{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:FYHFRVXR3TBNJ4ZVJGPE3Z2TOZ","short_pith_number":"pith:FYHFRVXR","schema_version":"1.0","canonical_sha256":"2e0e58d6f1dcc2d4f335499e4de753764affdc2100f6099649c30ff803af07c3","source":{"kind":"arxiv","id":"1406.0128","version":1},"attestation_state":"computed","paper":{"title":"Full Investigation on the Dynamics of Power-Law Kinetic Quintessence","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-th"],"primary_cat":"gr-qc","authors_text":"Chenggang Shu, Hong Tu, Jiasheng Huang, Wei Fang, Ying Li","submitted_at":"2014-06-01T04:14:26Z","abstract_excerpt":"We give a full investigation on the dynamics of power-law kinetic quintessence $L(X, \\phi)=V(\\phi)(-X+X^2)$ by considering the potential related parameter $\\Gamma$($=\\frac{V V''}{V'^2}$) as a function of another potential parameter $\\lambda$($=\\frac{V'}{\\kappa V^{3/2}}$), which correspondingly extends the analysis of the dynamical system of our universe from two-dimension to three-dimension. Beside the critical points found in previous papers, we find a new de-Sitter-like dominant attractor(\\textit{cp$6$}) and give its stable condition using the center manifold theorem. For the dark energy dom"},"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":"1406.0128","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2014-06-01T04:14:26Z","cross_cats_sorted":["astro-ph.CO","hep-th"],"title_canon_sha256":"c114f9be45c368f5c1e67250a4e0e372a75afe25ad4cf51fad6a1a9532f6e895","abstract_canon_sha256":"670310590405b4484a2b799ca4d1f95a78b7657dba5def95d908034e34fc4165"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:43:04.338789Z","signature_b64":"C9KlQcMZ4k7ku11vgVI3lfX6Xzrl5WTlSGT6Gk6Y++AitaAZYB6/ehoyiHtc+VLGix1X/Vgi5KeRoVCuEqvwAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2e0e58d6f1dcc2d4f335499e4de753764affdc2100f6099649c30ff803af07c3","last_reissued_at":"2026-05-18T01:43:04.338424Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:43:04.338424Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Full Investigation on the Dynamics of Power-Law Kinetic Quintessence","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-th"],"primary_cat":"gr-qc","authors_text":"Chenggang Shu, Hong Tu, Jiasheng Huang, Wei Fang, Ying Li","submitted_at":"2014-06-01T04:14:26Z","abstract_excerpt":"We give a full investigation on the dynamics of power-law kinetic quintessence $L(X, \\phi)=V(\\phi)(-X+X^2)$ by considering the potential related parameter $\\Gamma$($=\\frac{V V''}{V'^2}$) as a function of another potential parameter $\\lambda$($=\\frac{V'}{\\kappa V^{3/2}}$), which correspondingly extends the analysis of the dynamical system of our universe from two-dimension to three-dimension. Beside the critical points found in previous papers, we find a new de-Sitter-like dominant attractor(\\textit{cp$6$}) and give its stable condition using the center manifold theorem. For the dark energy dom"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1406.0128","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":"1406.0128","created_at":"2026-05-18T01:43:04.338483+00:00"},{"alias_kind":"arxiv_version","alias_value":"1406.0128v1","created_at":"2026-05-18T01:43:04.338483+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1406.0128","created_at":"2026-05-18T01:43:04.338483+00:00"},{"alias_kind":"pith_short_12","alias_value":"FYHFRVXR3TBN","created_at":"2026-05-18T12:28:28.263976+00:00"},{"alias_kind":"pith_short_16","alias_value":"FYHFRVXR3TBNJ4ZV","created_at":"2026-05-18T12:28:28.263976+00:00"},{"alias_kind":"pith_short_8","alias_value":"FYHFRVXR","created_at":"2026-05-18T12:28:28.263976+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2509.09202","citing_title":"Interacting $k$-essence field with non-pressureless Dark Matter: Cosmological Dynamics and Observational Constraints","ref_index":66,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FYHFRVXR3TBNJ4ZVJGPE3Z2TOZ","json":"https://pith.science/pith/FYHFRVXR3TBNJ4ZVJGPE3Z2TOZ.json","graph_json":"https://pith.science/api/pith-number/FYHFRVXR3TBNJ4ZVJGPE3Z2TOZ/graph.json","events_json":"https://pith.science/api/pith-number/FYHFRVXR3TBNJ4ZVJGPE3Z2TOZ/events.json","paper":"https://pith.science/paper/FYHFRVXR"},"agent_actions":{"view_html":"https://pith.science/pith/FYHFRVXR3TBNJ4ZVJGPE3Z2TOZ","download_json":"https://pith.science/pith/FYHFRVXR3TBNJ4ZVJGPE3Z2TOZ.json","view_paper":"https://pith.science/paper/FYHFRVXR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1406.0128&json=true","fetch_graph":"https://pith.science/api/pith-number/FYHFRVXR3TBNJ4ZVJGPE3Z2TOZ/graph.json","fetch_events":"https://pith.science/api/pith-number/FYHFRVXR3TBNJ4ZVJGPE3Z2TOZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FYHFRVXR3TBNJ4ZVJGPE3Z2TOZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FYHFRVXR3TBNJ4ZVJGPE3Z2TOZ/action/storage_attestation","attest_author":"https://pith.science/pith/FYHFRVXR3TBNJ4ZVJGPE3Z2TOZ/action/author_attestation","sign_citation":"https://pith.science/pith/FYHFRVXR3TBNJ4ZVJGPE3Z2TOZ/action/citation_signature","submit_replication":"https://pith.science/pith/FYHFRVXR3TBNJ4ZVJGPE3Z2TOZ/action/replication_record"}},"created_at":"2026-05-18T01:43:04.338483+00:00","updated_at":"2026-05-18T01:43:04.338483+00:00"}