{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:JLMG3GTNM6HTOAVW2URJITWQ7D","short_pith_number":"pith:JLMG3GTN","schema_version":"1.0","canonical_sha256":"4ad86d9a6d678f3702b6d522944ed0f8d828ab99477c317cdb16bade8dca1f15","source":{"kind":"arxiv","id":"1912.01638","version":2},"attestation_state":"computed","paper":{"title":"Detuning primordial black hole dark matter with early matter domination and axion monodromy","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":"Fabrizio Rompineve, Guillermo Ballesteros, Juli\\'an Rey","submitted_at":"2019-12-03T19:17:52Z","abstract_excerpt":"We present a scenario that ameliorates the tuning problems present in models of primordial black hole dark matter from inflation. Our setup employs the advantages of gravitational collapse in a long epoch of early matter domination with reheating temperature $\\lesssim 10^{6}~\\text{GeV}$. Furthermore, we make use of a string-inspired class of models where the inflaton is identified with a non-compact axion field. In this framework, the presence of multiple local minima in the inflaton potential can be traced back to an approximate discrete shift symmetry. This scenario allows the formation of p"},"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":"1912.01638","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2019-12-03T19:17:52Z","cross_cats_sorted":["gr-qc","hep-ph","hep-th"],"title_canon_sha256":"ba9bf6492e08a56d92ed6fc3d28d81e3fd1285070a995f0191be5ff3cc66a9c0","abstract_canon_sha256":"43a8b6d26e0e345caab7366431dd58ff2a488d444770406c528d0648a24294b7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:11:43.341943Z","signature_b64":"7X3ho/ZyEwZzGZR3oOzN+42A6f4zH2L4AggTy/Qaw3HzM72YXXKpYhlFk/SuQTV57wm8ztAJMhckDx1bwLwZBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4ad86d9a6d678f3702b6d522944ed0f8d828ab99477c317cdb16bade8dca1f15","last_reissued_at":"2026-07-05T01:11:43.341510Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:11:43.341510Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Detuning primordial black hole dark matter with early matter domination and axion monodromy","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":"Fabrizio Rompineve, Guillermo Ballesteros, Juli\\'an Rey","submitted_at":"2019-12-03T19:17:52Z","abstract_excerpt":"We present a scenario that ameliorates the tuning problems present in models of primordial black hole dark matter from inflation. Our setup employs the advantages of gravitational collapse in a long epoch of early matter domination with reheating temperature $\\lesssim 10^{6}~\\text{GeV}$. Furthermore, we make use of a string-inspired class of models where the inflaton is identified with a non-compact axion field. In this framework, the presence of multiple local minima in the inflaton potential can be traced back to an approximate discrete shift symmetry. This scenario allows the formation of p"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1912.01638","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/1912.01638/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":"1912.01638","created_at":"2026-07-05T01:11:43.341594+00:00"},{"alias_kind":"arxiv_version","alias_value":"1912.01638v2","created_at":"2026-07-05T01:11:43.341594+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1912.01638","created_at":"2026-07-05T01:11:43.341594+00:00"},{"alias_kind":"pith_short_12","alias_value":"JLMG3GTNM6HT","created_at":"2026-07-05T01:11:43.341594+00:00"},{"alias_kind":"pith_short_16","alias_value":"JLMG3GTNM6HTOAVW","created_at":"2026-07-05T01:11:43.341594+00:00"},{"alias_kind":"pith_short_8","alias_value":"JLMG3GTN","created_at":"2026-07-05T01:11:43.341594+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.11332","citing_title":"Reviving primordial black hole formation in slow first-order phase transitions","ref_index":47,"is_internal_anchor":false},{"citing_arxiv_id":"2605.11332","citing_title":"Reviving primordial black hole formation in slow first-order phase transitions","ref_index":46,"is_internal_anchor":false},{"citing_arxiv_id":"2604.25726","citing_title":"Imprint of domain wall annihilation on induced gravitational waves","ref_index":101,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/JLMG3GTNM6HTOAVW2URJITWQ7D","json":"https://pith.science/pith/JLMG3GTNM6HTOAVW2URJITWQ7D.json","graph_json":"https://pith.science/api/pith-number/JLMG3GTNM6HTOAVW2URJITWQ7D/graph.json","events_json":"https://pith.science/api/pith-number/JLMG3GTNM6HTOAVW2URJITWQ7D/events.json","paper":"https://pith.science/paper/JLMG3GTN"},"agent_actions":{"view_html":"https://pith.science/pith/JLMG3GTNM6HTOAVW2URJITWQ7D","download_json":"https://pith.science/pith/JLMG3GTNM6HTOAVW2URJITWQ7D.json","view_paper":"https://pith.science/paper/JLMG3GTN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1912.01638&json=true","fetch_graph":"https://pith.science/api/pith-number/JLMG3GTNM6HTOAVW2URJITWQ7D/graph.json","fetch_events":"https://pith.science/api/pith-number/JLMG3GTNM6HTOAVW2URJITWQ7D/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JLMG3GTNM6HTOAVW2URJITWQ7D/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JLMG3GTNM6HTOAVW2URJITWQ7D/action/storage_attestation","attest_author":"https://pith.science/pith/JLMG3GTNM6HTOAVW2URJITWQ7D/action/author_attestation","sign_citation":"https://pith.science/pith/JLMG3GTNM6HTOAVW2URJITWQ7D/action/citation_signature","submit_replication":"https://pith.science/pith/JLMG3GTNM6HTOAVW2URJITWQ7D/action/replication_record"}},"created_at":"2026-07-05T01:11:43.341594+00:00","updated_at":"2026-07-05T01:11:43.341594+00:00"}