{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:65ETIXEOSKDODT23Y5R272VOLE","short_pith_number":"pith:65ETIXEO","schema_version":"1.0","canonical_sha256":"f749345c8e9286e1cf5bc763afeaae59174573e243028392a816a6d6fd5005d0","source":{"kind":"arxiv","id":"2606.06557","version":1},"attestation_state":"computed","paper":{"title":"Robustness of the relativistic intermediate-axis instability around dark-matter-dressed rotating black holes","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"Mohsen Fathi","submitted_at":"2026-06-04T11:18:20Z","abstract_excerpt":"DARK-FLIP I introduced a semi-analytical and Python-based framework for studying a relativistic version of the intermediate-axis instability (IAI) of a coherent non-axisymmetric matter element around rotating black holes dressed by dark matter (DM). In this second paper I test the robustness of that idea. The main question is simple: if the local environment is changed by the DM profile, how does the flip frequency respond? To answer this, I use a controlled effective response model (ERM), not a full accretion or radiative-transfer simulation. The flip frequency is therefore treated as a diagn"},"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":"2606.06557","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2026-06-04T11:18:20Z","cross_cats_sorted":["astro-ph.CO","astro-ph.HE"],"title_canon_sha256":"c96b759ff800dce3e9f01514d91b9b0f6c3a93a41890fee01ac02535c2d1c7c4","abstract_canon_sha256":"fe2acdda7152e2e69f3bad4c24acab80f0157b883b5c8caee906aec1acedd660"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-06-08T00:03:44.370809Z","signature_b64":"xoGSMLdEbtpyi6LD1vosZnX87cN7E23G9ielp5rtRHbaNgq1MD0euMCEyCra0EDKamkQsWgqAH58MIFqLgn6DQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f749345c8e9286e1cf5bc763afeaae59174573e243028392a816a6d6fd5005d0","last_reissued_at":"2026-06-08T00:03:44.370015Z","signature_status":"signed_v1","first_computed_at":"2026-06-08T00:03:44.370015Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Robustness of the relativistic intermediate-axis instability around dark-matter-dressed rotating black holes","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"Mohsen Fathi","submitted_at":"2026-06-04T11:18:20Z","abstract_excerpt":"DARK-FLIP I introduced a semi-analytical and Python-based framework for studying a relativistic version of the intermediate-axis instability (IAI) of a coherent non-axisymmetric matter element around rotating black holes dressed by dark matter (DM). In this second paper I test the robustness of that idea. The main question is simple: if the local environment is changed by the DM profile, how does the flip frequency respond? To answer this, I use a controlled effective response model (ERM), not a full accretion or radiative-transfer simulation. The flip frequency is therefore treated as a diagn"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2606.06557","kind":"arxiv","version":1},"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/2606.06557/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":"2606.06557","created_at":"2026-06-08T00:03:44.370129+00:00"},{"alias_kind":"arxiv_version","alias_value":"2606.06557v1","created_at":"2026-06-08T00:03:44.370129+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2606.06557","created_at":"2026-06-08T00:03:44.370129+00:00"},{"alias_kind":"pith_short_12","alias_value":"65ETIXEOSKDO","created_at":"2026-06-08T00:03:44.370129+00:00"},{"alias_kind":"pith_short_16","alias_value":"65ETIXEOSKDODT23","created_at":"2026-06-08T00:03:44.370129+00:00"},{"alias_kind":"pith_short_8","alias_value":"65ETIXEO","created_at":"2026-06-08T00:03:44.370129+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/65ETIXEOSKDODT23Y5R272VOLE","json":"https://pith.science/pith/65ETIXEOSKDODT23Y5R272VOLE.json","graph_json":"https://pith.science/api/pith-number/65ETIXEOSKDODT23Y5R272VOLE/graph.json","events_json":"https://pith.science/api/pith-number/65ETIXEOSKDODT23Y5R272VOLE/events.json","paper":"https://pith.science/paper/65ETIXEO"},"agent_actions":{"view_html":"https://pith.science/pith/65ETIXEOSKDODT23Y5R272VOLE","download_json":"https://pith.science/pith/65ETIXEOSKDODT23Y5R272VOLE.json","view_paper":"https://pith.science/paper/65ETIXEO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2606.06557&json=true","fetch_graph":"https://pith.science/api/pith-number/65ETIXEOSKDODT23Y5R272VOLE/graph.json","fetch_events":"https://pith.science/api/pith-number/65ETIXEOSKDODT23Y5R272VOLE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/65ETIXEOSKDODT23Y5R272VOLE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/65ETIXEOSKDODT23Y5R272VOLE/action/storage_attestation","attest_author":"https://pith.science/pith/65ETIXEOSKDODT23Y5R272VOLE/action/author_attestation","sign_citation":"https://pith.science/pith/65ETIXEOSKDODT23Y5R272VOLE/action/citation_signature","submit_replication":"https://pith.science/pith/65ETIXEOSKDODT23Y5R272VOLE/action/replication_record"}},"created_at":"2026-06-08T00:03:44.370129+00:00","updated_at":"2026-06-08T00:03:44.370129+00:00"}