{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:FVCVBCL2FUBGC2FJ4NUIFNXM5W","short_pith_number":"pith:FVCVBCL2","schema_version":"1.0","canonical_sha256":"2d4550897a2d026168a9e36882b6eced8be022063561faf28bcceea85ab96ce4","source":{"kind":"arxiv","id":"2312.02275","version":3},"attestation_state":"computed","paper":{"title":"Examining the effects of dark matter spikes on eccentric intermediate mass ratio inspirals using N-body simulations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","gr-qc"],"primary_cat":"astro-ph.CO","authors_text":"A. Miguel Holgado, Diptajyoti Mukherjee, Go Ogiya, Hy Trac","submitted_at":"2023-12-04T19:00:06Z","abstract_excerpt":"Recent studies suggest that dark matter (DM) spikes around intermediate-mass black holes could cause observable dephasing in gravitational wave (GW) signals from Intermediate Mass Ratio Inspirals (IMRIs). Previous research primarily used non-self-consistent analytic methods to estimate the impact of DM spikes on eccentric IMRIs. Our study provides the first self-consistent treatment of this phenomenon using $N$-body simulations, incorporating Post-Newtonian effects up to the 2.5 order for accurate and robust results. Contrary to prior works, which posited that the cumulative effect of two-body"},"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":"2312.02275","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2023-12-04T19:00:06Z","cross_cats_sorted":["astro-ph.GA","gr-qc"],"title_canon_sha256":"ec4bed986d4125733e9b15d90972c66132d149ef28b94dac9cbd8207329f8cb8","abstract_canon_sha256":"a09113eb2ad40ba2a7531242d65fb8851e25af5a98fc4136582d9b70b70c5bc6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:02:39.917871Z","signature_b64":"JxEEOFtRnLb8pA+4CzPPDrsya3YtsuEEIkYQ+k/pQ95wVQJ0+WyymECdGyqGduJtSpmWALStH2WMkgpynGVHDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2d4550897a2d026168a9e36882b6eced8be022063561faf28bcceea85ab96ce4","last_reissued_at":"2026-07-05T09:02:39.917362Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:02:39.917362Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Examining the effects of dark matter spikes on eccentric intermediate mass ratio inspirals using N-body simulations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","gr-qc"],"primary_cat":"astro-ph.CO","authors_text":"A. Miguel Holgado, Diptajyoti Mukherjee, Go Ogiya, Hy Trac","submitted_at":"2023-12-04T19:00:06Z","abstract_excerpt":"Recent studies suggest that dark matter (DM) spikes around intermediate-mass black holes could cause observable dephasing in gravitational wave (GW) signals from Intermediate Mass Ratio Inspirals (IMRIs). Previous research primarily used non-self-consistent analytic methods to estimate the impact of DM spikes on eccentric IMRIs. Our study provides the first self-consistent treatment of this phenomenon using $N$-body simulations, incorporating Post-Newtonian effects up to the 2.5 order for accurate and robust results. Contrary to prior works, which posited that the cumulative effect of two-body"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2312.02275","kind":"arxiv","version":3},"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/2312.02275/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":"2312.02275","created_at":"2026-07-05T09:02:39.917425+00:00"},{"alias_kind":"arxiv_version","alias_value":"2312.02275v3","created_at":"2026-07-05T09:02:39.917425+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2312.02275","created_at":"2026-07-05T09:02:39.917425+00:00"},{"alias_kind":"pith_short_12","alias_value":"FVCVBCL2FUBG","created_at":"2026-07-05T09:02:39.917425+00:00"},{"alias_kind":"pith_short_16","alias_value":"FVCVBCL2FUBGC2FJ","created_at":"2026-07-05T09:02:39.917425+00:00"},{"alias_kind":"pith_short_8","alias_value":"FVCVBCL2","created_at":"2026-07-05T09:02:39.917425+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2411.14063","citing_title":"Probing dark matter halo profiles with multi-band observations of gravitational waves","ref_index":55,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FVCVBCL2FUBGC2FJ4NUIFNXM5W","json":"https://pith.science/pith/FVCVBCL2FUBGC2FJ4NUIFNXM5W.json","graph_json":"https://pith.science/api/pith-number/FVCVBCL2FUBGC2FJ4NUIFNXM5W/graph.json","events_json":"https://pith.science/api/pith-number/FVCVBCL2FUBGC2FJ4NUIFNXM5W/events.json","paper":"https://pith.science/paper/FVCVBCL2"},"agent_actions":{"view_html":"https://pith.science/pith/FVCVBCL2FUBGC2FJ4NUIFNXM5W","download_json":"https://pith.science/pith/FVCVBCL2FUBGC2FJ4NUIFNXM5W.json","view_paper":"https://pith.science/paper/FVCVBCL2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2312.02275&json=true","fetch_graph":"https://pith.science/api/pith-number/FVCVBCL2FUBGC2FJ4NUIFNXM5W/graph.json","fetch_events":"https://pith.science/api/pith-number/FVCVBCL2FUBGC2FJ4NUIFNXM5W/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FVCVBCL2FUBGC2FJ4NUIFNXM5W/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FVCVBCL2FUBGC2FJ4NUIFNXM5W/action/storage_attestation","attest_author":"https://pith.science/pith/FVCVBCL2FUBGC2FJ4NUIFNXM5W/action/author_attestation","sign_citation":"https://pith.science/pith/FVCVBCL2FUBGC2FJ4NUIFNXM5W/action/citation_signature","submit_replication":"https://pith.science/pith/FVCVBCL2FUBGC2FJ4NUIFNXM5W/action/replication_record"}},"created_at":"2026-07-05T09:02:39.917425+00:00","updated_at":"2026-07-05T09:02:39.917425+00:00"}