{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:BTR3A6JCTHEAFVJ32FDA7DE6KX","short_pith_number":"pith:BTR3A6JC","schema_version":"1.0","canonical_sha256":"0ce3b0792299c802d53bd1460f8c9e55c6257f174414e07a307ab87c97668c47","source":{"kind":"arxiv","id":"2303.16072","version":1},"attestation_state":"computed","paper":{"title":"Oscillon spectroscopy","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"hep-th","authors_text":"Evangelos Sfakianakis, Fabio van Dissel, Oriol Pujolas","submitted_at":"2023-03-28T15:48:43Z","abstract_excerpt":"The sine-Gordon model in 3+1 dimensions is known to admit two oscillons of different energy and frequency but comparable lifetime. We show that the oscillon spectrum includes more spherically symmetric ``states''. We identify new high-amplitude oscillons by allowing the field profile to have a number of nodes. For each number of nodes, we find 2 states with a comparable lifetime to the nodeless ones. Oscillons with nodes are, however, unstable to non-spherical perturbations and so their lifetime is significantly reduced. Interestingly, these states are seen to fragment into a collection of nod"},"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":"2303.16072","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-th","submitted_at":"2023-03-28T15:48:43Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"667f9bc529e7bc4b44d56c9a48967c38aaff04ba64f5ad5d2ab14f383acf71d9","abstract_canon_sha256":"f3f8d86cab959bafbd09b19faf4769564a35475211495cd129e110c6702161f1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:38:51.852630Z","signature_b64":"tDpmdSeZVP3XHk/PE5FBny+24mEA52sScGK0VN4OiCt2zVdPmpnkXjn6fDj+LVQmfQZaEQfX6jZn1Po67scrAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0ce3b0792299c802d53bd1460f8c9e55c6257f174414e07a307ab87c97668c47","last_reissued_at":"2026-07-05T06:38:51.852016Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:38:51.852016Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Oscillon spectroscopy","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"hep-th","authors_text":"Evangelos Sfakianakis, Fabio van Dissel, Oriol Pujolas","submitted_at":"2023-03-28T15:48:43Z","abstract_excerpt":"The sine-Gordon model in 3+1 dimensions is known to admit two oscillons of different energy and frequency but comparable lifetime. We show that the oscillon spectrum includes more spherically symmetric ``states''. We identify new high-amplitude oscillons by allowing the field profile to have a number of nodes. For each number of nodes, we find 2 states with a comparable lifetime to the nodeless ones. Oscillons with nodes are, however, unstable to non-spherical perturbations and so their lifetime is significantly reduced. Interestingly, these states are seen to fragment into a collection of nod"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2303.16072","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2303.16072/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":"2303.16072","created_at":"2026-07-05T06:38:51.852079+00:00"},{"alias_kind":"arxiv_version","alias_value":"2303.16072v1","created_at":"2026-07-05T06:38:51.852079+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2303.16072","created_at":"2026-07-05T06:38:51.852079+00:00"},{"alias_kind":"pith_short_12","alias_value":"BTR3A6JCTHEA","created_at":"2026-07-05T06:38:51.852079+00:00"},{"alias_kind":"pith_short_16","alias_value":"BTR3A6JCTHEAFVJ3","created_at":"2026-07-05T06:38:51.852079+00:00"},{"alias_kind":"pith_short_8","alias_value":"BTR3A6JC","created_at":"2026-07-05T06:38:51.852079+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2607.01177","citing_title":"Preheating and oscillon formation in Einstein-scalar-Gauss-Bonnet gravity","ref_index":43,"is_internal_anchor":false},{"citing_arxiv_id":"2602.07972","citing_title":"Self-resonance preheating in deformed attractor models: oscillon formation and evolution","ref_index":70,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/BTR3A6JCTHEAFVJ32FDA7DE6KX","json":"https://pith.science/pith/BTR3A6JCTHEAFVJ32FDA7DE6KX.json","graph_json":"https://pith.science/api/pith-number/BTR3A6JCTHEAFVJ32FDA7DE6KX/graph.json","events_json":"https://pith.science/api/pith-number/BTR3A6JCTHEAFVJ32FDA7DE6KX/events.json","paper":"https://pith.science/paper/BTR3A6JC"},"agent_actions":{"view_html":"https://pith.science/pith/BTR3A6JCTHEAFVJ32FDA7DE6KX","download_json":"https://pith.science/pith/BTR3A6JCTHEAFVJ32FDA7DE6KX.json","view_paper":"https://pith.science/paper/BTR3A6JC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2303.16072&json=true","fetch_graph":"https://pith.science/api/pith-number/BTR3A6JCTHEAFVJ32FDA7DE6KX/graph.json","fetch_events":"https://pith.science/api/pith-number/BTR3A6JCTHEAFVJ32FDA7DE6KX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BTR3A6JCTHEAFVJ32FDA7DE6KX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BTR3A6JCTHEAFVJ32FDA7DE6KX/action/storage_attestation","attest_author":"https://pith.science/pith/BTR3A6JCTHEAFVJ32FDA7DE6KX/action/author_attestation","sign_citation":"https://pith.science/pith/BTR3A6JCTHEAFVJ32FDA7DE6KX/action/citation_signature","submit_replication":"https://pith.science/pith/BTR3A6JCTHEAFVJ32FDA7DE6KX/action/replication_record"}},"created_at":"2026-07-05T06:38:51.852079+00:00","updated_at":"2026-07-05T06:38:51.852079+00:00"}