{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:43TCURWJGDBNHKOKT3PHMYWHUM","short_pith_number":"pith:43TCURWJ","schema_version":"1.0","canonical_sha256":"e6e62a46c930c2d3a9ca9ede7662c7a305086573f1d97b7ecdaba2d88ad149a7","source":{"kind":"arxiv","id":"2007.07917","version":2},"attestation_state":"computed","paper":{"title":"Hidden Sector Monopole Dark Matter with Matter Domination","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-th"],"primary_cat":"hep-ph","authors_text":"Jacek K. Osi\\'nski, Michael L. Graesser","submitted_at":"2020-07-15T18:02:06Z","abstract_excerpt":"The thermal freeze-out mechanism for relic dark matter heavier than $O(10-100 $ TeV$)$ requires cross-sections that violate perturbative unitarity. Yet the existence of dark matter heavier than these scales is certainly plausible from a particle physics perspective, pointing to the need for a non-thermal cosmological history for such theories. Topological dark matter is a well-motivated scenario of this kind. Here the hidden-sector dark matter can be produced in abundance through the Kibble-Zurek mechanism describing the non-equilibrium dynamics of defects produced in a second order phase tran"},"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":"2007.07917","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2020-07-15T18:02:06Z","cross_cats_sorted":["astro-ph.CO","hep-th"],"title_canon_sha256":"2fe5ff1957c5ec3f35ba8fa1bd708f1dce5e02b0fa09ecc92cf7668dca296ef5","abstract_canon_sha256":"0d524900e7ff3b70aecd8c80431ea731ff0c39f0344b0a1c7bfa6b01d6952dfa"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:02:40.715387Z","signature_b64":"ZJ2nqygJx3PKaky6CV+HUfTExnJl21YLmbAaCMCW3cQncQD9xqk759y2Os9j1SLdNrWEY3iHyN7H1lEV2GfaCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e6e62a46c930c2d3a9ca9ede7662c7a305086573f1d97b7ecdaba2d88ad149a7","last_reissued_at":"2026-07-05T02:02:40.714909Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:02:40.714909Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Hidden Sector Monopole Dark Matter with Matter Domination","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-th"],"primary_cat":"hep-ph","authors_text":"Jacek K. Osi\\'nski, Michael L. Graesser","submitted_at":"2020-07-15T18:02:06Z","abstract_excerpt":"The thermal freeze-out mechanism for relic dark matter heavier than $O(10-100 $ TeV$)$ requires cross-sections that violate perturbative unitarity. Yet the existence of dark matter heavier than these scales is certainly plausible from a particle physics perspective, pointing to the need for a non-thermal cosmological history for such theories. Topological dark matter is a well-motivated scenario of this kind. Here the hidden-sector dark matter can be produced in abundance through the Kibble-Zurek mechanism describing the non-equilibrium dynamics of defects produced in a second order phase tran"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2007.07917","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/2007.07917/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":"2007.07917","created_at":"2026-07-05T02:02:40.714969+00:00"},{"alias_kind":"arxiv_version","alias_value":"2007.07917v2","created_at":"2026-07-05T02:02:40.714969+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2007.07917","created_at":"2026-07-05T02:02:40.714969+00:00"},{"alias_kind":"pith_short_12","alias_value":"43TCURWJGDBN","created_at":"2026-07-05T02:02:40.714969+00:00"},{"alias_kind":"pith_short_16","alias_value":"43TCURWJGDBNHKOK","created_at":"2026-07-05T02:02:40.714969+00:00"},{"alias_kind":"pith_short_8","alias_value":"43TCURWJ","created_at":"2026-07-05T02:02:40.714969+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.21281","citing_title":"Self-Consistent Parker Bound on Magnetic Monopoles","ref_index":34,"is_internal_anchor":false},{"citing_arxiv_id":"2604.19873","citing_title":"Self-Interaction and Galactic Magnetic Field Bounds on Millicharged Magnetic Monopole Dark Matter","ref_index":44,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/43TCURWJGDBNHKOKT3PHMYWHUM","json":"https://pith.science/pith/43TCURWJGDBNHKOKT3PHMYWHUM.json","graph_json":"https://pith.science/api/pith-number/43TCURWJGDBNHKOKT3PHMYWHUM/graph.json","events_json":"https://pith.science/api/pith-number/43TCURWJGDBNHKOKT3PHMYWHUM/events.json","paper":"https://pith.science/paper/43TCURWJ"},"agent_actions":{"view_html":"https://pith.science/pith/43TCURWJGDBNHKOKT3PHMYWHUM","download_json":"https://pith.science/pith/43TCURWJGDBNHKOKT3PHMYWHUM.json","view_paper":"https://pith.science/paper/43TCURWJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2007.07917&json=true","fetch_graph":"https://pith.science/api/pith-number/43TCURWJGDBNHKOKT3PHMYWHUM/graph.json","fetch_events":"https://pith.science/api/pith-number/43TCURWJGDBNHKOKT3PHMYWHUM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/43TCURWJGDBNHKOKT3PHMYWHUM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/43TCURWJGDBNHKOKT3PHMYWHUM/action/storage_attestation","attest_author":"https://pith.science/pith/43TCURWJGDBNHKOKT3PHMYWHUM/action/author_attestation","sign_citation":"https://pith.science/pith/43TCURWJGDBNHKOKT3PHMYWHUM/action/citation_signature","submit_replication":"https://pith.science/pith/43TCURWJGDBNHKOKT3PHMYWHUM/action/replication_record"}},"created_at":"2026-07-05T02:02:40.714969+00:00","updated_at":"2026-07-05T02:02:40.714969+00:00"}