{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:OX4ZH6BEZK7JYT3D27FLLVN5SP","short_pith_number":"pith:OX4ZH6BE","schema_version":"1.0","canonical_sha256":"75f993f824cabe9c4f63d7cab5d5bd93c7099be0de2007742d338da07cb95467","source":{"kind":"arxiv","id":"1809.01198","version":2},"attestation_state":"computed","paper":{"title":"Strong gravitational radiation from a simple dark matter model","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Camilo Garcia-Cely, Iason Baldes","submitted_at":"2018-09-04T18:57:44Z","abstract_excerpt":"A rather minimal possibility is that dark matter consists of the gauge bosons of a spontaneously broken symmetry. Here we explore the possibility of detecting the gravitational waves produced by the phase transition associated with such breaking. Concretely, we focus on the scenario based on an $SU(2)_D$ group and argue that it is a case study for the sensitivity of future gravitational wave observatories to phase transitions associated with dark matter. This is because there are few parameters and those fixing the relic density also determine the effective potential establishing the strength "},"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":"1809.01198","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2018-09-04T18:57:44Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"5606ec757bf5c332b84c69190b36a77478e42b181778758012b87ba35e11c286","abstract_canon_sha256":"55871524f1b82d111a97c66ece25a928abe3fad5cf6b8ef3b7e412a99c0e8f98"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:44:48.123746Z","signature_b64":"vxzf2gzvzD76hiwPZGJiLKEsEvL0dGn06YGOJwVQr0kxmuOxYs8kneZXj0KVEJzgNTzl1lWY4MJ1UgQpg8SjCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"75f993f824cabe9c4f63d7cab5d5bd93c7099be0de2007742d338da07cb95467","last_reissued_at":"2026-05-17T23:44:48.123147Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:44:48.123147Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Strong gravitational radiation from a simple dark matter model","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Camilo Garcia-Cely, Iason Baldes","submitted_at":"2018-09-04T18:57:44Z","abstract_excerpt":"A rather minimal possibility is that dark matter consists of the gauge bosons of a spontaneously broken symmetry. Here we explore the possibility of detecting the gravitational waves produced by the phase transition associated with such breaking. Concretely, we focus on the scenario based on an $SU(2)_D$ group and argue that it is a case study for the sensitivity of future gravitational wave observatories to phase transitions associated with dark matter. This is because there are few parameters and those fixing the relic density also determine the effective potential establishing the strength "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1809.01198","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":"1809.01198","created_at":"2026-05-17T23:44:48.123228+00:00"},{"alias_kind":"arxiv_version","alias_value":"1809.01198v2","created_at":"2026-05-17T23:44:48.123228+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1809.01198","created_at":"2026-05-17T23:44:48.123228+00:00"},{"alias_kind":"pith_short_12","alias_value":"OX4ZH6BEZK7J","created_at":"2026-05-18T12:32:43.782077+00:00"},{"alias_kind":"pith_short_16","alias_value":"OX4ZH6BEZK7JYT3D","created_at":"2026-05-18T12:32:43.782077+00:00"},{"alias_kind":"pith_short_8","alias_value":"OX4ZH6BE","created_at":"2026-05-18T12:32:43.782077+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":5,"internal_anchor_count":4,"sample":[{"citing_arxiv_id":"1910.13125","citing_title":"Detecting gravitational waves from cosmological phase transitions with LISA: an update","ref_index":195,"is_internal_anchor":true},{"citing_arxiv_id":"2002.04615","citing_title":"New Sensitivity Curves for Gravitational-Wave Signals from Cosmological Phase Transitions","ref_index":33,"is_internal_anchor":true},{"citing_arxiv_id":"2408.03649","citing_title":"Probing radiative electroweak symmetry breaking with colliders and gravitational waves","ref_index":31,"is_internal_anchor":true},{"citing_arxiv_id":"2603.09126","citing_title":"Dark matter in classically conformal theories: WIMP and supercooling","ref_index":20,"is_internal_anchor":true},{"citing_arxiv_id":"2605.02955","citing_title":"Spontaneous Symmetry Breaking and the Emergent Einstein-Standard Model: From Weyl x SU (2)L x U (1)Y Gauge Theory to Geometric Mass Generation","ref_index":23,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/OX4ZH6BEZK7JYT3D27FLLVN5SP","json":"https://pith.science/pith/OX4ZH6BEZK7JYT3D27FLLVN5SP.json","graph_json":"https://pith.science/api/pith-number/OX4ZH6BEZK7JYT3D27FLLVN5SP/graph.json","events_json":"https://pith.science/api/pith-number/OX4ZH6BEZK7JYT3D27FLLVN5SP/events.json","paper":"https://pith.science/paper/OX4ZH6BE"},"agent_actions":{"view_html":"https://pith.science/pith/OX4ZH6BEZK7JYT3D27FLLVN5SP","download_json":"https://pith.science/pith/OX4ZH6BEZK7JYT3D27FLLVN5SP.json","view_paper":"https://pith.science/paper/OX4ZH6BE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1809.01198&json=true","fetch_graph":"https://pith.science/api/pith-number/OX4ZH6BEZK7JYT3D27FLLVN5SP/graph.json","fetch_events":"https://pith.science/api/pith-number/OX4ZH6BEZK7JYT3D27FLLVN5SP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OX4ZH6BEZK7JYT3D27FLLVN5SP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OX4ZH6BEZK7JYT3D27FLLVN5SP/action/storage_attestation","attest_author":"https://pith.science/pith/OX4ZH6BEZK7JYT3D27FLLVN5SP/action/author_attestation","sign_citation":"https://pith.science/pith/OX4ZH6BEZK7JYT3D27FLLVN5SP/action/citation_signature","submit_replication":"https://pith.science/pith/OX4ZH6BEZK7JYT3D27FLLVN5SP/action/replication_record"}},"created_at":"2026-05-17T23:44:48.123228+00:00","updated_at":"2026-05-17T23:44:48.123228+00:00"}