{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:PIKGUK6JWQYFEHNWOPCPKNO3TM","short_pith_number":"pith:PIKGUK6J","schema_version":"1.0","canonical_sha256":"7a146a2bc9b430521db673c4f535db9b3bb64aaec50803a820414194c06c168b","source":{"kind":"arxiv","id":"2404.12779","version":2},"attestation_state":"computed","paper":{"title":"Inflation, the Hubble Tension and Early Dark Energy: an alternative overview","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"William Giar\\`e","submitted_at":"2024-04-19T10:36:37Z","abstract_excerpt":"I review and discuss the possible implications for inflation resulting from considering new physics in light of the Hubble tension. My study is motivated by a simple argument that the constraints on inflationary parameters, most typically the spectral index $n_s$, depend to some extent on the cosmological framework. To avoid broadening the uncertainties resulting from marginalizing over additional parameters (typical in many alternative models), I first adopt the same alternative viewpoint of previous studies and analyze what happens if a physical theory can fix extra parameters to non-standar"},"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":"2404.12779","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2024-04-19T10:36:37Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"8fca3d08a8c50ea583dcf51b853a081202433bdadd94b6097b5928ebf2ad98d1","abstract_canon_sha256":"0ab605c51951983941463da65ee2860d3000dce59a0be023851187363e0dde40"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:37:19.551102Z","signature_b64":"FnLD7Ip1+D6ijbqlr2OHBUDszkp2q6q4OI3DypS62kPKSmXinvw+KFF7yibhp/R8Xwbx1weKZDjWzpa5IWzeDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7a146a2bc9b430521db673c4f535db9b3bb64aaec50803a820414194c06c168b","last_reissued_at":"2026-07-05T08:37:19.550630Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:37:19.550630Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Inflation, the Hubble Tension and Early Dark Energy: an alternative overview","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"William Giar\\`e","submitted_at":"2024-04-19T10:36:37Z","abstract_excerpt":"I review and discuss the possible implications for inflation resulting from considering new physics in light of the Hubble tension. My study is motivated by a simple argument that the constraints on inflationary parameters, most typically the spectral index $n_s$, depend to some extent on the cosmological framework. To avoid broadening the uncertainties resulting from marginalizing over additional parameters (typical in many alternative models), I first adopt the same alternative viewpoint of previous studies and analyze what happens if a physical theory can fix extra parameters to non-standar"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2404.12779","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/2404.12779/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":"2404.12779","created_at":"2026-07-05T08:37:19.550686+00:00"},{"alias_kind":"arxiv_version","alias_value":"2404.12779v2","created_at":"2026-07-05T08:37:19.550686+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2404.12779","created_at":"2026-07-05T08:37:19.550686+00:00"},{"alias_kind":"pith_short_12","alias_value":"PIKGUK6JWQYF","created_at":"2026-07-05T08:37:19.550686+00:00"},{"alias_kind":"pith_short_16","alias_value":"PIKGUK6JWQYFEHNW","created_at":"2026-07-05T08:37:19.550686+00:00"},{"alias_kind":"pith_short_8","alias_value":"PIKGUK6J","created_at":"2026-07-05T08:37:19.550686+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":7,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.06147","citing_title":"Imprint of swampland-inspired coupled early dark energy","ref_index":140,"is_internal_anchor":true},{"citing_arxiv_id":"2606.19090","citing_title":"Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data","ref_index":23,"is_internal_anchor":false},{"citing_arxiv_id":"2606.06495","citing_title":"What it takes to solve the Hubble tension through Modifications of Cosmological Recombination II: in light of ACT DR6 and DESI DR2","ref_index":98,"is_internal_anchor":false},{"citing_arxiv_id":"2605.26116","citing_title":"Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions","ref_index":119,"is_internal_anchor":false},{"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":150,"is_internal_anchor":false},{"citing_arxiv_id":"2606.31324","citing_title":"Cosmological Viability of Exponential Infrared $f(T)$ Gravity","ref_index":131,"is_internal_anchor":false},{"citing_arxiv_id":"2604.13535","citing_title":"Double the axions, half the tension: multi-field early dark energy eases the Hubble tension","ref_index":135,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/PIKGUK6JWQYFEHNWOPCPKNO3TM","json":"https://pith.science/pith/PIKGUK6JWQYFEHNWOPCPKNO3TM.json","graph_json":"https://pith.science/api/pith-number/PIKGUK6JWQYFEHNWOPCPKNO3TM/graph.json","events_json":"https://pith.science/api/pith-number/PIKGUK6JWQYFEHNWOPCPKNO3TM/events.json","paper":"https://pith.science/paper/PIKGUK6J"},"agent_actions":{"view_html":"https://pith.science/pith/PIKGUK6JWQYFEHNWOPCPKNO3TM","download_json":"https://pith.science/pith/PIKGUK6JWQYFEHNWOPCPKNO3TM.json","view_paper":"https://pith.science/paper/PIKGUK6J","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2404.12779&json=true","fetch_graph":"https://pith.science/api/pith-number/PIKGUK6JWQYFEHNWOPCPKNO3TM/graph.json","fetch_events":"https://pith.science/api/pith-number/PIKGUK6JWQYFEHNWOPCPKNO3TM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PIKGUK6JWQYFEHNWOPCPKNO3TM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PIKGUK6JWQYFEHNWOPCPKNO3TM/action/storage_attestation","attest_author":"https://pith.science/pith/PIKGUK6JWQYFEHNWOPCPKNO3TM/action/author_attestation","sign_citation":"https://pith.science/pith/PIKGUK6JWQYFEHNWOPCPKNO3TM/action/citation_signature","submit_replication":"https://pith.science/pith/PIKGUK6JWQYFEHNWOPCPKNO3TM/action/replication_record"}},"created_at":"2026-07-05T08:37:19.550686+00:00","updated_at":"2026-07-05T08:37:19.550686+00:00"}