{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:RMBW2IACBNLUT56JBT6SU7GW2S","short_pith_number":"pith:RMBW2IAC","schema_version":"1.0","canonical_sha256":"8b036d20020b5749f7c90cfd2a7cd6d4b7bcd5af2edc5d8f2c7d1845d4af7943","source":{"kind":"arxiv","id":"2505.03004","version":1},"attestation_state":"computed","paper":{"title":"Higgs-like inflation under ACTivated mass","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc"],"primary_cat":"hep-ph","authors_text":"Wen Yin","submitted_at":"2025-05-05T20:03:27Z","abstract_excerpt":"Recent analyses that combine the latest data from the Atacama Cosmology Telescope (ACT) with cosmic microwave background observations by BICEP/Keck and Planck, together with the DESI baryon acoustic-baryonic-oscillation (BAO) measurements, have tightened the limits on inflationary scenarios. The joint data set yields a spectral index of primordial scalar perturbations $n_s = 0.9743 \\pm 0.0034$ and an upper bound on the tensor-to-scalar ratio of $r < 0.038$. This slight upward shift in $n_s$ puts the previously favored Starobinsky model, and the conventional metric Higgs(-like) inflation--based"},"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":"2505.03004","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2025-05-05T20:03:27Z","cross_cats_sorted":["astro-ph.CO","gr-qc"],"title_canon_sha256":"3045085857afb4a41dc239daf10199ff8001b9c004a2e73cac664f3ce5576d18","abstract_canon_sha256":"b7545ee7d546b07b7bd77aa4bfae497ac4a3ffcf7c42b8ed0973251311e82441"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:58:50.853926Z","signature_b64":"0Ez5/28UXLBe3PHuIDPZp4UfK51yduc8dLCJW0hhTkxkt3uuI3PZZYF7KazAYKYkHTl+gxaUkVwWtFpJe+QbBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8b036d20020b5749f7c90cfd2a7cd6d4b7bcd5af2edc5d8f2c7d1845d4af7943","last_reissued_at":"2026-07-05T10:58:50.853370Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:58:50.853370Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Higgs-like inflation under ACTivated mass","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc"],"primary_cat":"hep-ph","authors_text":"Wen Yin","submitted_at":"2025-05-05T20:03:27Z","abstract_excerpt":"Recent analyses that combine the latest data from the Atacama Cosmology Telescope (ACT) with cosmic microwave background observations by BICEP/Keck and Planck, together with the DESI baryon acoustic-baryonic-oscillation (BAO) measurements, have tightened the limits on inflationary scenarios. The joint data set yields a spectral index of primordial scalar perturbations $n_s = 0.9743 \\pm 0.0034$ and an upper bound on the tensor-to-scalar ratio of $r < 0.038$. This slight upward shift in $n_s$ puts the previously favored Starobinsky model, and the conventional metric Higgs(-like) inflation--based"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2505.03004","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2505.03004/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":"2505.03004","created_at":"2026-07-05T10:58:50.853428+00:00"},{"alias_kind":"arxiv_version","alias_value":"2505.03004v1","created_at":"2026-07-05T10:58:50.853428+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2505.03004","created_at":"2026-07-05T10:58:50.853428+00:00"},{"alias_kind":"pith_short_12","alias_value":"RMBW2IACBNLU","created_at":"2026-07-05T10:58:50.853428+00:00"},{"alias_kind":"pith_short_16","alias_value":"RMBW2IACBNLUT56J","created_at":"2026-07-05T10:58:50.853428+00:00"},{"alias_kind":"pith_short_8","alias_value":"RMBW2IAC","created_at":"2026-07-05T10:58:50.853428+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":12,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.06112","citing_title":"Starobinsky Inflation in k-Essence Framework: Attractor Dynamics, Reheating, and Consistency with ACT DR6","ref_index":24,"is_internal_anchor":true},{"citing_arxiv_id":"2606.31362","citing_title":"Running into tension: primordial black holes from ultra-slow-roll inflation, spectral running, and the Hubble tension","ref_index":89,"is_internal_anchor":false},{"citing_arxiv_id":"2605.27727","citing_title":"Reconstructing ACT-compatible and GW170817-compatible Einstein-Gauss-Bonnet Inflation from the Observational Indices","ref_index":74,"is_internal_anchor":false},{"citing_arxiv_id":"2505.10534","citing_title":"ACT-ing on inflation: Implications of non Bunch-Davies initial condition and reheating on single-field slow roll models","ref_index":26,"is_internal_anchor":false},{"citing_arxiv_id":"2510.18320","citing_title":"The implications of inflation for the last ACT","ref_index":25,"is_internal_anchor":false},{"citing_arxiv_id":"2605.17813","citing_title":"ACT Data and Positive Running of the Spectral Index for Scalar Theory and Modified Gravity","ref_index":41,"is_internal_anchor":false},{"citing_arxiv_id":"2511.04933","citing_title":"Low-reheating scenario in dark Higgs inflation and its impact on dark photon dark matter production","ref_index":87,"is_internal_anchor":false},{"citing_arxiv_id":"2512.09079","citing_title":"Curvaton-assisted hilltop inflation","ref_index":25,"is_internal_anchor":false},{"citing_arxiv_id":"2602.05623","citing_title":"Induced-Gravity Palatini-Like Higgs Inflation in Supergravity Confronts ACT DR6","ref_index":23,"is_internal_anchor":false},{"citing_arxiv_id":"2604.18861","citing_title":"String-inspired Gauss-Bonnet Gravity Inflation and ACT","ref_index":54,"is_internal_anchor":false},{"citing_arxiv_id":"2604.14659","citing_title":"Constraining Quintessential Inflation with ACT: A Gauss-Bonnet Gateway","ref_index":67,"is_internal_anchor":false},{"citing_arxiv_id":"2604.17430","citing_title":"Testing $\\alpha$-attractor P-model of inflation by Cosmic Microwave Background radiation","ref_index":18,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/RMBW2IACBNLUT56JBT6SU7GW2S","json":"https://pith.science/pith/RMBW2IACBNLUT56JBT6SU7GW2S.json","graph_json":"https://pith.science/api/pith-number/RMBW2IACBNLUT56JBT6SU7GW2S/graph.json","events_json":"https://pith.science/api/pith-number/RMBW2IACBNLUT56JBT6SU7GW2S/events.json","paper":"https://pith.science/paper/RMBW2IAC"},"agent_actions":{"view_html":"https://pith.science/pith/RMBW2IACBNLUT56JBT6SU7GW2S","download_json":"https://pith.science/pith/RMBW2IACBNLUT56JBT6SU7GW2S.json","view_paper":"https://pith.science/paper/RMBW2IAC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2505.03004&json=true","fetch_graph":"https://pith.science/api/pith-number/RMBW2IACBNLUT56JBT6SU7GW2S/graph.json","fetch_events":"https://pith.science/api/pith-number/RMBW2IACBNLUT56JBT6SU7GW2S/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RMBW2IACBNLUT56JBT6SU7GW2S/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RMBW2IACBNLUT56JBT6SU7GW2S/action/storage_attestation","attest_author":"https://pith.science/pith/RMBW2IACBNLUT56JBT6SU7GW2S/action/author_attestation","sign_citation":"https://pith.science/pith/RMBW2IACBNLUT56JBT6SU7GW2S/action/citation_signature","submit_replication":"https://pith.science/pith/RMBW2IACBNLUT56JBT6SU7GW2S/action/replication_record"}},"created_at":"2026-07-05T10:58:50.853428+00:00","updated_at":"2026-07-05T10:58:50.853428+00:00"}