{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2002:JM3KWGSYI2F6R3I7AOLJTXPIHX","short_pith_number":"pith:JM3KWGSY","schema_version":"1.0","canonical_sha256":"4b36ab1a58468be8ed1f039699dde83dc8f34cbfddda2da4618054193b0a7fcb","source":{"kind":"arxiv","id":"hep-ph/0210395","version":1},"attestation_state":"computed","paper":{"title":"New Constraints on the running-mass inflation model","license":"","headline":"","cross_cats":["astro-ph"],"primary_cat":"hep-ph","authors_text":"Alessandro Melchiorri, David H. Lyth, Laura Covi","submitted_at":"2002-10-29T17:14:54Z","abstract_excerpt":"We evaluate new observational constraints on the two-parameter scale-dependent spectral index predicted by the running-mass inflation model by combining the latest Cosmic Microwave Background (CMB) anisotropy measurements with the recent 2dFGRS data on the matter power spectrum, with Lyman $\\alpha $ forest data and finally with theoretical constraints on the reionization redshift. We find that present data still allow significant scale-dependence of $n$, which occurs in a physically reasonable regime of parameter space."},"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":"hep-ph/0210395","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"hep-ph","submitted_at":"2002-10-29T17:14:54Z","cross_cats_sorted":["astro-ph"],"title_canon_sha256":"9dade20c3b32b07f04095b04d4fe0d367b1e3873e07a53e6bd8538b8130f7289","abstract_canon_sha256":"439ce412a556dc011ed92bc08d4e06dfd88caeb295d0a569367ce35ec50e79ef"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:36:37.081928Z","signature_b64":"Gm55P6cGP8lcWdi/owoTyS+CNi9P6nCdNvPS+zVBAH5w2CJ0kbrgMYym5XSbdS9syHCxTKedU89+opIhJ8yzDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4b36ab1a58468be8ed1f039699dde83dc8f34cbfddda2da4618054193b0a7fcb","last_reissued_at":"2026-05-18T02:36:37.081391Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:36:37.081391Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"New Constraints on the running-mass inflation model","license":"","headline":"","cross_cats":["astro-ph"],"primary_cat":"hep-ph","authors_text":"Alessandro Melchiorri, David H. Lyth, Laura Covi","submitted_at":"2002-10-29T17:14:54Z","abstract_excerpt":"We evaluate new observational constraints on the two-parameter scale-dependent spectral index predicted by the running-mass inflation model by combining the latest Cosmic Microwave Background (CMB) anisotropy measurements with the recent 2dFGRS data on the matter power spectrum, with Lyman $\\alpha $ forest data and finally with theoretical constraints on the reionization redshift. We find that present data still allow significant scale-dependence of $n$, which occurs in a physically reasonable regime of parameter space."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-ph/0210395","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":"hep-ph/0210395","created_at":"2026-05-18T02:36:37.081496+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-ph/0210395v1","created_at":"2026-05-18T02:36:37.081496+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-ph/0210395","created_at":"2026-05-18T02:36:37.081496+00:00"},{"alias_kind":"pith_short_12","alias_value":"JM3KWGSYI2F6","created_at":"2026-05-18T12:25:50.845339+00:00"},{"alias_kind":"pith_short_16","alias_value":"JM3KWGSYI2F6R3I7","created_at":"2026-05-18T12:25:50.845339+00:00"},{"alias_kind":"pith_short_8","alias_value":"JM3KWGSY","created_at":"2026-05-18T12:25:50.845339+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/JM3KWGSYI2F6R3I7AOLJTXPIHX","json":"https://pith.science/pith/JM3KWGSYI2F6R3I7AOLJTXPIHX.json","graph_json":"https://pith.science/api/pith-number/JM3KWGSYI2F6R3I7AOLJTXPIHX/graph.json","events_json":"https://pith.science/api/pith-number/JM3KWGSYI2F6R3I7AOLJTXPIHX/events.json","paper":"https://pith.science/paper/JM3KWGSY"},"agent_actions":{"view_html":"https://pith.science/pith/JM3KWGSYI2F6R3I7AOLJTXPIHX","download_json":"https://pith.science/pith/JM3KWGSYI2F6R3I7AOLJTXPIHX.json","view_paper":"https://pith.science/paper/JM3KWGSY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-ph/0210395&json=true","fetch_graph":"https://pith.science/api/pith-number/JM3KWGSYI2F6R3I7AOLJTXPIHX/graph.json","fetch_events":"https://pith.science/api/pith-number/JM3KWGSYI2F6R3I7AOLJTXPIHX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JM3KWGSYI2F6R3I7AOLJTXPIHX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JM3KWGSYI2F6R3I7AOLJTXPIHX/action/storage_attestation","attest_author":"https://pith.science/pith/JM3KWGSYI2F6R3I7AOLJTXPIHX/action/author_attestation","sign_citation":"https://pith.science/pith/JM3KWGSYI2F6R3I7AOLJTXPIHX/action/citation_signature","submit_replication":"https://pith.science/pith/JM3KWGSYI2F6R3I7AOLJTXPIHX/action/replication_record"}},"created_at":"2026-05-18T02:36:37.081496+00:00","updated_at":"2026-05-18T02:36:37.081496+00:00"}