{"as_of":"2026-08-08T10:41:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:4e7776b4d1a5cc266337706db7d5f4349010f0bb5e1abf2a1d284c4033591294","coverage":[{"denominator":28,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":28,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T22:37:11.820009Z","state":"measured"},{"denominator":28,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":28,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-08T06:32:00.761636+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2506.21494/citation-record","integrity":"/paper/2506.21494/integrity","json":"/paper/2506.21494/citation-record.json","paper":"/paper/2506.21494"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T22:37:08.709852Z","title":null,"venue":null,"work_id":null,"year":1976},"citing_paper":{"arxiv_id":"2506.21494","last_updated":"2025-06-26T17:22:47Z","snapshot_observed_at":"2026-08-07T23:45:22.319419Z","submitted_at":"2025-06-26T17:22:47Z","title":"Scaling solutions for current-carrying cosmic string networks. II. Biased solutions","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-06T22:37:08.709852Z"},"links":{"citing_paper":"/paper/2506.21494"},"observation_digest":"sha256:e31e4abdbaadf0bd8f456185f7419247809f92f30ad4cb9102d5c3d91306329f","observation_id":"c979a6c6-c36c-4756-8a84-453ecabbd773","resolution":{"observed_at":"2026-08-06T22:37:08.709852Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T22:37:08.776948Z","title":"Vilenkin and E","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2506.21494","last_updated":"2025-06-26T17:22:47Z","snapshot_observed_at":"2026-08-07T23:45:22.319419Z","submitted_at":"2025-06-26T17:22:47Z","title":"Scaling solutions for current-carrying cosmic string networks. II. Biased solutions","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-06T22:37:08.776948Z"},"links":{"citing_paper":"/paper/2506.21494"},"observation_digest":"sha256:54d21e4a43069ba124d69bea4afb7141c105a6e5f6822b93ae2ef7268d44e9b5","observation_id":"16c8f0fc-565c-4988-8df0-cf898efd21b7","resolution":{"observed_at":"2026-08-06T22:37:08.776948Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T22:37:16.230827Z","title":"Witten, Superconducting Strings, Nucl","venue":null,"work_id":"36a97e8c-161a-4478-b259-634059be3cf4","year":1985},"citing_paper":{"arxiv_id":"2506.21494","last_updated":"2025-06-26T17:22:47Z","snapshot_observed_at":"2026-08-07T23:45:22.319419Z","submitted_at":"2025-06-26T17:22:47Z","title":"Scaling solutions for current-carrying cosmic string networks. II. Biased solutions","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-06T22:37:08.893337Z"},"links":{"citing_paper":"/paper/2506.21494"},"observation_digest":"sha256:ff597fd5394a39680ef7a34a25958fe6e66efb70c4981c6a49b0b1e99fbee749","observation_id":"27533c6a-8bb2-4ec2-bc89-be3289e971df","resolution":{"observed_at":"2026-08-06T22:37:16.290162Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T22:37:16.080080Z","title":"Witten, Cosmic Superstrings, Phys","venue":null,"work_id":"e851e758-6569-45bf-9bb8-32474c7da49c","year":1985},"citing_paper":{"arxiv_id":"2506.21494","last_updated":"2025-06-26T17:22:47Z","snapshot_observed_at":"2026-08-07T23:45:22.319419Z","submitted_at":"2025-06-26T17:22:47Z","title":"Scaling solutions for current-carrying cosmic string networks. II. Biased solutions","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-06T22:37:08.983987Z"},"links":{"citing_paper":"/paper/2506.21494"},"observation_digest":"sha256:bb123d346a23c23c3bed00bcd68c0314e88068707ece75a2524335f843917c56","observation_id":"d63de34a-88df-4cd6-8fec-f80be45b547d","resolution":{"observed_at":"2026-08-06T22:37:16.156197Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0911.1345","last_updated":"2009-11-26T17:22:37Z","snapshot_observed_at":"2026-07-06T01:59:52.714720Z","submitted_at":"2009-11-06T20:26:57Z","title":"Cosmic Strings and Superstrings","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0911.1345","snapshot_observed_at":"2026-08-06T22:37:09.068707Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2506.21494","last_updated":"2025-06-26T17:22:47Z","snapshot_observed_at":"2026-08-07T23:45:22.319419Z","submitted_at":"2025-06-26T17:22:47Z","title":"Scaling solutions for current-carrying cosmic string networks. II. Biased solutions","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-06T22:37:09.068707Z"},"links":{"cited_paper":"/paper/0911.1345","citing_paper":"/paper/2506.21494"},"observation_digest":"sha256:7a880214a55150791728b0b33c6272736d884645d382e1771856975bf873c2fe","observation_id":"8c9f95de-e611-4a9a-a917-8da1a6637e0b","resolution":{"observed_at":"2026-08-06T22:37:09.068707Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T22:37:15.891463Z","title":null,"venue":null,"work_id":"904a85b1-8a31-4965-afd9-17cf4174972d","year":1986},"citing_paper":{"arxiv_id":"2506.21494","last_updated":"2025-06-26T17:22:47Z","snapshot_observed_at":"2026-08-07T23:45:22.319419Z","submitted_at":"2025-06-26T17:22:47Z","title":"Scaling solutions for current-carrying cosmic string networks. II. Biased solutions","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-06T22:37:09.174945Z"},"links":{"citing_paper":"/paper/2506.21494"},"observation_digest":"sha256:cbe9d04c35d594deb25b5603d244fe945de0ea243f49611fb47a576b0ddeb97e","observation_id":"72f73d9a-6034-4c25-a7c5-1b108579cbc0","resolution":{"observed_at":"2026-08-06T22:37:15.979254Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T22:37:15.707221Z","title":"Vilenkin and T","venue":null,"work_id":"9adffeae-9ddd-4814-848a-0a73701585cc","year":1987},"citing_paper":{"arxiv_id":"2506.21494","last_updated":"2025-06-26T17:22:47Z","snapshot_observed_at":"2026-08-07T23:45:22.319419Z","submitted_at":"2025-06-26T17:22:47Z","title":"Scaling solutions for current-carrying cosmic string networks. II. Biased solutions","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-06T22:37:09.296441Z"},"links":{"citing_paper":"/paper/2506.21494"},"observation_digest":"sha256:1e41d31b8c302f3d741f877d6a9d906b74beddd95c0989b8976b7c488e24ab8a","observation_id":"8570c1bc-ff73-429a-8056-0c4621dcd40c","resolution":{"observed_at":"2026-08-06T22:37:15.795399Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0506138","last_updated":"2005-06-16T16:04:58Z","snapshot_observed_at":"2026-07-07T04:54:20.781743Z","submitted_at":"2005-06-16T16:04:58Z","title":"A practical model for cosmic (p,q) superstrings","version":1},"cited_work":{"arxiv_id":"hep-th/0506138","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-th/0506138","snapshot_observed_at":"2026-08-06T22:37:14.118823Z","title":"A practical model for cosmic (p,q) superstrings","venue":"hep-th","work_id":"242418f0-4858-422a-992b-5cc4c618b8c9","year":2005},"citing_paper":{"arxiv_id":"2506.21494","last_updated":"2025-06-26T17:22:47Z","snapshot_observed_at":"2026-08-07T23:45:22.319419Z","submitted_at":"2025-06-26T17:22:47Z","title":"Scaling solutions for current-carrying cosmic string networks. II. Biased solutions","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-06T22:37:09.462822Z"},"links":{"cited_paper":"/paper/hep-th/0506138","citing_paper":"/paper/2506.21494"},"observation_digest":"sha256:3bd3921a6231f97c9b572d440475bc26980161aae7849982f0c9c1f142599438","observation_id":"487e8ca1-10bb-4ba2-a34c-c41a9fabfaee","resolution":{"observed_at":"2026-08-06T22:37:14.198891Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0712.1146","last_updated":"2008-02-11T13:57:05Z","snapshot_observed_at":"2026-07-06T01:33:43.553947Z","submitted_at":"2007-12-07T14:10:41Z","title":"Evolution of cosmic superstring networks: a numerical simulation","version":2},"cited_work":{"arxiv_id":"0712.1146","doi":null,"metadata_source":"pith","pith_arxiv_id":"0712.1146","snapshot_observed_at":"2026-08-06T22:37:13.915657Z","title":"Evolution of cosmic superstring networks: a numerical simulation","venue":"hep-th","work_id":"e4c71fd0-5475-4bbf-aaad-4725c409784f","year":2007},"citing_paper":{"arxiv_id":"2506.21494","last_updated":"2025-06-26T17:22:47Z","snapshot_observed_at":"2026-08-07T23:45:22.319419Z","submitted_at":"2025-06-26T17:22:47Z","title":"Scaling solutions for current-carrying cosmic string networks. II. Biased solutions","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-06T22:37:09.557912Z"},"links":{"cited_paper":"/paper/0712.1146","citing_paper":"/paper/2506.21494"},"observation_digest":"sha256:54d4732564ac10f80304bcdc0ffbbf898bdef521f020f5e35994c120c74e006f","observation_id":"6d6d0504-5578-442d-b0e2-d4f5f831fe0b","resolution":{"observed_at":"2026-08-06T22:37:14.022603Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1602.08014","last_updated":"2016-04-27T14:13:50Z","snapshot_observed_at":"2026-07-06T04:47:23.881795Z","submitted_at":"2016-02-25T17:53:54Z","title":"Survival of pq-superstrings in field theory simulations","version":2},"cited_work":{"arxiv_id":"1602.08014","doi":null,"metadata_source":"pith","pith_arxiv_id":"1602.08014","snapshot_observed_at":"2026-08-06T22:37:13.754538Z","title":"Survival of pq-superstrings in field theory simulations","venue":"astro-ph.CO","work_id":"70364303-a9ac-4eb3-a8dd-e54d411eb058","year":2016},"citing_paper":{"arxiv_id":"2506.21494","last_updated":"2025-06-26T17:22:47Z","snapshot_observed_at":"2026-08-07T23:45:22.319419Z","submitted_at":"2025-06-26T17:22:47Z","title":"Scaling solutions for current-carrying cosmic string networks. II. Biased solutions","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-06T22:37:09.640394Z"},"links":{"cited_paper":"/paper/1602.08014","citing_paper":"/paper/2506.21494"},"observation_digest":"sha256:23c07b0ba24300b03b87de2d992c597110fb01ae6b66897ebc19d76df22d39a3","observation_id":"aec7d151-41d2-4aa3-9638-5f3cce65d58e","resolution":{"observed_at":"2026-08-06T22:37:13.824330Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T22:37:15.530911Z","title":null,"venue":null,"work_id":"b5f54176-9af8-4992-9084-e39851e1bb5f","year":2022},"citing_paper":{"arxiv_id":"2506.21494","last_updated":"2025-06-26T17:22:47Z","snapshot_observed_at":"2026-08-07T23:45:22.319419Z","submitted_at":"2025-06-26T17:22:47Z","title":"Scaling solutions for current-carrying cosmic string networks. II. Biased solutions","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-06T22:37:09.760927Z"},"links":{"citing_paper":"/paper/2506.21494"},"observation_digest":"sha256:0848702f8d4f651dc4e54157dc381208063fb2b1b5acff712c1d471b3e42a381","observation_id":"5fb77cac-a33a-4329-a149-bf5063197157","resolution":{"observed_at":"2026-08-06T22:37:15.612985Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2212.06491","last_updated":"2022-12-13T11:17:02Z","snapshot_observed_at":"2026-07-06T14:29:57.303212Z","submitted_at":"2022-12-13T11:17:02Z","title":"Pinching instabilities in superconducting strings","version":1},"cited_work":{"arxiv_id":"2212.06491","doi":null,"metadata_source":"pith","pith_arxiv_id":"2212.06491","snapshot_observed_at":"2026-08-06T22:37:13.571297Z","title":"Pinching instabilities in superconducting strings","venue":"hep-ph","work_id":"acc9edef-3ad4-4a62-a408-82f413109953","year":2022},"citing_paper":{"arxiv_id":"2506.21494","last_updated":"2025-06-26T17:22:47Z","snapshot_observed_at":"2026-08-07T23:45:22.319419Z","submitted_at":"2025-06-26T17:22:47Z","title":"Scaling solutions for current-carrying cosmic string networks. II. Biased solutions","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-06T22:37:09.851894Z"},"links":{"cited_paper":"/paper/2212.06491","citing_paper":"/paper/2506.21494"},"observation_digest":"sha256:90d427087313249167527432ff28f70a9c35fef87595f1de610774ec11e1e993","observation_id":"232e1718-e882-4b90-80a2-4c15ce4c67d7","resolution":{"observed_at":"2026-08-06T22:37:13.677339Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2406.03931","last_updated":"2024-06-06T10:17:35Z","snapshot_observed_at":"2026-07-06T18:26:23.994796Z","submitted_at":"2024-06-06T10:17:35Z","title":"Evolution of current-carrying string networks","version":1},"cited_work":{"arxiv_id":"2406.03931","doi":null,"metadata_source":"pith","pith_arxiv_id":"2406.03931","snapshot_observed_at":"2026-08-06T22:37:13.423543Z","title":"Evolution of current-carrying string networks","venue":"hep-ph","work_id":"6de147c1-c401-4cbc-b011-f1c224ebd458","year":2024},"citing_paper":{"arxiv_id":"2506.21494","last_updated":"2025-06-26T17:22:47Z","snapshot_observed_at":"2026-08-07T23:45:22.319419Z","submitted_at":"2025-06-26T17:22:47Z","title":"Scaling solutions for current-carrying cosmic string networks. II. Biased solutions","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-06T22:37:09.945324Z"},"links":{"cited_paper":"/paper/2406.03931","citing_paper":"/paper/2506.21494"},"observation_digest":"sha256:c41720e0ae39b7df6d05476bea3c84f3507d502a67927c20fea7857651da1f01","observation_id":"8f6ea475-48a7-4af2-ad05-27607eacc9aa","resolution":{"observed_at":"2026-08-06T22:37:13.482434Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9602271","last_updated":"1996-02-13T07:53:36Z","snapshot_observed_at":"2026-07-07T04:21:54.735991Z","submitted_at":"1996-02-12T09:55:21Z","title":"Quantitative String Evolution","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/9602271","snapshot_observed_at":"2026-08-06T22:37:10.042912Z","title":null,"venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2506.21494","last_updated":"2025-06-26T17:22:47Z","snapshot_observed_at":"2026-08-07T23:45:22.319419Z","submitted_at":"2025-06-26T17:22:47Z","title":"Scaling solutions for current-carrying cosmic string networks. II. Biased solutions","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-06T22:37:10.042912Z"},"links":{"cited_paper":"/paper/hep-ph/9602271","citing_paper":"/paper/2506.21494"},"observation_digest":"sha256:3c3273c5ce1a1f0d689fea7ff148aa83f6c285558ed710e06d05aab271c94534","observation_id":"41749adc-29d6-4f4d-bfc1-bff649d0c72a","resolution":{"observed_at":"2026-08-06T22:37:10.042912Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T22:37:15.378682Z","title":null,"venue":null,"work_id":"20422ac0-363b-4bc7-8d6d-5f8b46cc74f7","year":2002},"citing_paper":{"arxiv_id":"2506.21494","last_updated":"2025-06-26T17:22:47Z","snapshot_observed_at":"2026-08-07T23:45:22.319419Z","submitted_at":"2025-06-26T17:22:47Z","title":"Scaling solutions for current-carrying cosmic string networks. II. Biased solutions","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-06T22:37:10.153579Z"},"links":{"citing_paper":"/paper/2506.21494"},"observation_digest":"sha256:4a20032b1efc2ed46c3661daccfd27bf9afb07a0b01f1db4cce2b12c15596bd2","observation_id":"e93aae11-3a5d-4a93-aa22-7f4d19a6989a","resolution":{"observed_at":"2026-08-06T22:37:15.465642Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T22:37:15.200110Z","title":"Martins, Defect Evolution in Cosmology and Con- densed Matter: Quantitative Analysis with the Velocity- Dependent One-Scale Model , 1st ed","venue":null,"work_id":"82f114b5-81c5-4546-8895-88a57e21cd90","year":2016},"citing_paper":{"arxiv_id":"2506.21494","last_updated":"2025-06-26T17:22:47Z","snapshot_observed_at":"2026-08-07T23:45:22.319419Z","submitted_at":"2025-06-26T17:22:47Z","title":"Scaling solutions for current-carrying cosmic string networks. II. Biased solutions","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-06T22:37:10.219374Z"},"links":{"citing_paper":"/paper/2506.21494"},"observation_digest":"sha256:b091f59da47edcb066765e1817f7479288a1235bcb262f0bdfd03c87935801b2","observation_id":"5a19547b-353b-4bb0-b1da-1e622b854f47","resolution":{"observed_at":"2026-08-06T22:37:15.288045Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2011.09700","last_updated":"2020-11-19T07:37:42Z","snapshot_observed_at":"2026-08-04T22:26:50.923819Z","submitted_at":"2020-11-19T07:37:42Z","title":"Generalised velocity-dependent one-scale model for current-carrying strings","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.09700","snapshot_observed_at":"2026-08-06T22:37:10.392942Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2506.21494","last_updated":"2025-06-26T17:22:47Z","snapshot_observed_at":"2026-08-07T23:45:22.319419Z","submitted_at":"2025-06-26T17:22:47Z","title":"Scaling solutions for current-carrying cosmic string networks. II. Biased solutions","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-06T22:37:10.392942Z"},"links":{"cited_paper":"/paper/2011.09700","citing_paper":"/paper/2506.21494"},"observation_digest":"sha256:c1f39e75c54b014beaf9ac4bd66832e04fcce6c80920838a0972319628370b45","observation_id":"e8d7614d-f245-4f87-838c-b1631b0d110e","resolution":{"observed_at":"2026-08-06T22:37:10.392942Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2304.00053","last_updated":"2023-03-31T18:14:43Z","snapshot_observed_at":"2026-08-04T12:06:07.893368Z","submitted_at":"2023-03-31T18:14:43Z","title":"Cosmological evolution of Witten superconducting string networks","version":1},"cited_work":{"arxiv_id":"2304.00053","doi":null,"metadata_source":"pith","pith_arxiv_id":"2304.00053","snapshot_observed_at":"2026-08-06T22:37:13.163987Z","title":"Cosmological evolution of Witten superconducting string networks","venue":"astro-ph.CO","work_id":"a17bdaf5-9945-4ce4-88d9-7ba346d2d62c","year":2023},"citing_paper":{"arxiv_id":"2506.21494","last_updated":"2025-06-26T17:22:47Z","snapshot_observed_at":"2026-08-07T23:45:22.319419Z","submitted_at":"2025-06-26T17:22:47Z","title":"Scaling solutions for current-carrying cosmic string networks. II. Biased solutions","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-06T22:37:10.547249Z"},"links":{"cited_paper":"/paper/2304.00053","citing_paper":"/paper/2506.21494"},"observation_digest":"sha256:f8a83a7e84eccf87ded8b5de92f0ef6e72d00f3162385cd32d0518745ebdca7f","observation_id":"7aa80806-81d3-4ed0-ab95-2bc59142d6e0","resolution":{"observed_at":"2026-08-06T22:37:13.280147Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2108.07513","last_updated":"2021-08-17T08:57:20Z","snapshot_observed_at":"2026-07-06T11:38:52.634811Z","submitted_at":"2021-08-17T08:57:20Z","title":"High resolution calibration of the cosmic strings velocity dependent one-scale model","version":1},"cited_work":{"arxiv_id":"2108.07513","doi":null,"metadata_source":"pith","pith_arxiv_id":"2108.07513","snapshot_observed_at":"2026-08-06T22:37:12.919288Z","title":"High resolution calibration of the cosmic strings velocity dependent one-scale model","venue":"astro-ph.CO","work_id":"ee61b4b1-37a3-40a6-8cc7-4cd16b96ebca","year":2021},"citing_paper":{"arxiv_id":"2506.21494","last_updated":"2025-06-26T17:22:47Z","snapshot_observed_at":"2026-08-07T23:45:22.319419Z","submitted_at":"2025-06-26T17:22:47Z","title":"Scaling solutions for current-carrying cosmic string networks. II. Biased solutions","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-06T22:37:10.707801Z"},"links":{"cited_paper":"/paper/2108.07513","citing_paper":"/paper/2506.21494"},"observation_digest":"sha256:d2b632f9bc6d8a2e92190d8243b61cc4f032d8300a19b6a9539a45073cc390b9","observation_id":"ca2a66e1-ebbb-41fa-b3e9-edc2dc23bfdc","resolution":{"observed_at":"2026-08-06T22:37:13.030689Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2406.03940","last_updated":"2024-06-06T10:28:05Z","snapshot_observed_at":"2026-07-06T18:26:23.994796Z","submitted_at":"2024-06-06T10:28:05Z","title":"Scaling solutions for current-carrying cosmic string networks","version":1},"cited_work":{"arxiv_id":"2406.03940","doi":null,"metadata_source":"pith","pith_arxiv_id":"2406.03940","snapshot_observed_at":"2026-08-06T22:37:12.676450Z","title":"Scaling solutions for current-carrying cosmic string networks","venue":"hep-ph","work_id":"292e6a47-2c11-4b09-8e2f-9edce0c42496","year":2024},"citing_paper":{"arxiv_id":"2506.21494","last_updated":"2025-06-26T17:22:47Z","snapshot_observed_at":"2026-08-07T23:45:22.319419Z","submitted_at":"2025-06-26T17:22:47Z","title":"Scaling solutions for current-carrying cosmic string networks. II. Biased solutions","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-06T22:37:10.820289Z"},"links":{"cited_paper":"/paper/2406.03940","citing_paper":"/paper/2506.21494"},"observation_digest":"sha256:4bad941dd04b8e6a63566b0a19d8b12eef01d178942a6256f0a26f36581bd1f3","observation_id":"f3a64352-0c5e-4544-9cf9-7cc731c33bfc","resolution":{"observed_at":"2026-08-06T22:37:12.788034Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T22:37:15.018594Z","title":null,"venue":null,"work_id":"95a0d2a8-9a38-4bdc-848a-48864549b248","year":2012},"citing_paper":{"arxiv_id":"2506.21494","last_updated":"2025-06-26T17:22:47Z","snapshot_observed_at":"2026-08-07T23:45:22.319419Z","submitted_at":"2025-06-26T17:22:47Z","title":"Scaling solutions for current-carrying cosmic string networks. II. Biased solutions","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-06T22:37:10.986519Z"},"links":{"citing_paper":"/paper/2506.21494"},"observation_digest":"sha256:2c6de95a21eef46a5c477f0d0d43154aa7c3184addd72d3ac2a297abf4e974f0","observation_id":"712c0f75-83bc-4847-b44e-8d5d769e3274","resolution":{"observed_at":"2026-08-06T22:37:15.098061Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T22:37:14.831718Z","title":null,"venue":null,"work_id":"88488537-bc05-46a6-bb1e-c89dd9da60eb","year":2021},"citing_paper":{"arxiv_id":"2506.21494","last_updated":"2025-06-26T17:22:47Z","snapshot_observed_at":"2026-08-07T23:45:22.319419Z","submitted_at":"2025-06-26T17:22:47Z","title":"Scaling solutions for current-carrying cosmic string networks. II. Biased solutions","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-06T22:37:11.147864Z"},"links":{"citing_paper":"/paper/2506.21494"},"observation_digest":"sha256:b65349fb45ad63a87056670318831231d65e5bffea5eb67069b616e4becd3b02","observation_id":"8117c492-0c09-4931-acbe-71c87607788d","resolution":{"observed_at":"2026-08-06T22:37:14.920109Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T22:37:14.629134Z","title":null,"venue":null,"work_id":"fac7e3e8-7b5d-4dea-a672-0197d1c41437","year":2022},"citing_paper":{"arxiv_id":"2506.21494","last_updated":"2025-06-26T17:22:47Z","snapshot_observed_at":"2026-08-07T23:45:22.319419Z","submitted_at":"2025-06-26T17:22:47Z","title":"Scaling solutions for current-carrying cosmic string networks. II. Biased solutions","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-06T22:37:11.304014Z"},"links":{"citing_paper":"/paper/2506.21494"},"observation_digest":"sha256:4790aea200985d4eaf525b0abb1a8a5a8bf1c07b81f028e68e4c93382b73b6e2","observation_id":"30ae7d3e-90cf-4721-a5a8-8d9241fea4cd","resolution":{"observed_at":"2026-08-06T22:37:14.707625Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T22:37:14.457584Z","title":null,"venue":null,"work_id":"31b59cd6-8a7e-4e92-955a-0cc70106e271","year":2023},"citing_paper":{"arxiv_id":"2506.21494","last_updated":"2025-06-26T17:22:47Z","snapshot_observed_at":"2026-08-07T23:45:22.319419Z","submitted_at":"2025-06-26T17:22:47Z","title":"Scaling solutions for current-carrying cosmic string networks. II. Biased solutions","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-06T22:37:11.426584Z"},"links":{"citing_paper":"/paper/2506.21494"},"observation_digest":"sha256:c29a50fedc75dbda1409fe7bf66c50e48dd83beafe16bea2a6e4ecc29adbd4cf","observation_id":"d7429537-d7d4-4fcf-9fb7-12ee028123a9","resolution":{"observed_at":"2026-08-06T22:37:14.536891Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2108.03147","last_updated":"2021-10-14T15:39:08Z","snapshot_observed_at":"2026-08-06T03:53:44.583812Z","submitted_at":"2021-08-06T14:42:35Z","title":"Charge-velocity-dependent one-scale linear model","version":2},"cited_work":{"arxiv_id":"2108.03147","doi":null,"metadata_source":"pith","pith_arxiv_id":"2108.03147","snapshot_observed_at":"2026-08-06T22:37:12.424311Z","title":"Charge-velocity-dependent one-scale linear model","venue":"astro-ph.CO","work_id":"c178543e-a2f3-41f1-b812-4fa03d8484f7","year":2021},"citing_paper":{"arxiv_id":"2506.21494","last_updated":"2025-06-26T17:22:47Z","snapshot_observed_at":"2026-08-07T23:45:22.319419Z","submitted_at":"2025-06-26T17:22:47Z","title":"Scaling solutions for current-carrying cosmic string networks. II. Biased solutions","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-06T22:37:11.509683Z"},"links":{"cited_paper":"/paper/2108.03147","citing_paper":"/paper/2506.21494"},"observation_digest":"sha256:85e4fffeef401e136c30372725a8180dfe4e7004dc130e11ce4796f3200e127d","observation_id":"7a5095a0-3f97-4903-8f2e-4027e248efa3","resolution":{"observed_at":"2026-08-06T22:37:12.537179Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T22:37:14.303379Z","title":null,"venue":null,"work_id":"a98f7a22-deba-4f06-ab71-065b00a6f565","year":1998},"citing_paper":{"arxiv_id":"2506.21494","last_updated":"2025-06-26T17:22:47Z","snapshot_observed_at":"2026-08-07T23:45:22.319419Z","submitted_at":"2025-06-26T17:22:47Z","title":"Scaling solutions for current-carrying cosmic string networks. II. Biased solutions","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-06T22:37:11.604140Z"},"links":{"citing_paper":"/paper/2506.21494"},"observation_digest":"sha256:de57b0a4b0b305e04ed87b2d27af0e86d38bd4d6a83656439b0d2dc7552fe503","observation_id":"053e0fd7-f570-4405-8995-69f5eee070bf","resolution":{"observed_at":"2026-08-06T22:37:14.351456Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1809.00995","last_updated":"2020-04-28T09:49:43Z","snapshot_observed_at":"2026-07-06T06:59:05.580891Z","submitted_at":"2018-08-30T11:04:21Z","title":"Abelian-Higgs Cosmic String Evolution with CUDA","version":2},"cited_work":{"arxiv_id":"1809.00995","doi":null,"metadata_source":"pith","pith_arxiv_id":"1809.00995","snapshot_observed_at":"2026-08-06T22:37:12.178375Z","title":"Abelian-Higgs Cosmic String Evolution with CUDA","venue":"physics.comp-ph","work_id":"d66345a0-282d-45d3-a321-79dc044d20a9","year":2018},"citing_paper":{"arxiv_id":"2506.21494","last_updated":"2025-06-26T17:22:47Z","snapshot_observed_at":"2026-08-07T23:45:22.319419Z","submitted_at":"2025-06-26T17:22:47Z","title":"Scaling solutions for current-carrying cosmic string networks. II. Biased solutions","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-06T22:37:11.722083Z"},"links":{"cited_paper":"/paper/1809.00995","citing_paper":"/paper/2506.21494"},"observation_digest":"sha256:3d374165967b4585fda85b130c102b6fdad773a0ec7d06620cd3dea7e1248a5f","observation_id":"d6143854-0c8c-4ae9-a327-49468f1ee743","resolution":{"observed_at":"2026-08-06T22:37:12.267929Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2005.14454","last_updated":"2020-11-18T16:35:29Z","snapshot_observed_at":"2026-08-04T13:51:23.623560Z","submitted_at":"2020-05-29T08:59:06Z","title":"Abelian-Higgs cosmic string evolution with multiple GPUs","version":2},"cited_work":{"arxiv_id":"2005.14454","doi":null,"metadata_source":"pith","pith_arxiv_id":"2005.14454","snapshot_observed_at":"2026-08-06T22:37:11.948872Z","title":"Abelian-Higgs cosmic string evolution with multiple GPUs","venue":"physics.comp-ph","work_id":"f728ddc8-2b5c-48a3-9170-775c868b46d9","year":2020},"citing_paper":{"arxiv_id":"2506.21494","last_updated":"2025-06-26T17:22:47Z","snapshot_observed_at":"2026-08-07T23:45:22.319419Z","submitted_at":"2025-06-26T17:22:47Z","title":"Scaling solutions for current-carrying cosmic string networks. II. Biased solutions","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-06T22:37:11.820009Z"},"links":{"cited_paper":"/paper/2005.14454","citing_paper":"/paper/2506.21494"},"observation_digest":"sha256:3160d9b49da8a34ec918ea3e1041ebd4b21c698070fd9cae537f01cbbb15d1ed","observation_id":"7b9ad31d-4ac2-4e3f-b28f-d4889afbf781","resolution":{"observed_at":"2026-08-06T22:37:12.044965Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2506.21494","last_updated":"2025-06-26T17:22:47Z","latest_version":1,"primary_category":"hep-ph","snapshot_observed_at":"2026-08-07T23:45:22.319419Z","submitted_at":"2025-06-26T17:22:47Z","title":"Scaling solutions for current-carrying cosmic string networks. II. Biased solutions"},"reference_resolution":{"displayed":28,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":13,"verified_exact":11,"verified_fuzzy":4},"total_outbound_references":28},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"thesis":"As of 8 August 2026, this Paper Citation Record lists 28 of 28 outbound references and 0 inbound Pith citation observations for arXiv:2506.21494."}