{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:4JBSMI7YX53XKAEDKAMJNZDLH7","short_pith_number":"pith:4JBSMI7Y","schema_version":"1.0","canonical_sha256":"e2432623f8bf77750083501896e46b3fcd80f37cb005b81db47106e468c92270","source":{"kind":"arxiv","id":"2607.19113","version":1},"attestation_state":"computed","paper":{"title":"Modes in Transitional Millisecond Pulsars: Evidence of Pulsar Wind-Induced Disk Heating from GRMHD and Radiative Transfer","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Linares Manuel, Mignon-Risse Rapha\\\"el, Parfrey Kyle, Ressler Sean, Tchekhovskoy Alexander","submitted_at":"2026-07-21T13:56:38Z","abstract_excerpt":"Transitional millisecond pulsars (tMSPs) alternate between radio and X-ray pulsar states, and can represent the missing link between rotation- and accretion-powered neutron stars. Their disk state switches stochastically between the low and high X-ray modes, both of unknown physical origin and less luminous than low-mass X-ray binaries. To reveal the source of the X-ray emission, we carry out 2D axisymmetric general-relativistic magnetohydrodynamical simulations of the interaction between an accretion disk and tMSP magnetosphere. For the first time, we post-process tMSP simulations with a radi"},"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":"2607.19113","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2026-07-21T13:56:38Z","cross_cats_sorted":[],"title_canon_sha256":"3826ab4a7195e0cb65152ce098d10f7b54e9444be16d0f4c2fede3acad831d8c","abstract_canon_sha256":"de4afa2d9e243170b8f65fd8bce458ce923f8da20d3d7918fa3e1e8837932e55"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-22T01:24:09.257372Z","signature_b64":"YCqqipCk5ZtKDPQud9GsW1rKiAFNBqWX9CYkXRdVxiLispM9MsMDAo4D7VdLiVRBbWRSro2adYDfjMb8SZQgBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e2432623f8bf77750083501896e46b3fcd80f37cb005b81db47106e468c92270","last_reissued_at":"2026-07-22T01:24:09.256519Z","signature_status":"signed_v1","first_computed_at":"2026-07-22T01:24:09.256519Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Modes in Transitional Millisecond Pulsars: Evidence of Pulsar Wind-Induced Disk Heating from GRMHD and Radiative Transfer","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Linares Manuel, Mignon-Risse Rapha\\\"el, Parfrey Kyle, Ressler Sean, Tchekhovskoy Alexander","submitted_at":"2026-07-21T13:56:38Z","abstract_excerpt":"Transitional millisecond pulsars (tMSPs) alternate between radio and X-ray pulsar states, and can represent the missing link between rotation- and accretion-powered neutron stars. Their disk state switches stochastically between the low and high X-ray modes, both of unknown physical origin and less luminous than low-mass X-ray binaries. To reveal the source of the X-ray emission, we carry out 2D axisymmetric general-relativistic magnetohydrodynamical simulations of the interaction between an accretion disk and tMSP magnetosphere. For the first time, we post-process tMSP simulations with a radi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2607.19113","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/2607.19113/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":"2607.19113","created_at":"2026-07-22T01:24:09.256960+00:00"},{"alias_kind":"arxiv_version","alias_value":"2607.19113v1","created_at":"2026-07-22T01:24:09.256960+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2607.19113","created_at":"2026-07-22T01:24:09.256960+00:00"},{"alias_kind":"pith_short_12","alias_value":"4JBSMI7YX53X","created_at":"2026-07-22T01:24:09.256960+00:00"},{"alias_kind":"pith_short_16","alias_value":"4JBSMI7YX53XKAED","created_at":"2026-07-22T01:24:09.256960+00:00"},{"alias_kind":"pith_short_8","alias_value":"4JBSMI7Y","created_at":"2026-07-22T01:24:09.256960+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/4JBSMI7YX53XKAEDKAMJNZDLH7","json":"https://pith.science/pith/4JBSMI7YX53XKAEDKAMJNZDLH7.json","graph_json":"https://pith.science/api/pith-number/4JBSMI7YX53XKAEDKAMJNZDLH7/graph.json","events_json":"https://pith.science/api/pith-number/4JBSMI7YX53XKAEDKAMJNZDLH7/events.json","paper":"https://pith.science/paper/4JBSMI7Y"},"agent_actions":{"view_html":"https://pith.science/pith/4JBSMI7YX53XKAEDKAMJNZDLH7","download_json":"https://pith.science/pith/4JBSMI7YX53XKAEDKAMJNZDLH7.json","view_paper":"https://pith.science/paper/4JBSMI7Y","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2607.19113&json=true","fetch_graph":"https://pith.science/api/pith-number/4JBSMI7YX53XKAEDKAMJNZDLH7/graph.json","fetch_events":"https://pith.science/api/pith-number/4JBSMI7YX53XKAEDKAMJNZDLH7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4JBSMI7YX53XKAEDKAMJNZDLH7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4JBSMI7YX53XKAEDKAMJNZDLH7/action/storage_attestation","attest_author":"https://pith.science/pith/4JBSMI7YX53XKAEDKAMJNZDLH7/action/author_attestation","sign_citation":"https://pith.science/pith/4JBSMI7YX53XKAEDKAMJNZDLH7/action/citation_signature","submit_replication":"https://pith.science/pith/4JBSMI7YX53XKAEDKAMJNZDLH7/action/replication_record"}},"created_at":"2026-07-22T01:24:09.256960+00:00","updated_at":"2026-07-22T01:24:09.256960+00:00"}