{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:TWOHUCK2WTBZE4ZZRUORSQATJ6","short_pith_number":"pith:TWOHUCK2","schema_version":"1.0","canonical_sha256":"9d9c7a095ab4c39273398d1d1940134f9d6c1ed5222a873c6c77be74fcf6d7fd","source":{"kind":"arxiv","id":"1711.06129","version":2},"attestation_state":"computed","paper":{"title":"Double inflation as a single origin of primordial black holes for all dark matter and LIGO observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Keisuke Inomata, Kyohei Mukaida, Masahiro Kawasaki, Tsutomu T. Yanagida","submitted_at":"2017-11-16T15:13:30Z","abstract_excerpt":"Primordial Black Hole (PBH) is one of the leading non-particle candidates for dark matter (DM). Although several observations severely constrain the amount of PBHs, it is recently pointed out that there is an uncertainty on the microlensing constraints below $\\sim 10^{-10} M_\\odot$ which was ignored originally but may weaken the constraints significantly. In this paper, facing this uncertainty, we investigate the possibility that PBHs can make up all DM in a broad mass spectrum. Moreover, we propose a concrete inflation model which can simultaneously produce PBHs for all DM in a broad mass spe"},"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":"1711.06129","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2017-11-16T15:13:30Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"092b2a60c1cdcd0a23d9a60392e1239556953f63c0f1746d248ca18eeb75a67d","abstract_canon_sha256":"523be4ba5d61d8f53d8259812d2c521dc5fc4a7cdc0f388fa448cbccbee3aa87"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:22:57.743003Z","signature_b64":"G5ZBcMPqnJ8apTMOAjWXstYI/YaW/m+5mZeLsnrPBHWAwEGSx8EKSqXGZLT8zs/cG17FvpnwJrwFvcB/WWRvAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9d9c7a095ab4c39273398d1d1940134f9d6c1ed5222a873c6c77be74fcf6d7fd","last_reissued_at":"2026-05-18T00:22:57.742369Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:22:57.742369Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Double inflation as a single origin of primordial black holes for all dark matter and LIGO observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Keisuke Inomata, Kyohei Mukaida, Masahiro Kawasaki, Tsutomu T. Yanagida","submitted_at":"2017-11-16T15:13:30Z","abstract_excerpt":"Primordial Black Hole (PBH) is one of the leading non-particle candidates for dark matter (DM). Although several observations severely constrain the amount of PBHs, it is recently pointed out that there is an uncertainty on the microlensing constraints below $\\sim 10^{-10} M_\\odot$ which was ignored originally but may weaken the constraints significantly. In this paper, facing this uncertainty, we investigate the possibility that PBHs can make up all DM in a broad mass spectrum. Moreover, we propose a concrete inflation model which can simultaneously produce PBHs for all DM in a broad mass spe"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.06129","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":""},"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":"1711.06129","created_at":"2026-05-18T00:22:57.742469+00:00"},{"alias_kind":"arxiv_version","alias_value":"1711.06129v2","created_at":"2026-05-18T00:22:57.742469+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1711.06129","created_at":"2026-05-18T00:22:57.742469+00:00"},{"alias_kind":"pith_short_12","alias_value":"TWOHUCK2WTBZ","created_at":"2026-05-18T12:31:46.661854+00:00"},{"alias_kind":"pith_short_16","alias_value":"TWOHUCK2WTBZE4ZZ","created_at":"2026-05-18T12:31:46.661854+00:00"},{"alias_kind":"pith_short_8","alias_value":"TWOHUCK2","created_at":"2026-05-18T12:31:46.661854+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":4,"sample":[{"citing_arxiv_id":"2607.01818","citing_title":"Gravitational Waves from Primordial Black Holes: Connecting Low-Frequency Scalar-Induced Signatures to High-Frequency Binary Mergers","ref_index":22,"is_internal_anchor":true},{"citing_arxiv_id":"2607.01780","citing_title":"Lattice study of primordial black hole formation in bumpy axion inflation","ref_index":15,"is_internal_anchor":true},{"citing_arxiv_id":"2606.07505","citing_title":"Primordial Black Hole Triggered Type Ia Supernovae II: Comparison with Supernova Remnants and Galactic Chemical Evolution","ref_index":144,"is_internal_anchor":true},{"citing_arxiv_id":"2109.01398","citing_title":"Scalar induced gravitational waves review","ref_index":254,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TWOHUCK2WTBZE4ZZRUORSQATJ6","json":"https://pith.science/pith/TWOHUCK2WTBZE4ZZRUORSQATJ6.json","graph_json":"https://pith.science/api/pith-number/TWOHUCK2WTBZE4ZZRUORSQATJ6/graph.json","events_json":"https://pith.science/api/pith-number/TWOHUCK2WTBZE4ZZRUORSQATJ6/events.json","paper":"https://pith.science/paper/TWOHUCK2"},"agent_actions":{"view_html":"https://pith.science/pith/TWOHUCK2WTBZE4ZZRUORSQATJ6","download_json":"https://pith.science/pith/TWOHUCK2WTBZE4ZZRUORSQATJ6.json","view_paper":"https://pith.science/paper/TWOHUCK2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1711.06129&json=true","fetch_graph":"https://pith.science/api/pith-number/TWOHUCK2WTBZE4ZZRUORSQATJ6/graph.json","fetch_events":"https://pith.science/api/pith-number/TWOHUCK2WTBZE4ZZRUORSQATJ6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TWOHUCK2WTBZE4ZZRUORSQATJ6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TWOHUCK2WTBZE4ZZRUORSQATJ6/action/storage_attestation","attest_author":"https://pith.science/pith/TWOHUCK2WTBZE4ZZRUORSQATJ6/action/author_attestation","sign_citation":"https://pith.science/pith/TWOHUCK2WTBZE4ZZRUORSQATJ6/action/citation_signature","submit_replication":"https://pith.science/pith/TWOHUCK2WTBZE4ZZRUORSQATJ6/action/replication_record"}},"created_at":"2026-05-18T00:22:57.742469+00:00","updated_at":"2026-05-18T00:22:57.742469+00:00"}