{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:OIWYQ7LE6KMRJXG2I7CUWLHZSX","short_pith_number":"pith:OIWYQ7LE","schema_version":"1.0","canonical_sha256":"722d887d64f29914dcda47c54b2cf995e5141162d98ab5add94d50ab65a43e98","source":{"kind":"arxiv","id":"1004.4658","version":2},"attestation_state":"computed","paper":{"title":"Long-Lived Time-Dependent Remnants During Cosmological Symmetry Breaking: From Inflation to the Electroweak Scale","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"astro-ph.CO","authors_text":"Marcelo Gleiser, Nikitas Stamatopoulos, Noah Graham","submitted_at":"2010-04-26T21:11:59Z","abstract_excerpt":"Through a detailed numerical investigation in three spatial dimensions, we demonstrate that long-lived time-dependent field configurations emerge dynamically during symmetry breaking in an expanding de Sitter spacetime. We investigate two situations: a single scalar field with a double-well potential and the bosonic sector of an SU(2) non-Abelian Higgs model. For the single scalar, we show that large-amplitude oscillon configurations emerge spontaneously and persist to contribute about 1.2% of the energy density of the universe. We also show that for a range of parameters, oscillon lifetimes a"},"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":"1004.4658","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-04-26T21:11:59Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"6d349356ee9fef9180b36d0943a068c058de027c14b3d50e71887716676d2306","abstract_canon_sha256":"67986ac7064e94de0b6a3b1b3611f4764f2bd3109fdc2785ccab9aeb2d07b3bb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:41:36.632985Z","signature_b64":"1sys0Tkq7+/SagPNJY3NDo/yjJoJL8MR63D1k2wYc+iiI1Yen+A3cZ+fJPUiMk6yNCapVT5OH6C4qW2ajDmxCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"722d887d64f29914dcda47c54b2cf995e5141162d98ab5add94d50ab65a43e98","last_reissued_at":"2026-05-18T04:41:36.632537Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:41:36.632537Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Long-Lived Time-Dependent Remnants During Cosmological Symmetry Breaking: From Inflation to the Electroweak Scale","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"astro-ph.CO","authors_text":"Marcelo Gleiser, Nikitas Stamatopoulos, Noah Graham","submitted_at":"2010-04-26T21:11:59Z","abstract_excerpt":"Through a detailed numerical investigation in three spatial dimensions, we demonstrate that long-lived time-dependent field configurations emerge dynamically during symmetry breaking in an expanding de Sitter spacetime. We investigate two situations: a single scalar field with a double-well potential and the bosonic sector of an SU(2) non-Abelian Higgs model. For the single scalar, we show that large-amplitude oscillon configurations emerge spontaneously and persist to contribute about 1.2% of the energy density of the universe. We also show that for a range of parameters, oscillon lifetimes a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1004.4658","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":"1004.4658","created_at":"2026-05-18T04:41:36.632603+00:00"},{"alias_kind":"arxiv_version","alias_value":"1004.4658v2","created_at":"2026-05-18T04:41:36.632603+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1004.4658","created_at":"2026-05-18T04:41:36.632603+00:00"},{"alias_kind":"pith_short_12","alias_value":"OIWYQ7LE6KMR","created_at":"2026-05-18T12:26:12.377268+00:00"},{"alias_kind":"pith_short_16","alias_value":"OIWYQ7LE6KMRJXG2","created_at":"2026-05-18T12:26:12.377268+00:00"},{"alias_kind":"pith_short_8","alias_value":"OIWYQ7LE","created_at":"2026-05-18T12:26:12.377268+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/OIWYQ7LE6KMRJXG2I7CUWLHZSX","json":"https://pith.science/pith/OIWYQ7LE6KMRJXG2I7CUWLHZSX.json","graph_json":"https://pith.science/api/pith-number/OIWYQ7LE6KMRJXG2I7CUWLHZSX/graph.json","events_json":"https://pith.science/api/pith-number/OIWYQ7LE6KMRJXG2I7CUWLHZSX/events.json","paper":"https://pith.science/paper/OIWYQ7LE"},"agent_actions":{"view_html":"https://pith.science/pith/OIWYQ7LE6KMRJXG2I7CUWLHZSX","download_json":"https://pith.science/pith/OIWYQ7LE6KMRJXG2I7CUWLHZSX.json","view_paper":"https://pith.science/paper/OIWYQ7LE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1004.4658&json=true","fetch_graph":"https://pith.science/api/pith-number/OIWYQ7LE6KMRJXG2I7CUWLHZSX/graph.json","fetch_events":"https://pith.science/api/pith-number/OIWYQ7LE6KMRJXG2I7CUWLHZSX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OIWYQ7LE6KMRJXG2I7CUWLHZSX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OIWYQ7LE6KMRJXG2I7CUWLHZSX/action/storage_attestation","attest_author":"https://pith.science/pith/OIWYQ7LE6KMRJXG2I7CUWLHZSX/action/author_attestation","sign_citation":"https://pith.science/pith/OIWYQ7LE6KMRJXG2I7CUWLHZSX/action/citation_signature","submit_replication":"https://pith.science/pith/OIWYQ7LE6KMRJXG2I7CUWLHZSX/action/replication_record"}},"created_at":"2026-05-18T04:41:36.632603+00:00","updated_at":"2026-05-18T04:41:36.632603+00:00"}