{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:3YKMVRZYAOZIUIXEE5DAU4MZNH","short_pith_number":"pith:3YKMVRZY","schema_version":"1.0","canonical_sha256":"de14cac73803b28a22e427460a719969e60cdeae7a349caef7d2f0722a595392","source":{"kind":"arxiv","id":"1006.0687","version":2},"attestation_state":"computed","paper":{"title":"Analytical model for CMB temperature angular power spectrum from cosmic (super-)strings","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Chul-Moon Yoo, Daisuke Yamauchi, Keitaro Takahashi, Misao Sasaki, Yuuiti Sendouda","submitted_at":"2010-06-03T16:17:59Z","abstract_excerpt":"We present a new analytical method to calculate the small angle CMB temperature angular power spectrum due to cosmic (super-)string segments. In particular, using our method, we clarify the dependence on the intercommuting probability $P$. We find that the power spectrum is dominated by Poisson-distributed string segments. The power spectrum for a general value of $P$ has a plateau on large angular scales and shows a power-law decrease on small angular scales. The resulting spectrum in the case of conventional cosmic strings is in very good agreement with the numerical result obtained by Frais"},"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":"1006.0687","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-06-03T16:17:59Z","cross_cats_sorted":["gr-qc","hep-ph"],"title_canon_sha256":"0321ab3b27c29b9e79f17a90552a5471284ce03f03d6ef21006e04cea2570a95","abstract_canon_sha256":"37b66858dc7d7a278fe89a321c40cf2d5f4122e4e0597e3df92a022bb8f2ff7e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:33:18.054237Z","signature_b64":"KZMS4RctcHm0gzjpuSu5bATi0HaPV40o8YUiJ3cmdz7MtqkOERvnmVDFOAtg6e3Hq4xEq+7N3XJ9h3l6ZDgrCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"de14cac73803b28a22e427460a719969e60cdeae7a349caef7d2f0722a595392","last_reissued_at":"2026-05-18T02:33:18.053608Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:33:18.053608Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Analytical model for CMB temperature angular power spectrum from cosmic (super-)strings","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Chul-Moon Yoo, Daisuke Yamauchi, Keitaro Takahashi, Misao Sasaki, Yuuiti Sendouda","submitted_at":"2010-06-03T16:17:59Z","abstract_excerpt":"We present a new analytical method to calculate the small angle CMB temperature angular power spectrum due to cosmic (super-)string segments. In particular, using our method, we clarify the dependence on the intercommuting probability $P$. We find that the power spectrum is dominated by Poisson-distributed string segments. The power spectrum for a general value of $P$ has a plateau on large angular scales and shows a power-law decrease on small angular scales. The resulting spectrum in the case of conventional cosmic strings is in very good agreement with the numerical result obtained by Frais"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1006.0687","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":"1006.0687","created_at":"2026-05-18T02:33:18.053699+00:00"},{"alias_kind":"arxiv_version","alias_value":"1006.0687v2","created_at":"2026-05-18T02:33:18.053699+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1006.0687","created_at":"2026-05-18T02:33:18.053699+00:00"},{"alias_kind":"pith_short_12","alias_value":"3YKMVRZYAOZI","created_at":"2026-05-18T12:26:03.138858+00:00"},{"alias_kind":"pith_short_16","alias_value":"3YKMVRZYAOZIUIXE","created_at":"2026-05-18T12:26:03.138858+00:00"},{"alias_kind":"pith_short_8","alias_value":"3YKMVRZY","created_at":"2026-05-18T12:26:03.138858+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/3YKMVRZYAOZIUIXEE5DAU4MZNH","json":"https://pith.science/pith/3YKMVRZYAOZIUIXEE5DAU4MZNH.json","graph_json":"https://pith.science/api/pith-number/3YKMVRZYAOZIUIXEE5DAU4MZNH/graph.json","events_json":"https://pith.science/api/pith-number/3YKMVRZYAOZIUIXEE5DAU4MZNH/events.json","paper":"https://pith.science/paper/3YKMVRZY"},"agent_actions":{"view_html":"https://pith.science/pith/3YKMVRZYAOZIUIXEE5DAU4MZNH","download_json":"https://pith.science/pith/3YKMVRZYAOZIUIXEE5DAU4MZNH.json","view_paper":"https://pith.science/paper/3YKMVRZY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1006.0687&json=true","fetch_graph":"https://pith.science/api/pith-number/3YKMVRZYAOZIUIXEE5DAU4MZNH/graph.json","fetch_events":"https://pith.science/api/pith-number/3YKMVRZYAOZIUIXEE5DAU4MZNH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3YKMVRZYAOZIUIXEE5DAU4MZNH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3YKMVRZYAOZIUIXEE5DAU4MZNH/action/storage_attestation","attest_author":"https://pith.science/pith/3YKMVRZYAOZIUIXEE5DAU4MZNH/action/author_attestation","sign_citation":"https://pith.science/pith/3YKMVRZYAOZIUIXEE5DAU4MZNH/action/citation_signature","submit_replication":"https://pith.science/pith/3YKMVRZYAOZIUIXEE5DAU4MZNH/action/replication_record"}},"created_at":"2026-05-18T02:33:18.053699+00:00","updated_at":"2026-05-18T02:33:18.053699+00:00"}