{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:2XIRO4GO4WOGDXVGQZ2MR5HYEL","short_pith_number":"pith:2XIRO4GO","schema_version":"1.0","canonical_sha256":"d5d11770cee59c61dea68674c8f4f822c01310bc2dcb991f814e2527c8042e98","source":{"kind":"arxiv","id":"1707.03310","version":2},"attestation_state":"computed","paper":{"title":"Structure Formation and Microlensing with Axion Miniclusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"David J. E. Marsh, J\\'er\\'emie Quevillon, Malcolm Fairbairn, Simon Rozier","submitted_at":"2017-07-11T15:02:57Z","abstract_excerpt":"If the symmetry breaking responsible for axion dark matter production occurs during the radiation-dominated epoch in the early Universe, then this produces large amplitude perturbations that collapse into dense objects known as axion miniclusters. The characteristic minicluster mass, $M_0$, is set by the mass inside the horizon when axion oscillations begin. For the QCD axion $M_0\\sim 10^{-10}M_\\odot$, however for an axion-like particle $M_0$ can approach $M_\\odot$ or higher. Using the Press-Schechter formalism we compute the mass function of halos formed by hierarchical structure formation fr"},"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":"1707.03310","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2017-07-11T15:02:57Z","cross_cats_sorted":["astro-ph.GA","hep-ph"],"title_canon_sha256":"72cf1e95d84ccf3bdde435728bb3e63d92cd85b178ce59fcd9e7c2eb36f97b74","abstract_canon_sha256":"8392a7eb3cfea54d61ad5dcc42c3634fe7af2ab747d2fa4ea482b435d2b7f79a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T23:52:17.847230Z","signature_b64":"ZrvD1j7ztrCtnFZXOjWjM9S/KrJh/9LA9FkYMvEoZzjyqRTRDepFYw/yfvJMtXe27zduwICgKgDinx21Y0XwBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d5d11770cee59c61dea68674c8f4f822c01310bc2dcb991f814e2527c8042e98","last_reissued_at":"2026-07-04T23:52:17.846788Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T23:52:17.846788Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Structure Formation and Microlensing with Axion Miniclusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"David J. E. Marsh, J\\'er\\'emie Quevillon, Malcolm Fairbairn, Simon Rozier","submitted_at":"2017-07-11T15:02:57Z","abstract_excerpt":"If the symmetry breaking responsible for axion dark matter production occurs during the radiation-dominated epoch in the early Universe, then this produces large amplitude perturbations that collapse into dense objects known as axion miniclusters. The characteristic minicluster mass, $M_0$, is set by the mass inside the horizon when axion oscillations begin. For the QCD axion $M_0\\sim 10^{-10}M_\\odot$, however for an axion-like particle $M_0$ can approach $M_\\odot$ or higher. Using the Press-Schechter formalism we compute the mass function of halos formed by hierarchical structure formation fr"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1707.03310","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/1707.03310/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":"1707.03310","created_at":"2026-07-04T23:52:17.846842+00:00"},{"alias_kind":"arxiv_version","alias_value":"1707.03310v2","created_at":"2026-07-04T23:52:17.846842+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1707.03310","created_at":"2026-07-04T23:52:17.846842+00:00"},{"alias_kind":"pith_short_12","alias_value":"2XIRO4GO4WOG","created_at":"2026-07-04T23:52:17.846842+00:00"},{"alias_kind":"pith_short_16","alias_value":"2XIRO4GO4WOGDXVG","created_at":"2026-07-04T23:52:17.846842+00:00"},{"alias_kind":"pith_short_8","alias_value":"2XIRO4GO","created_at":"2026-07-04T23:52:17.846842+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":6,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.19439","citing_title":"From Rags to Jeans: Axion Miniclusters from Early matter domination","ref_index":85,"is_internal_anchor":false},{"citing_arxiv_id":"2607.01333","citing_title":"Axion Misalignment Across First-Order Phase Transitions","ref_index":56,"is_internal_anchor":false},{"citing_arxiv_id":"2605.28005","citing_title":"Transient axion streams from disrupted miniclusters","ref_index":23,"is_internal_anchor":false},{"citing_arxiv_id":"2508.14535","citing_title":"Axion Star Bosenova in Axion Miniclusters","ref_index":14,"is_internal_anchor":false},{"citing_arxiv_id":"2605.00103","citing_title":"Pre-inflationary QCD axion stars after moduli domination","ref_index":74,"is_internal_anchor":false},{"citing_arxiv_id":"2604.15241","citing_title":"Echoes of Global Cosmic Strings","ref_index":28,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/2XIRO4GO4WOGDXVGQZ2MR5HYEL","json":"https://pith.science/pith/2XIRO4GO4WOGDXVGQZ2MR5HYEL.json","graph_json":"https://pith.science/api/pith-number/2XIRO4GO4WOGDXVGQZ2MR5HYEL/graph.json","events_json":"https://pith.science/api/pith-number/2XIRO4GO4WOGDXVGQZ2MR5HYEL/events.json","paper":"https://pith.science/paper/2XIRO4GO"},"agent_actions":{"view_html":"https://pith.science/pith/2XIRO4GO4WOGDXVGQZ2MR5HYEL","download_json":"https://pith.science/pith/2XIRO4GO4WOGDXVGQZ2MR5HYEL.json","view_paper":"https://pith.science/paper/2XIRO4GO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1707.03310&json=true","fetch_graph":"https://pith.science/api/pith-number/2XIRO4GO4WOGDXVGQZ2MR5HYEL/graph.json","fetch_events":"https://pith.science/api/pith-number/2XIRO4GO4WOGDXVGQZ2MR5HYEL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2XIRO4GO4WOGDXVGQZ2MR5HYEL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2XIRO4GO4WOGDXVGQZ2MR5HYEL/action/storage_attestation","attest_author":"https://pith.science/pith/2XIRO4GO4WOGDXVGQZ2MR5HYEL/action/author_attestation","sign_citation":"https://pith.science/pith/2XIRO4GO4WOGDXVGQZ2MR5HYEL/action/citation_signature","submit_replication":"https://pith.science/pith/2XIRO4GO4WOGDXVGQZ2MR5HYEL/action/replication_record"}},"created_at":"2026-07-04T23:52:17.846842+00:00","updated_at":"2026-07-04T23:52:17.846842+00:00"}