{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:KVHBKITAGYQ3T5U32VAHGTK7KX","short_pith_number":"pith:KVHBKITA","schema_version":"1.0","canonical_sha256":"554e1522603621b9f69bd540734d5f55e59ce8007612130fa2df141c946daa73","source":{"kind":"arxiv","id":"1406.0369","version":4},"attestation_state":"computed","paper":{"title":"Viability of the matter bounce scenario in Loop Quantum Cosmology for general potentials","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Jaume Amor\\'os, Jaume Haro","submitted_at":"2014-06-02T13:49:56Z","abstract_excerpt":"We consider the matter bounce scenario in Loop Quantum Cosmology (LQC) for physical potentials that at early times provide a nearly matter dominated Universe in the contracting phase, having a reheating mechanism in the expanding phase, i.e., being able to release the energy of the scalar field creating particles that thermalize in order to match with the hot Friedmann Universe, and finally at late times leading to the current cosmic acceleration. For these models, numerically solving the dynamical equations we have seen that the teleparallel version of LQC leads to theoretical results that fi"},"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":"1406.0369","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2014-06-02T13:49:56Z","cross_cats_sorted":[],"title_canon_sha256":"15379a19b2f3f71b6daa113884a47e476ea56c092d577450f83282fbf41b6759","abstract_canon_sha256":"cf72a074867f8b348f5a43f7af58daf80588bb525253930cd160fd587accd41d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:43:02.939380Z","signature_b64":"8FBT5U9OU5YG4VHTihiZ/zSG4PzZMJDCl0V8q8mGhcELcjEb0rNv9wnYTMZT5Cz6sC7J11S2CeOZy8aff/zsAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"554e1522603621b9f69bd540734d5f55e59ce8007612130fa2df141c946daa73","last_reissued_at":"2026-05-18T01:43:02.938891Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:43:02.938891Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Viability of the matter bounce scenario in Loop Quantum Cosmology for general potentials","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Jaume Amor\\'os, Jaume Haro","submitted_at":"2014-06-02T13:49:56Z","abstract_excerpt":"We consider the matter bounce scenario in Loop Quantum Cosmology (LQC) for physical potentials that at early times provide a nearly matter dominated Universe in the contracting phase, having a reheating mechanism in the expanding phase, i.e., being able to release the energy of the scalar field creating particles that thermalize in order to match with the hot Friedmann Universe, and finally at late times leading to the current cosmic acceleration. For these models, numerically solving the dynamical equations we have seen that the teleparallel version of LQC leads to theoretical results that fi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1406.0369","kind":"arxiv","version":4},"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":"1406.0369","created_at":"2026-05-18T01:43:02.938962+00:00"},{"alias_kind":"arxiv_version","alias_value":"1406.0369v4","created_at":"2026-05-18T01:43:02.938962+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1406.0369","created_at":"2026-05-18T01:43:02.938962+00:00"},{"alias_kind":"pith_short_12","alias_value":"KVHBKITAGYQ3","created_at":"2026-05-18T12:28:35.611951+00:00"},{"alias_kind":"pith_short_16","alias_value":"KVHBKITAGYQ3T5U3","created_at":"2026-05-18T12:28:35.611951+00:00"},{"alias_kind":"pith_short_8","alias_value":"KVHBKITA","created_at":"2026-05-18T12:28:35.611951+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"1705.11098","citing_title":"Modified Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution","ref_index":229,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/KVHBKITAGYQ3T5U32VAHGTK7KX","json":"https://pith.science/pith/KVHBKITAGYQ3T5U32VAHGTK7KX.json","graph_json":"https://pith.science/api/pith-number/KVHBKITAGYQ3T5U32VAHGTK7KX/graph.json","events_json":"https://pith.science/api/pith-number/KVHBKITAGYQ3T5U32VAHGTK7KX/events.json","paper":"https://pith.science/paper/KVHBKITA"},"agent_actions":{"view_html":"https://pith.science/pith/KVHBKITAGYQ3T5U32VAHGTK7KX","download_json":"https://pith.science/pith/KVHBKITAGYQ3T5U32VAHGTK7KX.json","view_paper":"https://pith.science/paper/KVHBKITA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1406.0369&json=true","fetch_graph":"https://pith.science/api/pith-number/KVHBKITAGYQ3T5U32VAHGTK7KX/graph.json","fetch_events":"https://pith.science/api/pith-number/KVHBKITAGYQ3T5U32VAHGTK7KX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KVHBKITAGYQ3T5U32VAHGTK7KX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KVHBKITAGYQ3T5U32VAHGTK7KX/action/storage_attestation","attest_author":"https://pith.science/pith/KVHBKITAGYQ3T5U32VAHGTK7KX/action/author_attestation","sign_citation":"https://pith.science/pith/KVHBKITAGYQ3T5U32VAHGTK7KX/action/citation_signature","submit_replication":"https://pith.science/pith/KVHBKITAGYQ3T5U32VAHGTK7KX/action/replication_record"}},"created_at":"2026-05-18T01:43:02.938962+00:00","updated_at":"2026-05-18T01:43:02.938962+00:00"}