{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2015:WUDDHLBSMQHYS5GJDFVFENO7L2","short_pith_number":"pith:WUDDHLBS","canonical_record":{"source":{"id":"1507.07987","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2015-07-28T23:42:35Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"e1b7ea6d258a7e45dfebcf12d740367b84388d382283dbd9c4adc75743067fcc","abstract_canon_sha256":"c94a3320d8bc5ee0e9e9fc31a72faf0343d9d955fc7287ff13a8c03ccd9f2bab"},"schema_version":"1.0"},"canonical_sha256":"b50633ac32640f8974c9196a5235df5ea484ece8406d8efda956f909acd68b17","source":{"kind":"arxiv","id":"1507.07987","version":4},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1507.07987","created_at":"2026-05-18T01:24:10Z"},{"alias_kind":"arxiv_version","alias_value":"1507.07987v4","created_at":"2026-05-18T01:24:10Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1507.07987","created_at":"2026-05-18T01:24:10Z"},{"alias_kind":"pith_short_12","alias_value":"WUDDHLBSMQHY","created_at":"2026-05-18T12:29:47Z"},{"alias_kind":"pith_short_16","alias_value":"WUDDHLBSMQHYS5GJ","created_at":"2026-05-18T12:29:47Z"},{"alias_kind":"pith_short_8","alias_value":"WUDDHLBS","created_at":"2026-05-18T12:29:47Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2015:WUDDHLBSMQHYS5GJDFVFENO7L2","target":"record","payload":{"canonical_record":{"source":{"id":"1507.07987","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2015-07-28T23:42:35Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"e1b7ea6d258a7e45dfebcf12d740367b84388d382283dbd9c4adc75743067fcc","abstract_canon_sha256":"c94a3320d8bc5ee0e9e9fc31a72faf0343d9d955fc7287ff13a8c03ccd9f2bab"},"schema_version":"1.0"},"canonical_sha256":"b50633ac32640f8974c9196a5235df5ea484ece8406d8efda956f909acd68b17","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:24:10.657778Z","signature_b64":"TUz+nkHowKy+JoXITgKliUDRJShHgwse2yeaYsD5t6GN3o9NGn/XfKg0iMJaj3pwIzxq8aexRUNNgLJ38kM4DA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b50633ac32640f8974c9196a5235df5ea484ece8406d8efda956f909acd68b17","last_reissued_at":"2026-05-18T01:24:10.657311Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:24:10.657311Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1507.07987","source_version":4,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T01:24:10Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"r03cSvJYeTS25CGOxhaw3YzBqNtEQW1g2XL0vWiQ0lNKYudqj7c91VIw0uFypW+L1HDiSltDf3b7pogBIByuBw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-30T04:17:20.548893Z"},"content_sha256":"9b1c582ca88c27750a3f418cd840c699c170374be2b63594cab68e3a3edc3ae9","schema_version":"1.0","event_id":"sha256:9b1c582ca88c27750a3f418cd840c699c170374be2b63594cab68e3a3edc3ae9"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2015:WUDDHLBSMQHYS5GJDFVFENO7L2","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Limits on dark matter proton scattering from neutrino telescopes using micrOMEGAs","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"A. Pukhov, G. Belanger, J. Da Silva, T. Perrillat-Bottonet","submitted_at":"2015-07-28T23:42:35Z","abstract_excerpt":"Limits on dark matter spin dependent elastic scattering cross section on protons derived from IceCube data are obtained for different dark matter annihilation channels using micrOMEGAs. The uncertainty on the derived limits, estimated by using different neutrino spectra, can reach a factor two. For all dark matter annihilation channels except for quarks, the limits on the spin dependent cross section are more stringent than those obtained in direct detection experiments. The new functions that allow to derive those limits are described."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1507.07987","kind":"arxiv","version":4},"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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T01:24:10Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"d6PhylXu1QH70obJc8BWapnWySHcNaAv8vQ3N7LdhuTR6Xz8M7NxPfHb11/UGgz7dvVpKiwB2pL+2dtnTkZFBg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-30T04:17:20.549244Z"},"content_sha256":"763d1fd1b92a775a6657aab50f7279f219951394800422823a5dcde2ab3cc634","schema_version":"1.0","event_id":"sha256:763d1fd1b92a775a6657aab50f7279f219951394800422823a5dcde2ab3cc634"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/WUDDHLBSMQHYS5GJDFVFENO7L2/bundle.json","state_url":"https://pith.science/pith/WUDDHLBSMQHYS5GJDFVFENO7L2/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/WUDDHLBSMQHYS5GJDFVFENO7L2/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-05-30T04:17:20Z","links":{"resolver":"https://pith.science/pith/WUDDHLBSMQHYS5GJDFVFENO7L2","bundle":"https://pith.science/pith/WUDDHLBSMQHYS5GJDFVFENO7L2/bundle.json","state":"https://pith.science/pith/WUDDHLBSMQHYS5GJDFVFENO7L2/state.json","well_known_bundle":"https://pith.science/.well-known/pith/WUDDHLBSMQHYS5GJDFVFENO7L2/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2015:WUDDHLBSMQHYS5GJDFVFENO7L2","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"c94a3320d8bc5ee0e9e9fc31a72faf0343d9d955fc7287ff13a8c03ccd9f2bab","cross_cats_sorted":["astro-ph.HE"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2015-07-28T23:42:35Z","title_canon_sha256":"e1b7ea6d258a7e45dfebcf12d740367b84388d382283dbd9c4adc75743067fcc"},"schema_version":"1.0","source":{"id":"1507.07987","kind":"arxiv","version":4}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1507.07987","created_at":"2026-05-18T01:24:10Z"},{"alias_kind":"arxiv_version","alias_value":"1507.07987v4","created_at":"2026-05-18T01:24:10Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1507.07987","created_at":"2026-05-18T01:24:10Z"},{"alias_kind":"pith_short_12","alias_value":"WUDDHLBSMQHY","created_at":"2026-05-18T12:29:47Z"},{"alias_kind":"pith_short_16","alias_value":"WUDDHLBSMQHYS5GJ","created_at":"2026-05-18T12:29:47Z"},{"alias_kind":"pith_short_8","alias_value":"WUDDHLBS","created_at":"2026-05-18T12:29:47Z"}],"graph_snapshots":[{"event_id":"sha256:763d1fd1b92a775a6657aab50f7279f219951394800422823a5dcde2ab3cc634","target":"graph","created_at":"2026-05-18T01:24:10Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"Limits on dark matter spin dependent elastic scattering cross section on protons derived from IceCube data are obtained for different dark matter annihilation channels using micrOMEGAs. The uncertainty on the derived limits, estimated by using different neutrino spectra, can reach a factor two. For all dark matter annihilation channels except for quarks, the limits on the spin dependent cross section are more stringent than those obtained in direct detection experiments. The new functions that allow to derive those limits are described.","authors_text":"A. Pukhov, G. Belanger, J. Da Silva, T. Perrillat-Bottonet","cross_cats":["astro-ph.HE"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2015-07-28T23:42:35Z","title":"Limits on dark matter proton scattering from neutrino telescopes using micrOMEGAs"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1507.07987","kind":"arxiv","version":4},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:9b1c582ca88c27750a3f418cd840c699c170374be2b63594cab68e3a3edc3ae9","target":"record","created_at":"2026-05-18T01:24:10Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"c94a3320d8bc5ee0e9e9fc31a72faf0343d9d955fc7287ff13a8c03ccd9f2bab","cross_cats_sorted":["astro-ph.HE"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2015-07-28T23:42:35Z","title_canon_sha256":"e1b7ea6d258a7e45dfebcf12d740367b84388d382283dbd9c4adc75743067fcc"},"schema_version":"1.0","source":{"id":"1507.07987","kind":"arxiv","version":4}},"canonical_sha256":"b50633ac32640f8974c9196a5235df5ea484ece8406d8efda956f909acd68b17","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"b50633ac32640f8974c9196a5235df5ea484ece8406d8efda956f909acd68b17","first_computed_at":"2026-05-18T01:24:10.657311Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:24:10.657311Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"TUz+nkHowKy+JoXITgKliUDRJShHgwse2yeaYsD5t6GN3o9NGn/XfKg0iMJaj3pwIzxq8aexRUNNgLJ38kM4DA==","signature_status":"signed_v1","signed_at":"2026-05-18T01:24:10.657778Z","signed_message":"canonical_sha256_bytes"},"source_id":"1507.07987","source_kind":"arxiv","source_version":4}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:9b1c582ca88c27750a3f418cd840c699c170374be2b63594cab68e3a3edc3ae9","sha256:763d1fd1b92a775a6657aab50f7279f219951394800422823a5dcde2ab3cc634"],"state_sha256":"fd73b9f3d548f979836c50e2ae1aa5a5191597464d43ed0d1504a25d35c3ec63"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"uphrch6xYI2lazMy7iFRXMbDfsyjEpiQc1+HeTpnKyPzk0KEb/1a2VNvr4px+dmEOt4KMDIvVHGDY77wa1G4Cg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-30T04:17:20.551474Z","bundle_sha256":"11d123a22a3592d3a4bd805c3a1e6a4687f3aabd37f5fb8bca90126243cdc403"}}