{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:CCAJEJWMZXKFXR5KB3VHGOTGJ2","short_pith_number":"pith:CCAJEJWM","schema_version":"1.0","canonical_sha256":"10809226cccdd45bc7aa0eea733a664e99affc3ad101b0fe2153a45201f2e2de","source":{"kind":"arxiv","id":"2603.04182","version":2},"attestation_state":"computed","paper":{"title":"Non-minimally coupled loop quantum inflation with inverse-volume corrections","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-th"],"primary_cat":"gr-qc","authors_text":"Giovanni Otalora, Joel Saavedra, Rudranil Roy, Salvatore Capozziello","submitted_at":"2026-03-04T15:36:52Z","abstract_excerpt":"We study slow-roll inflation driven by a scalar field non-minimally coupled to gravity within the effective framework of Loop Quantum Cosmology (LQC), including inverse-volume corrections. We consider two physically motivated classes of potentials, a Higgs-like quartic potential $V\\propto\\phi^{4}$ and string-inspired fractional monomial potentials $V\\propto\\phi^{p}$ with $p<1$. Working at first order in the slow-roll expansion, we derive analytic expressions for the inflationary observables, namely the scalar spectral index $n_s$, the tensor-to-scalar ratio $r$, and the running $\\alpha_s\\equiv"},"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":"2603.04182","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2026-03-04T15:36:52Z","cross_cats_sorted":["astro-ph.CO","hep-th"],"title_canon_sha256":"96985b06893d914c3b61fba3c837bfa4a5aec8bc81f0f353814becbee0953281","abstract_canon_sha256":"e44a79b7a4e5f4392da492bffb1670d0e79da7cff8651f83522c55f19f58c99d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-06-02T01:03:44.592995Z","signature_b64":"GvdFOQ311zc9O4pF4yVdK9pbzYLNU4DL9TASxJuBLLKER26bQpFXGJie6wQ5Vi8mOt5sEBgPTb2vcaaU6zg1Aw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"10809226cccdd45bc7aa0eea733a664e99affc3ad101b0fe2153a45201f2e2de","last_reissued_at":"2026-06-02T01:03:44.592392Z","signature_status":"signed_v1","first_computed_at":"2026-06-02T01:03:44.592392Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Non-minimally coupled loop quantum inflation with inverse-volume corrections","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-th"],"primary_cat":"gr-qc","authors_text":"Giovanni Otalora, Joel Saavedra, Rudranil Roy, Salvatore Capozziello","submitted_at":"2026-03-04T15:36:52Z","abstract_excerpt":"We study slow-roll inflation driven by a scalar field non-minimally coupled to gravity within the effective framework of Loop Quantum Cosmology (LQC), including inverse-volume corrections. We consider two physically motivated classes of potentials, a Higgs-like quartic potential $V\\propto\\phi^{4}$ and string-inspired fractional monomial potentials $V\\propto\\phi^{p}$ with $p<1$. Working at first order in the slow-roll expansion, we derive analytic expressions for the inflationary observables, namely the scalar spectral index $n_s$, the tensor-to-scalar ratio $r$, and the running $\\alpha_s\\equiv"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2603.04182","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2603.04182/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2603.04182","created_at":"2026-06-02T01:03:44.592471+00:00"},{"alias_kind":"arxiv_version","alias_value":"2603.04182v2","created_at":"2026-06-02T01:03:44.592471+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2603.04182","created_at":"2026-06-02T01:03:44.592471+00:00"},{"alias_kind":"pith_short_12","alias_value":"CCAJEJWMZXKF","created_at":"2026-06-02T01:03:44.592471+00:00"},{"alias_kind":"pith_short_16","alias_value":"CCAJEJWMZXKFXR5K","created_at":"2026-06-02T01:03:44.592471+00:00"},{"alias_kind":"pith_short_8","alias_value":"CCAJEJWM","created_at":"2026-06-02T01:03:44.592471+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2604.24011","citing_title":"Primordial black hole production in scalar field inflation within $f(T)$ gravity","ref_index":9,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CCAJEJWMZXKFXR5KB3VHGOTGJ2","json":"https://pith.science/pith/CCAJEJWMZXKFXR5KB3VHGOTGJ2.json","graph_json":"https://pith.science/api/pith-number/CCAJEJWMZXKFXR5KB3VHGOTGJ2/graph.json","events_json":"https://pith.science/api/pith-number/CCAJEJWMZXKFXR5KB3VHGOTGJ2/events.json","paper":"https://pith.science/paper/CCAJEJWM"},"agent_actions":{"view_html":"https://pith.science/pith/CCAJEJWMZXKFXR5KB3VHGOTGJ2","download_json":"https://pith.science/pith/CCAJEJWMZXKFXR5KB3VHGOTGJ2.json","view_paper":"https://pith.science/paper/CCAJEJWM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2603.04182&json=true","fetch_graph":"https://pith.science/api/pith-number/CCAJEJWMZXKFXR5KB3VHGOTGJ2/graph.json","fetch_events":"https://pith.science/api/pith-number/CCAJEJWMZXKFXR5KB3VHGOTGJ2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CCAJEJWMZXKFXR5KB3VHGOTGJ2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CCAJEJWMZXKFXR5KB3VHGOTGJ2/action/storage_attestation","attest_author":"https://pith.science/pith/CCAJEJWMZXKFXR5KB3VHGOTGJ2/action/author_attestation","sign_citation":"https://pith.science/pith/CCAJEJWMZXKFXR5KB3VHGOTGJ2/action/citation_signature","submit_replication":"https://pith.science/pith/CCAJEJWMZXKFXR5KB3VHGOTGJ2/action/replication_record"}},"created_at":"2026-06-02T01:03:44.592471+00:00","updated_at":"2026-06-02T01:03:44.592471+00:00"}