{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:JASK5YRE7DCMK4DSWQP5D6Y33R","short_pith_number":"pith:JASK5YRE","schema_version":"1.0","canonical_sha256":"4824aee224f8c4c57072b41fd1fb1bdc5fd244646fc3b06a873d999affe4191e","source":{"kind":"arxiv","id":"1909.03883","version":2},"attestation_state":"computed","paper":{"title":"Circular polarization of cosmic photons due to their interactions with Sterile neutrino dark matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"M. Haghighat, R.Mohammadi, S. Mahmoudi, S.S Xue, S. Tizchang","submitted_at":"2019-09-09T14:22:43Z","abstract_excerpt":"In this paper, we explore the possibility of the polarization conversion of a wide energy range of cosmic photons to the circular polarization through their interactions with right handed Sterile neutrinos as a candidate for dark matter. By considering the Sterile neutrino in the seesaw mechanism framework and right-handed current model, we examine the Faraday conversion $\\Delta \\phi_\\text{\\tiny{FC}}$ of gamma ray burst (GRB) photons at both the prompt and afterglow emission levels as well as the radio photons emitted from our galaxy and extra-galactic sources interacting with the Sterile neut"},"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":"1909.03883","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2019-09-09T14:22:43Z","cross_cats_sorted":[],"title_canon_sha256":"e70a9e79c3f4c98ee2c376e9e68e6023a6869ac48aa7a0a524229673edfb248f","abstract_canon_sha256":"9e0ec2d488df6f3c6883c01047ea2acf03e8f326f172279012c7565f3d694107"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:14:28.287995Z","signature_b64":"wXpJok9/gqEIyaIw/z9QCsDbqKbVmoghaybItFFdqTrTO9QpbJrHwB4ban1jBsH1ag7vbverSu3J6IxO5Gy4Dg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4824aee224f8c4c57072b41fd1fb1bdc5fd244646fc3b06a873d999affe4191e","last_reissued_at":"2026-07-05T01:14:28.287494Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:14:28.287494Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Circular polarization of cosmic photons due to their interactions with Sterile neutrino dark matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"M. Haghighat, R.Mohammadi, S. Mahmoudi, S.S Xue, S. Tizchang","submitted_at":"2019-09-09T14:22:43Z","abstract_excerpt":"In this paper, we explore the possibility of the polarization conversion of a wide energy range of cosmic photons to the circular polarization through their interactions with right handed Sterile neutrinos as a candidate for dark matter. By considering the Sterile neutrino in the seesaw mechanism framework and right-handed current model, we examine the Faraday conversion $\\Delta \\phi_\\text{\\tiny{FC}}$ of gamma ray burst (GRB) photons at both the prompt and afterglow emission levels as well as the radio photons emitted from our galaxy and extra-galactic sources interacting with the Sterile neut"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1909.03883","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/1909.03883/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":"1909.03883","created_at":"2026-07-05T01:14:28.287554+00:00"},{"alias_kind":"arxiv_version","alias_value":"1909.03883v2","created_at":"2026-07-05T01:14:28.287554+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1909.03883","created_at":"2026-07-05T01:14:28.287554+00:00"},{"alias_kind":"pith_short_12","alias_value":"JASK5YRE7DCM","created_at":"2026-07-05T01:14:28.287554+00:00"},{"alias_kind":"pith_short_16","alias_value":"JASK5YRE7DCMK4DS","created_at":"2026-07-05T01:14:28.287554+00:00"},{"alias_kind":"pith_short_8","alias_value":"JASK5YRE","created_at":"2026-07-05T01:14:28.287554+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2509.04028","citing_title":"Primordial black holes versus their impersonators at gravitational wave observatories","ref_index":87,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/JASK5YRE7DCMK4DSWQP5D6Y33R","json":"https://pith.science/pith/JASK5YRE7DCMK4DSWQP5D6Y33R.json","graph_json":"https://pith.science/api/pith-number/JASK5YRE7DCMK4DSWQP5D6Y33R/graph.json","events_json":"https://pith.science/api/pith-number/JASK5YRE7DCMK4DSWQP5D6Y33R/events.json","paper":"https://pith.science/paper/JASK5YRE"},"agent_actions":{"view_html":"https://pith.science/pith/JASK5YRE7DCMK4DSWQP5D6Y33R","download_json":"https://pith.science/pith/JASK5YRE7DCMK4DSWQP5D6Y33R.json","view_paper":"https://pith.science/paper/JASK5YRE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1909.03883&json=true","fetch_graph":"https://pith.science/api/pith-number/JASK5YRE7DCMK4DSWQP5D6Y33R/graph.json","fetch_events":"https://pith.science/api/pith-number/JASK5YRE7DCMK4DSWQP5D6Y33R/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JASK5YRE7DCMK4DSWQP5D6Y33R/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JASK5YRE7DCMK4DSWQP5D6Y33R/action/storage_attestation","attest_author":"https://pith.science/pith/JASK5YRE7DCMK4DSWQP5D6Y33R/action/author_attestation","sign_citation":"https://pith.science/pith/JASK5YRE7DCMK4DSWQP5D6Y33R/action/citation_signature","submit_replication":"https://pith.science/pith/JASK5YRE7DCMK4DSWQP5D6Y33R/action/replication_record"}},"created_at":"2026-07-05T01:14:28.287554+00:00","updated_at":"2026-07-05T01:14:28.287554+00:00"}