{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:Y6BHKWOKVQ2GU52TRPAFR4BP2B","short_pith_number":"pith:Y6BHKWOK","schema_version":"1.0","canonical_sha256":"c7827559caac346a77538bc058f02fd04333a6e4e4c4db00d5c0e8f6c522ead6","source":{"kind":"arxiv","id":"2304.04065","version":2},"attestation_state":"computed","paper":{"title":"Galileon inflation evades the no-go for PBH formation in the single-field framework","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph","hep-th"],"primary_cat":"astro-ph.CO","authors_text":"M. Sami, Sayantan Choudhury, Sudhakar Panda","submitted_at":"2023-04-08T16:31:31Z","abstract_excerpt":"We consider Galileon inflation in the Effective Field Theory (EFT) framework and examine the possibility for PBH formation during slow roll (SR) to ultra slow roll (USR) transitions. We show that loop corrections to the power spectrum, in this case, do not impose additional constraints on the masses of PBHs produced. We indicate that the remarkable non-renormalization property of Galileans due to generalized shift symmetry dubbed as Galilean symmetry is responsible for protecting PBH formation from quantum loop corrections."},"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":"2304.04065","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2023-04-08T16:31:31Z","cross_cats_sorted":["gr-qc","hep-ph","hep-th"],"title_canon_sha256":"590d8e1f7370025334b6de21ea14caba6ddf9d5b5b999cba9b63dc8b8221e085","abstract_canon_sha256":"f2af79032ea5894419e4dac1cc5b220d7eaa903c362992d3baf3219f2d8ac826"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:46:03.065533Z","signature_b64":"QCMWBe+Yjj9+DQc4Lv5KDxqB2hwXiS3kS064Q5XxMLtnaH8i33JiGChACw+LnO/qyRwuSvwhM7hZrJBlrQMsAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c7827559caac346a77538bc058f02fd04333a6e4e4c4db00d5c0e8f6c522ead6","last_reissued_at":"2026-07-05T06:46:03.065093Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:46:03.065093Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Galileon inflation evades the no-go for PBH formation in the single-field framework","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph","hep-th"],"primary_cat":"astro-ph.CO","authors_text":"M. Sami, Sayantan Choudhury, Sudhakar Panda","submitted_at":"2023-04-08T16:31:31Z","abstract_excerpt":"We consider Galileon inflation in the Effective Field Theory (EFT) framework and examine the possibility for PBH formation during slow roll (SR) to ultra slow roll (USR) transitions. We show that loop corrections to the power spectrum, in this case, do not impose additional constraints on the masses of PBHs produced. We indicate that the remarkable non-renormalization property of Galileans due to generalized shift symmetry dubbed as Galilean symmetry is responsible for protecting PBH formation from quantum loop corrections."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2304.04065","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/2304.04065/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":"2304.04065","created_at":"2026-07-05T06:46:03.065159+00:00"},{"alias_kind":"arxiv_version","alias_value":"2304.04065v2","created_at":"2026-07-05T06:46:03.065159+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2304.04065","created_at":"2026-07-05T06:46:03.065159+00:00"},{"alias_kind":"pith_short_12","alias_value":"Y6BHKWOKVQ2G","created_at":"2026-07-05T06:46:03.065159+00:00"},{"alias_kind":"pith_short_16","alias_value":"Y6BHKWOKVQ2GU52T","created_at":"2026-07-05T06:46:03.065159+00:00"},{"alias_kind":"pith_short_8","alias_value":"Y6BHKWOK","created_at":"2026-07-05T06:46:03.065159+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":5,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.24111","citing_title":"Constant-Roll Inflation: Analytical Formulae for Power Spectrum and Implications for Induced Gravitational Waves","ref_index":53,"is_internal_anchor":false},{"citing_arxiv_id":"2606.06355","citing_title":"$\\tt BlackHawk$ $\\tt v3.0$: Hawking Radiation from Regular Black Holes","ref_index":146,"is_internal_anchor":false},{"citing_arxiv_id":"2502.09481","citing_title":"Non-Perturbative Hamiltonian and Higher Loop Corrections in USR Inflation","ref_index":25,"is_internal_anchor":false},{"citing_arxiv_id":"2502.10287","citing_title":"Hamiltonians to all Orders in Perturbation Theory and Higher Loop Corrections in Single Field Inflation with PBHs Formation","ref_index":13,"is_internal_anchor":false},{"citing_arxiv_id":"2507.09552","citing_title":"Probing the scalar-induced gravitational waves with the Five-hundred-meter Aperture Spherical radio Telescope and the Square Kilometer Array","ref_index":85,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/Y6BHKWOKVQ2GU52TRPAFR4BP2B","json":"https://pith.science/pith/Y6BHKWOKVQ2GU52TRPAFR4BP2B.json","graph_json":"https://pith.science/api/pith-number/Y6BHKWOKVQ2GU52TRPAFR4BP2B/graph.json","events_json":"https://pith.science/api/pith-number/Y6BHKWOKVQ2GU52TRPAFR4BP2B/events.json","paper":"https://pith.science/paper/Y6BHKWOK"},"agent_actions":{"view_html":"https://pith.science/pith/Y6BHKWOKVQ2GU52TRPAFR4BP2B","download_json":"https://pith.science/pith/Y6BHKWOKVQ2GU52TRPAFR4BP2B.json","view_paper":"https://pith.science/paper/Y6BHKWOK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2304.04065&json=true","fetch_graph":"https://pith.science/api/pith-number/Y6BHKWOKVQ2GU52TRPAFR4BP2B/graph.json","fetch_events":"https://pith.science/api/pith-number/Y6BHKWOKVQ2GU52TRPAFR4BP2B/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/Y6BHKWOKVQ2GU52TRPAFR4BP2B/action/timestamp_anchor","attest_storage":"https://pith.science/pith/Y6BHKWOKVQ2GU52TRPAFR4BP2B/action/storage_attestation","attest_author":"https://pith.science/pith/Y6BHKWOKVQ2GU52TRPAFR4BP2B/action/author_attestation","sign_citation":"https://pith.science/pith/Y6BHKWOKVQ2GU52TRPAFR4BP2B/action/citation_signature","submit_replication":"https://pith.science/pith/Y6BHKWOKVQ2GU52TRPAFR4BP2B/action/replication_record"}},"created_at":"2026-07-05T06:46:03.065159+00:00","updated_at":"2026-07-05T06:46:03.065159+00:00"}