{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:7K6BQZOVMBFZM2PMA5KP3SDNAZ","short_pith_number":"pith:7K6BQZOV","schema_version":"1.0","canonical_sha256":"fabc1865d5604b9669ec0754fdc86d067cd423cbf69e45452e03c8c90c2b8124","source":{"kind":"arxiv","id":"1510.03264","version":2},"attestation_state":"computed","paper":{"title":"Cosmology with nonminimal kinetic coupling and a Higgs-like potential","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-th"],"primary_cat":"gr-qc","authors_text":"Jiro Matsumoto, Sergey V. Sushkov","submitted_at":"2015-10-12T12:59:39Z","abstract_excerpt":"We consider cosmological dynamics in the theory of gravity with the scalar field possessing the nonminimal kinetic coupling to curvature given as $\\kappa G^{\\mu\\nu}\\phi_{,\\mu}\\phi_{,\\nu}$, and the Higgs-like potential $V(\\phi)=\\frac{\\lambda}{4}(\\phi^2-\\phi_0^2)^2$. Using the dynamical system method, we analyze stationary points, their stability, and all possible asymptotical regimes of the model under consideration. We show that the Higgs field with the kinetic coupling provides an existence of accelerated regimes of the Universe evolution. There are three possible cosmological scenarios with "},"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":"1510.03264","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2015-10-12T12:59:39Z","cross_cats_sorted":["astro-ph.CO","hep-th"],"title_canon_sha256":"d8aa66c76a210efa5a829f1cfa88f91b8c85cba542d62d61963ca2680772e13c","abstract_canon_sha256":"abf320c8ce2939455168bcda909b172330f6aa811ac33fbb143543c2850ac5d0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:35:09.587066Z","signature_b64":"ej1UvIvQapi5ZwKvriC7+pzBE3iKK7rXo29jWvVi7BlKb8CjHVMPC/n5F9HGAkcmBFS3FSXx4M8izVb9o6JkDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fabc1865d5604b9669ec0754fdc86d067cd423cbf69e45452e03c8c90c2b8124","last_reissued_at":"2026-05-18T00:35:09.586678Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:35:09.586678Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cosmology with nonminimal kinetic coupling and a Higgs-like potential","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-th"],"primary_cat":"gr-qc","authors_text":"Jiro Matsumoto, Sergey V. Sushkov","submitted_at":"2015-10-12T12:59:39Z","abstract_excerpt":"We consider cosmological dynamics in the theory of gravity with the scalar field possessing the nonminimal kinetic coupling to curvature given as $\\kappa G^{\\mu\\nu}\\phi_{,\\mu}\\phi_{,\\nu}$, and the Higgs-like potential $V(\\phi)=\\frac{\\lambda}{4}(\\phi^2-\\phi_0^2)^2$. Using the dynamical system method, we analyze stationary points, their stability, and all possible asymptotical regimes of the model under consideration. We show that the Higgs field with the kinetic coupling provides an existence of accelerated regimes of the Universe evolution. There are three possible cosmological scenarios with "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1510.03264","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":"1510.03264","created_at":"2026-05-18T00:35:09.586741+00:00"},{"alias_kind":"arxiv_version","alias_value":"1510.03264v2","created_at":"2026-05-18T00:35:09.586741+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1510.03264","created_at":"2026-05-18T00:35:09.586741+00:00"},{"alias_kind":"pith_short_12","alias_value":"7K6BQZOVMBFZ","created_at":"2026-05-18T12:29:10.953037+00:00"},{"alias_kind":"pith_short_16","alias_value":"7K6BQZOVMBFZM2PM","created_at":"2026-05-18T12:29:10.953037+00:00"},{"alias_kind":"pith_short_8","alias_value":"7K6BQZOV","created_at":"2026-05-18T12:29:10.953037+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.11987","citing_title":"Asymptotic Theorems and Averaging in Scalar Field Cosmology","ref_index":36,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/7K6BQZOVMBFZM2PMA5KP3SDNAZ","json":"https://pith.science/pith/7K6BQZOVMBFZM2PMA5KP3SDNAZ.json","graph_json":"https://pith.science/api/pith-number/7K6BQZOVMBFZM2PMA5KP3SDNAZ/graph.json","events_json":"https://pith.science/api/pith-number/7K6BQZOVMBFZM2PMA5KP3SDNAZ/events.json","paper":"https://pith.science/paper/7K6BQZOV"},"agent_actions":{"view_html":"https://pith.science/pith/7K6BQZOVMBFZM2PMA5KP3SDNAZ","download_json":"https://pith.science/pith/7K6BQZOVMBFZM2PMA5KP3SDNAZ.json","view_paper":"https://pith.science/paper/7K6BQZOV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1510.03264&json=true","fetch_graph":"https://pith.science/api/pith-number/7K6BQZOVMBFZM2PMA5KP3SDNAZ/graph.json","fetch_events":"https://pith.science/api/pith-number/7K6BQZOVMBFZM2PMA5KP3SDNAZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7K6BQZOVMBFZM2PMA5KP3SDNAZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7K6BQZOVMBFZM2PMA5KP3SDNAZ/action/storage_attestation","attest_author":"https://pith.science/pith/7K6BQZOVMBFZM2PMA5KP3SDNAZ/action/author_attestation","sign_citation":"https://pith.science/pith/7K6BQZOVMBFZM2PMA5KP3SDNAZ/action/citation_signature","submit_replication":"https://pith.science/pith/7K6BQZOVMBFZM2PMA5KP3SDNAZ/action/replication_record"}},"created_at":"2026-05-18T00:35:09.586741+00:00","updated_at":"2026-05-18T00:35:09.586741+00:00"}