{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:K2XYFN3IJ6HOFD7Z6O63C3EKZH","short_pith_number":"pith:K2XYFN3I","schema_version":"1.0","canonical_sha256":"56af82b7684f8ee28ff9f3bdb16c8ac9f31e3dc9f26278ad349b2d0d754ce20f","source":{"kind":"arxiv","id":"1501.04934","version":3},"attestation_state":"computed","paper":{"title":"Extragalactic star-forming galaxies with hypernovae and supernovae as high-energy neutrino and gamma-ray sources: the case of the 10 TeV neutrino data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Kohta Murase, Martin J. Rees, Nicholas Senno, Peter M\\'esz\\'aros, Philipp Baerwald","submitted_at":"2015-01-20T19:55:49Z","abstract_excerpt":"In light of the latest IceCube data, we discuss the implications of the cosmic ray energy input from hypernovae and supernovae into the Universe, and their propagation in the hosting galaxy and galaxy clusters or groups. The magnetic confinement in these environments may lead to efficient $pp$ collisions, resulting in a diffuse neutrino spectrum extending from PeV down to 10 TeV energies, with a spectrum and flux level compatible with that recently reported by IceCube. If the diffuse 10 TeV neutrino background largely comes from such the CR reservoirs, the corresponding diffuse gamma-ray backg"},"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":"1501.04934","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2015-01-20T19:55:49Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"d061e7994d59d6c83678c27c7fb0495ddc37adad5b2c7d9364e231cfcd612d8f","abstract_canon_sha256":"b2194aacc870dfd0ecb92e4a4383292d12055e0f54ca5d8f8f0291d4efc73a5e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:55:52.794547Z","signature_b64":"/4g5ni0N4V1DA3Bb+xNJEDQFfOMsicuy53fTOSy9RlWm4s8AQjh9IYIIk0CbY2o7uelpzGGfSmdF2ATYx4G8DA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"56af82b7684f8ee28ff9f3bdb16c8ac9f31e3dc9f26278ad349b2d0d754ce20f","last_reissued_at":"2026-05-18T01:55:52.794175Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:55:52.794175Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Extragalactic star-forming galaxies with hypernovae and supernovae as high-energy neutrino and gamma-ray sources: the case of the 10 TeV neutrino data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Kohta Murase, Martin J. Rees, Nicholas Senno, Peter M\\'esz\\'aros, Philipp Baerwald","submitted_at":"2015-01-20T19:55:49Z","abstract_excerpt":"In light of the latest IceCube data, we discuss the implications of the cosmic ray energy input from hypernovae and supernovae into the Universe, and their propagation in the hosting galaxy and galaxy clusters or groups. The magnetic confinement in these environments may lead to efficient $pp$ collisions, resulting in a diffuse neutrino spectrum extending from PeV down to 10 TeV energies, with a spectrum and flux level compatible with that recently reported by IceCube. If the diffuse 10 TeV neutrino background largely comes from such the CR reservoirs, the corresponding diffuse gamma-ray backg"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1501.04934","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":""},"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":"1501.04934","created_at":"2026-05-18T01:55:52.794230+00:00"},{"alias_kind":"arxiv_version","alias_value":"1501.04934v3","created_at":"2026-05-18T01:55:52.794230+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1501.04934","created_at":"2026-05-18T01:55:52.794230+00:00"},{"alias_kind":"pith_short_12","alias_value":"K2XYFN3IJ6HO","created_at":"2026-05-18T12:29:27.538025+00:00"},{"alias_kind":"pith_short_16","alias_value":"K2XYFN3IJ6HOFD7Z","created_at":"2026-05-18T12:29:27.538025+00:00"},{"alias_kind":"pith_short_8","alias_value":"K2XYFN3I","created_at":"2026-05-18T12:29:27.538025+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/K2XYFN3IJ6HOFD7Z6O63C3EKZH","json":"https://pith.science/pith/K2XYFN3IJ6HOFD7Z6O63C3EKZH.json","graph_json":"https://pith.science/api/pith-number/K2XYFN3IJ6HOFD7Z6O63C3EKZH/graph.json","events_json":"https://pith.science/api/pith-number/K2XYFN3IJ6HOFD7Z6O63C3EKZH/events.json","paper":"https://pith.science/paper/K2XYFN3I"},"agent_actions":{"view_html":"https://pith.science/pith/K2XYFN3IJ6HOFD7Z6O63C3EKZH","download_json":"https://pith.science/pith/K2XYFN3IJ6HOFD7Z6O63C3EKZH.json","view_paper":"https://pith.science/paper/K2XYFN3I","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1501.04934&json=true","fetch_graph":"https://pith.science/api/pith-number/K2XYFN3IJ6HOFD7Z6O63C3EKZH/graph.json","fetch_events":"https://pith.science/api/pith-number/K2XYFN3IJ6HOFD7Z6O63C3EKZH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/K2XYFN3IJ6HOFD7Z6O63C3EKZH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/K2XYFN3IJ6HOFD7Z6O63C3EKZH/action/storage_attestation","attest_author":"https://pith.science/pith/K2XYFN3IJ6HOFD7Z6O63C3EKZH/action/author_attestation","sign_citation":"https://pith.science/pith/K2XYFN3IJ6HOFD7Z6O63C3EKZH/action/citation_signature","submit_replication":"https://pith.science/pith/K2XYFN3IJ6HOFD7Z6O63C3EKZH/action/replication_record"}},"created_at":"2026-05-18T01:55:52.794230+00:00","updated_at":"2026-05-18T01:55:52.794230+00:00"}