackles this problem in the context of an extended velocity-dependent one-scale model. We find a general procedure to determine all the scaling solutions admitted by a specific string model and study their stability, enabling a detailed comparison with future numerical simulations. A simpler c"},"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":"1611.06103","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2016-11-18T14:38:51Z","cross_cats_sorted":["astro-ph.HE","gr-qc","hep-ph"],"title_canon_sha256":"59b3344fc18926cbdd82a6db363ac49ea199f52d8ea09b123726a602e08cebd1","abstract_canon_sha256":"b6c35e76d836c28fab37f87e65e01d4a1a26d683241254355b0048fe534e8a54"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:57:43.090686Z","signature_b64":"EtS03Y7jsDi6gErwU1ANLJq9oHYGJSq35l0QfBMippn9iKwQRhi+OQXGzNAtmTIaQk08zifKLGQuIYioXItcAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"757f323059e6af55fc73540b03b7577cc404d79d13c989a143653af951db6c3f","last_reissued_at":"2026-05-18T00:57:43.090130Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:57:43.090130Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Models for Small-Scale Structure on Cosmic Strings: II. Scaling and its stability","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","gr-qc","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"C.J.A.P. Martins, E.P.S. Shellard, J. P. P. Vieira","submitted_at":"2016-11-18T14:38:51Z","abstract_excerpt":"We make use of the formalism described in a previous paper [Martins {\\it et al.} Phys. Rev. D90 (2014) 043518] to address general features of wiggly cosmic string evolution. In particular, we highlight the important role played by poorly understood energy loss mechanisms and propose a simple ansatz which tackles this problem in the context of an extended velocity-dependent one-scale model. We find a general procedure to determine all the scaling solutions admitted by a specific string model and study their stability, enabling a detailed comparison with future numerical simulations. A simpler c"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1611.06103","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":""},"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":"1611.06103","created_at":"2026-05-18T00:57:43.090202+00:00"},{"alias_kind":"arxiv_version","alias_value":"1611.06103v1","created_at":"2026-05-18T00:57:43.090202+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1611.06103","created_at":"2026-05-18T00:57:43.090202+00:00"},{"alias_kind":"pith_short_12","alias_value":"OV7TEMCZ42XV","created_at":"2026-05-18T12:30:36.002864+00:00"},{"alias_kind":"pith_short_16","alias_value":"OV7TEMCZ42XVL7DT","created_at":"2026-05-18T12:30:36.002864+00:00"},{"alias_kind":"pith_short_8","alias_value":"OV7TEMCZ","created_at":"2026-05-18T12:30:36.002864+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/OV7TEMCZ42XVL7DTKQFQHN2XPT","json":"https://pith.science/pith/OV7TEMCZ42XVL7DTKQFQHN2XPT.json","graph_json":"https://pith.science/api/pith-number/OV7TEMCZ42XVL7DTKQFQHN2XPT/graph.json","events_json":"https://pith.science/api/pith-number/OV7TEMCZ42XVL7DTKQFQHN2XPT/events.json","paper":"https://pith.science/paper/OV7TEMCZ"},"agent_actions":{"view_html":"https://pith.science/pith/OV7TEMCZ42XVL7DTKQFQHN2XPT","download_json":"https://pith.science/pith/OV7TEMCZ42XVL7DTKQFQHN2XPT.json","view_paper":"https://pith.science/paper/OV7TEMCZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1611.06103&json=true","fetch_graph":"https://pith.science/api/pith-number/OV7TEMCZ42XVL7DTKQFQHN2XPT/graph.json","fetch_events":"https://pith.science/api/pith-number/OV7TEMCZ42XVL7DTKQFQHN2XPT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OV7TEMCZ42XVL7DTKQFQHN2XPT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OV7TEMCZ42XVL7DTKQFQHN2XPT/action/storage_attestation","attest_author":"https://pith.science/pith/OV7TEMCZ42XVL7DTKQFQHN2XPT/action/author_attestation","sign_citation":"https://pith.science/pith/OV7TEMCZ42XVL7DTKQFQHN2XPT/action/citation_signature","submit_replication":"https://pith.science/pith/OV7TEMCZ42XVL7DTKQFQHN2XPT/action/replication_record"}},"created_at":"2026-05-18T00:57:43.090202+00:00","updated_at":"2026-05-18T00:57:43.090202+00:00"}