{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2008:WLCEG6XDSXZFZE72LJWB5CO26H","short_pith_number":"pith:WLCEG6XD","schema_version":"1.0","canonical_sha256":"b2c4437ae395f25c93fa5a6c1e89daf1d44a2b71af46fa3d9581c968992db5a1","source":{"kind":"arxiv","id":"0812.1919","version":1},"attestation_state":"computed","paper":{"title":"Computation of the radiation amplitude of oscillons","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Gyula Fodor, M\\'ark Mezei, P\\'eter Forg\\'acs, Zal\\'an Horv\\'ath","submitted_at":"2008-12-10T14:04:52Z","abstract_excerpt":"The radiation loss of small amplitude oscillons (very long-living, spatially localized, time dependent solutions) in one dimensional scalar field theories is computed in the small-amplitude expansion analytically using matched asymptotic series expansions and Borel summation. The amplitude of the radiation is beyond all orders in perturbation theory and the method used has been developed by Segur and Kruskal in Phys. Rev. Lett. 58, 747 (1987). Our results are in good agreement with those of long time numerical simulations of oscillons."},"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":"0812.1919","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2008-12-10T14:04:52Z","cross_cats_sorted":[],"title_canon_sha256":"1616b51d63bc73e672713c50eb90e9744b4ee890b187cc4500f8800ecad45b60","abstract_canon_sha256":"5fdd232905ae806fbd7dd9627359d0803132ef86cc27fce37045c4798155df4e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:20:59.435906Z","signature_b64":"Jh1lF3IrEgiLFrvz30keWkuoGiVc2bl9u/sSka9CdCMlJa/eKVdvbkzSMuq4l9MOxaKMQWlViD8LCR/plv1eBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b2c4437ae395f25c93fa5a6c1e89daf1d44a2b71af46fa3d9581c968992db5a1","last_reissued_at":"2026-05-18T04:20:59.435278Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:20:59.435278Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Computation of the radiation amplitude of oscillons","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Gyula Fodor, M\\'ark Mezei, P\\'eter Forg\\'acs, Zal\\'an Horv\\'ath","submitted_at":"2008-12-10T14:04:52Z","abstract_excerpt":"The radiation loss of small amplitude oscillons (very long-living, spatially localized, time dependent solutions) in one dimensional scalar field theories is computed in the small-amplitude expansion analytically using matched asymptotic series expansions and Borel summation. The amplitude of the radiation is beyond all orders in perturbation theory and the method used has been developed by Segur and Kruskal in Phys. Rev. Lett. 58, 747 (1987). Our results are in good agreement with those of long time numerical simulations of oscillons."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0812.1919","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":""},"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":"0812.1919","created_at":"2026-05-18T04:20:59.435365+00:00"},{"alias_kind":"arxiv_version","alias_value":"0812.1919v1","created_at":"2026-05-18T04:20:59.435365+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0812.1919","created_at":"2026-05-18T04:20:59.435365+00:00"},{"alias_kind":"pith_short_12","alias_value":"WLCEG6XDSXZF","created_at":"2026-05-18T12:25:58.018023+00:00"},{"alias_kind":"pith_short_16","alias_value":"WLCEG6XDSXZFZE72","created_at":"2026-05-18T12:25:58.018023+00:00"},{"alias_kind":"pith_short_8","alias_value":"WLCEG6XD","created_at":"2026-05-18T12:25:58.018023+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"1202.5809","citing_title":"Dynamical Boson Stars","ref_index":190,"is_internal_anchor":true},{"citing_arxiv_id":"2602.07972","citing_title":"Self-resonance preheating in deformed attractor models: oscillon formation and evolution","ref_index":76,"is_internal_anchor":true},{"citing_arxiv_id":"2604.04494","citing_title":"Multi-field oscillons/I-balls in the Friedberg-Lee-Sirlin model","ref_index":26,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/WLCEG6XDSXZFZE72LJWB5CO26H","json":"https://pith.science/pith/WLCEG6XDSXZFZE72LJWB5CO26H.json","graph_json":"https://pith.science/api/pith-number/WLCEG6XDSXZFZE72LJWB5CO26H/graph.json","events_json":"https://pith.science/api/pith-number/WLCEG6XDSXZFZE72LJWB5CO26H/events.json","paper":"https://pith.science/paper/WLCEG6XD"},"agent_actions":{"view_html":"https://pith.science/pith/WLCEG6XDSXZFZE72LJWB5CO26H","download_json":"https://pith.science/pith/WLCEG6XDSXZFZE72LJWB5CO26H.json","view_paper":"https://pith.science/paper/WLCEG6XD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0812.1919&json=true","fetch_graph":"https://pith.science/api/pith-number/WLCEG6XDSXZFZE72LJWB5CO26H/graph.json","fetch_events":"https://pith.science/api/pith-number/WLCEG6XDSXZFZE72LJWB5CO26H/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/WLCEG6XDSXZFZE72LJWB5CO26H/action/timestamp_anchor","attest_storage":"https://pith.science/pith/WLCEG6XDSXZFZE72LJWB5CO26H/action/storage_attestation","attest_author":"https://pith.science/pith/WLCEG6XDSXZFZE72LJWB5CO26H/action/author_attestation","sign_citation":"https://pith.science/pith/WLCEG6XDSXZFZE72LJWB5CO26H/action/citation_signature","submit_replication":"https://pith.science/pith/WLCEG6XDSXZFZE72LJWB5CO26H/action/replication_record"}},"created_at":"2026-05-18T04:20:59.435365+00:00","updated_at":"2026-05-18T04:20:59.435365+00:00"}