{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:UKWUE3DJE6NEWYCP7RAPHKQJ77","short_pith_number":"pith:UKWUE3DJ","schema_version":"1.0","canonical_sha256":"a2ad426c69279a4b604ffc40f3aa09fffbb3ce36ec1c589bfccd8e17b440aba4","source":{"kind":"arxiv","id":"1511.02757","version":2},"attestation_state":"computed","paper":{"title":"From topological to non-topological solitons: kinks, domain walls and Q-balls in a scalar field model with non-trivial vacuum manifold","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"hep-th","authors_text":"Adolfo Cisterna, Betti Hartmann, Gabriel Luchini, Yves Brihaye","submitted_at":"2015-11-09T16:56:12Z","abstract_excerpt":"We consider a scalar field model with a self-interaction potential that possesses a discrete vacuum manifold. We point out that this model allows for both topological as well as non-topological solitons. In (1+1) dimensions both type of solutions have finite energy, while in (3+1) dimensions, the topological solitons have finite energy per unit area only and correspond to domain walls. Non-topological solitons with finite energy do exist in (3+1) dimensions due to a non-trivial phase of the scalar field and an associated U(1) symmetry of the model, though. We construct these so-called Q-ball s"},"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":"1511.02757","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2015-11-09T16:56:12Z","cross_cats_sorted":["gr-qc","hep-ph"],"title_canon_sha256":"5ac1823ba2b5c3bc62c8d96fd2e11d87841e3fba1d6b11fb9983023daf54fa30","abstract_canon_sha256":"57ebeb6670cb90f1d8f99083e63fe120c8ed5733d4fbf449a69a47e90874cd8f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:23:22.667501Z","signature_b64":"ISwwLDanDp//fFBbLlusVVkcOjR0l4zfJDnoDi90nJNitglZRliaEr1psJ/zOdBr9BFRbI2cRNXfp7jfva6eBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a2ad426c69279a4b604ffc40f3aa09fffbb3ce36ec1c589bfccd8e17b440aba4","last_reissued_at":"2026-05-18T01:23:22.666742Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:23:22.666742Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"From topological to non-topological solitons: kinks, domain walls and Q-balls in a scalar field model with non-trivial vacuum manifold","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"hep-th","authors_text":"Adolfo Cisterna, Betti Hartmann, Gabriel Luchini, Yves Brihaye","submitted_at":"2015-11-09T16:56:12Z","abstract_excerpt":"We consider a scalar field model with a self-interaction potential that possesses a discrete vacuum manifold. We point out that this model allows for both topological as well as non-topological solitons. In (1+1) dimensions both type of solutions have finite energy, while in (3+1) dimensions, the topological solitons have finite energy per unit area only and correspond to domain walls. Non-topological solitons with finite energy do exist in (3+1) dimensions due to a non-trivial phase of the scalar field and an associated U(1) symmetry of the model, though. We construct these so-called Q-ball s"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1511.02757","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":"1511.02757","created_at":"2026-05-18T01:23:22.666872+00:00"},{"alias_kind":"arxiv_version","alias_value":"1511.02757v2","created_at":"2026-05-18T01:23:22.666872+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1511.02757","created_at":"2026-05-18T01:23:22.666872+00:00"},{"alias_kind":"pith_short_12","alias_value":"UKWUE3DJE6NE","created_at":"2026-05-18T12:29:44.643036+00:00"},{"alias_kind":"pith_short_16","alias_value":"UKWUE3DJE6NEWYCP","created_at":"2026-05-18T12:29:44.643036+00:00"},{"alias_kind":"pith_short_8","alias_value":"UKWUE3DJ","created_at":"2026-05-18T12:29:44.643036+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2412.15158","citing_title":"Gravitational Waves From Dark Binaries With Finite-Range Dark Forces","ref_index":72,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/UKWUE3DJE6NEWYCP7RAPHKQJ77","json":"https://pith.science/pith/UKWUE3DJE6NEWYCP7RAPHKQJ77.json","graph_json":"https://pith.science/api/pith-number/UKWUE3DJE6NEWYCP7RAPHKQJ77/graph.json","events_json":"https://pith.science/api/pith-number/UKWUE3DJE6NEWYCP7RAPHKQJ77/events.json","paper":"https://pith.science/paper/UKWUE3DJ"},"agent_actions":{"view_html":"https://pith.science/pith/UKWUE3DJE6NEWYCP7RAPHKQJ77","download_json":"https://pith.science/pith/UKWUE3DJE6NEWYCP7RAPHKQJ77.json","view_paper":"https://pith.science/paper/UKWUE3DJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1511.02757&json=true","fetch_graph":"https://pith.science/api/pith-number/UKWUE3DJE6NEWYCP7RAPHKQJ77/graph.json","fetch_events":"https://pith.science/api/pith-number/UKWUE3DJE6NEWYCP7RAPHKQJ77/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UKWUE3DJE6NEWYCP7RAPHKQJ77/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UKWUE3DJE6NEWYCP7RAPHKQJ77/action/storage_attestation","attest_author":"https://pith.science/pith/UKWUE3DJE6NEWYCP7RAPHKQJ77/action/author_attestation","sign_citation":"https://pith.science/pith/UKWUE3DJE6NEWYCP7RAPHKQJ77/action/citation_signature","submit_replication":"https://pith.science/pith/UKWUE3DJE6NEWYCP7RAPHKQJ77/action/replication_record"}},"created_at":"2026-05-18T01:23:22.666872+00:00","updated_at":"2026-05-18T01:23:22.666872+00:00"}