{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:7RWPNDWYPLEOEVPWEWKQ4XYFML","short_pith_number":"pith:7RWPNDWY","schema_version":"1.0","canonical_sha256":"fc6cf68ed87ac8e255f625950e5f0562f95e614ef2418a526f77f7bb574ab8de","source":{"kind":"arxiv","id":"1310.5991","version":2},"attestation_state":"computed","paper":{"title":"Gamma ray emission in Fermi bubbles and Higgs portal dark matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"Nobuchika Okada, Osamu Seto","submitted_at":"2013-10-22T17:20:13Z","abstract_excerpt":"It has been recently pointed out that the excess of the gamma ray spectrum in the Fermi Bubbles at low latitude can be well explained by the annihilation of dark matter particles. The best-fit candidate corresponds to the annihilation of a dark matter with mass of around $62$ GeV into $b \\bar{b}$ with the cross section, $\\sigma v \\simeq 3.3 \\times 10^{-26}$ cm$^3$/s, or the annihilation of a dark matter with mass of around $10$ GeV into a tau lepton pair with the cross section, $\\sigma v \\simeq 5.6 \\times 10^{-27}$ cm$^3$/s. We point out that the Higgs portal dark matter models are perfectly c"},"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":"1310.5991","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2013-10-22T17:20:13Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"dd059f93697b2a8ffcaf13852db7122696b1b8a6a2d6a0c599241f1156593e81","abstract_canon_sha256":"40ed8ba6b19ab9817d75856ba407aa5c4b537ea40a7dc2116abb6d6b6071dab1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:46:56.078375Z","signature_b64":"RxtOZWJgDhKSnCm13Pb8mOubWfe0keb9YvimmVZfgpbgnaeHYY0arvGCYkeCnnLPHjBWkjh2DQtRLNZMw8LHDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fc6cf68ed87ac8e255f625950e5f0562f95e614ef2418a526f77f7bb574ab8de","last_reissued_at":"2026-05-18T01:46:56.077834Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:46:56.077834Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gamma ray emission in Fermi bubbles and Higgs portal dark matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"Nobuchika Okada, Osamu Seto","submitted_at":"2013-10-22T17:20:13Z","abstract_excerpt":"It has been recently pointed out that the excess of the gamma ray spectrum in the Fermi Bubbles at low latitude can be well explained by the annihilation of dark matter particles. The best-fit candidate corresponds to the annihilation of a dark matter with mass of around $62$ GeV into $b \\bar{b}$ with the cross section, $\\sigma v \\simeq 3.3 \\times 10^{-26}$ cm$^3$/s, or the annihilation of a dark matter with mass of around $10$ GeV into a tau lepton pair with the cross section, $\\sigma v \\simeq 5.6 \\times 10^{-27}$ cm$^3$/s. We point out that the Higgs portal dark matter models are perfectly c"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1310.5991","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":""},"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":"1310.5991","created_at":"2026-05-18T01:46:56.077922+00:00"},{"alias_kind":"arxiv_version","alias_value":"1310.5991v2","created_at":"2026-05-18T01:46:56.077922+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1310.5991","created_at":"2026-05-18T01:46:56.077922+00:00"},{"alias_kind":"pith_short_12","alias_value":"7RWPNDWYPLEO","created_at":"2026-05-18T12:27:36.564083+00:00"},{"alias_kind":"pith_short_16","alias_value":"7RWPNDWYPLEOEVPW","created_at":"2026-05-18T12:27:36.564083+00:00"},{"alias_kind":"pith_short_8","alias_value":"7RWPNDWY","created_at":"2026-05-18T12:27:36.564083+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/7RWPNDWYPLEOEVPWEWKQ4XYFML","json":"https://pith.science/pith/7RWPNDWYPLEOEVPWEWKQ4XYFML.json","graph_json":"https://pith.science/api/pith-number/7RWPNDWYPLEOEVPWEWKQ4XYFML/graph.json","events_json":"https://pith.science/api/pith-number/7RWPNDWYPLEOEVPWEWKQ4XYFML/events.json","paper":"https://pith.science/paper/7RWPNDWY"},"agent_actions":{"view_html":"https://pith.science/pith/7RWPNDWYPLEOEVPWEWKQ4XYFML","download_json":"https://pith.science/pith/7RWPNDWYPLEOEVPWEWKQ4XYFML.json","view_paper":"https://pith.science/paper/7RWPNDWY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1310.5991&json=true","fetch_graph":"https://pith.science/api/pith-number/7RWPNDWYPLEOEVPWEWKQ4XYFML/graph.json","fetch_events":"https://pith.science/api/pith-number/7RWPNDWYPLEOEVPWEWKQ4XYFML/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7RWPNDWYPLEOEVPWEWKQ4XYFML/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7RWPNDWYPLEOEVPWEWKQ4XYFML/action/storage_attestation","attest_author":"https://pith.science/pith/7RWPNDWYPLEOEVPWEWKQ4XYFML/action/author_attestation","sign_citation":"https://pith.science/pith/7RWPNDWYPLEOEVPWEWKQ4XYFML/action/citation_signature","submit_replication":"https://pith.science/pith/7RWPNDWYPLEOEVPWEWKQ4XYFML/action/replication_record"}},"created_at":"2026-05-18T01:46:56.077922+00:00","updated_at":"2026-05-18T01:46:56.077922+00:00"}