{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2017:ZTR4NQVOJRIDNTRRD2FSF4Y75O","short_pith_number":"pith:ZTR4NQVO","canonical_record":{"source":{"id":"1711.11085","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2017-11-29T20:03:07Z","cross_cats_sorted":[],"title_canon_sha256":"069aa025e60a68408c12ff7eff9d04f80204ad9e59f1b2a6df959973c8a96c41","abstract_canon_sha256":"139bcbe07f9e799971dc3333fca0cdc412f2746f206a03f4face72a66f01e07e"},"schema_version":"1.0"},"canonical_sha256":"cce3c6c2ae4c5036ce311e8b22f31feb9360d5cf7082c93e19519fa6f570c6d1","source":{"kind":"arxiv","id":"1711.11085","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1711.11085","created_at":"2026-05-17T23:58:05Z"},{"alias_kind":"arxiv_version","alias_value":"1711.11085v1","created_at":"2026-05-17T23:58:05Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1711.11085","created_at":"2026-05-17T23:58:05Z"},{"alias_kind":"pith_short_12","alias_value":"ZTR4NQVOJRID","created_at":"2026-05-18T12:31:59Z"},{"alias_kind":"pith_short_16","alias_value":"ZTR4NQVOJRIDNTRR","created_at":"2026-05-18T12:31:59Z"},{"alias_kind":"pith_short_8","alias_value":"ZTR4NQVO","created_at":"2026-05-18T12:31:59Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2017:ZTR4NQVOJRIDNTRRD2FSF4Y75O","target":"record","payload":{"canonical_record":{"source":{"id":"1711.11085","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2017-11-29T20:03:07Z","cross_cats_sorted":[],"title_canon_sha256":"069aa025e60a68408c12ff7eff9d04f80204ad9e59f1b2a6df959973c8a96c41","abstract_canon_sha256":"139bcbe07f9e799971dc3333fca0cdc412f2746f206a03f4face72a66f01e07e"},"schema_version":"1.0"},"canonical_sha256":"cce3c6c2ae4c5036ce311e8b22f31feb9360d5cf7082c93e19519fa6f570c6d1","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:58:05.312183Z","signature_b64":"AkY0RD2iw5noiv7SAZq9XfL7L2UyUnpqjBBoXnCtK2sjS5Do8+JIst4jvo6nLSXdFTbmf4MoSf4qf+Pa1+fCDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cce3c6c2ae4c5036ce311e8b22f31feb9360d5cf7082c93e19519fa6f570c6d1","last_reissued_at":"2026-05-17T23:58:05.311825Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:58:05.311825Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1711.11085","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-17T23:58:05Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"AGZvTgIcI2U5/GxyLi5hefPtqGtbwM/02EVK80+k7GAAgp206MpM8IoghungoomiZ8IvAVpzzbCjQfDwROaWAw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-01T17:15:18.059619Z"},"content_sha256":"29409cd6b90139a5b609042fcdeb865dd1db1f1382c0d793088a632d74c780fe","schema_version":"1.0","event_id":"sha256:29409cd6b90139a5b609042fcdeb865dd1db1f1382c0d793088a632d74c780fe"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2017:ZTR4NQVOJRIDNTRRD2FSF4Y75O","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Dark matter halos in the multicomponent model. II. Density profiles of galactic halos","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Keita Todoroki, Mikhail V. Medvedev","submitted_at":"2017-11-29T20:03:07Z","abstract_excerpt":"The multicomponent dark matter model with self-scattering and inter-conversions of species into one another is an alternative dark matter paradigm that is capable of resolving the long-standing problems of $\\Lambda$CDM cosmology at small scales. In this paper, we have studied in detail the properties of dark matter halos with $M \\sim 4-5 \\times10^{11} M_{\\odot}$ obtained in $N$-body cosmological simulations with the simplest two-component (2cDM) model. A large set of velocity-dependent cross-section prescriptions for elastic scattering and mass conversions, $\\sigma_s(v)\\propto v^{a_s}$ and $\\s"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.11085","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":""},"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":"2026-05-17T23:58:05Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"dlSXlvTvsbyStasPJFsox2JDa9dbINuSTdTcPuj7pqf4CjRRwRjVQc1mlH2z0dumBTeh9NzS2Jddyses5Xv2Aw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-01T17:15:18.059965Z"},"content_sha256":"c043faf25f3e97341db4d00a3bb5a727910e4508d1a394198c9889c4717cc47d","schema_version":"1.0","event_id":"sha256:c043faf25f3e97341db4d00a3bb5a727910e4508d1a394198c9889c4717cc47d"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/ZTR4NQVOJRIDNTRRD2FSF4Y75O/bundle.json","state_url":"https://pith.science/pith/ZTR4NQVOJRIDNTRRD2FSF4Y75O/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/ZTR4NQVOJRIDNTRRD2FSF4Y75O/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":"2026-06-01T17:15:18Z","links":{"resolver":"https://pith.science/pith/ZTR4NQVOJRIDNTRRD2FSF4Y75O","bundle":"https://pith.science/pith/ZTR4NQVOJRIDNTRRD2FSF4Y75O/bundle.json","state":"https://pith.science/pith/ZTR4NQVOJRIDNTRRD2FSF4Y75O/state.json","well_known_bundle":"https://pith.science/.well-known/pith/ZTR4NQVOJRIDNTRRD2FSF4Y75O/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2017:ZTR4NQVOJRIDNTRRD2FSF4Y75O","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":"139bcbe07f9e799971dc3333fca0cdc412f2746f206a03f4face72a66f01e07e","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2017-11-29T20:03:07Z","title_canon_sha256":"069aa025e60a68408c12ff7eff9d04f80204ad9e59f1b2a6df959973c8a96c41"},"schema_version":"1.0","source":{"id":"1711.11085","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1711.11085","created_at":"2026-05-17T23:58:05Z"},{"alias_kind":"arxiv_version","alias_value":"1711.11085v1","created_at":"2026-05-17T23:58:05Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1711.11085","created_at":"2026-05-17T23:58:05Z"},{"alias_kind":"pith_short_12","alias_value":"ZTR4NQVOJRID","created_at":"2026-05-18T12:31:59Z"},{"alias_kind":"pith_short_16","alias_value":"ZTR4NQVOJRIDNTRR","created_at":"2026-05-18T12:31:59Z"},{"alias_kind":"pith_short_8","alias_value":"ZTR4NQVO","created_at":"2026-05-18T12:31:59Z"}],"graph_snapshots":[{"event_id":"sha256:c043faf25f3e97341db4d00a3bb5a727910e4508d1a394198c9889c4717cc47d","target":"graph","created_at":"2026-05-17T23:58:05Z","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":"The multicomponent dark matter model with self-scattering and inter-conversions of species into one another is an alternative dark matter paradigm that is capable of resolving the long-standing problems of $\\Lambda$CDM cosmology at small scales. In this paper, we have studied in detail the properties of dark matter halos with $M \\sim 4-5 \\times10^{11} M_{\\odot}$ obtained in $N$-body cosmological simulations with the simplest two-component (2cDM) model. A large set of velocity-dependent cross-section prescriptions for elastic scattering and mass conversions, $\\sigma_s(v)\\propto v^{a_s}$ and $\\s","authors_text":"Keita Todoroki, Mikhail V. Medvedev","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2017-11-29T20:03:07Z","title":"Dark matter halos in the multicomponent model. II. Density profiles of galactic halos"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.11085","kind":"arxiv","version":1},"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":"sha256:29409cd6b90139a5b609042fcdeb865dd1db1f1382c0d793088a632d74c780fe","target":"record","created_at":"2026-05-17T23:58:05Z","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":"139bcbe07f9e799971dc3333fca0cdc412f2746f206a03f4face72a66f01e07e","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2017-11-29T20:03:07Z","title_canon_sha256":"069aa025e60a68408c12ff7eff9d04f80204ad9e59f1b2a6df959973c8a96c41"},"schema_version":"1.0","source":{"id":"1711.11085","kind":"arxiv","version":1}},"canonical_sha256":"cce3c6c2ae4c5036ce311e8b22f31feb9360d5cf7082c93e19519fa6f570c6d1","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"cce3c6c2ae4c5036ce311e8b22f31feb9360d5cf7082c93e19519fa6f570c6d1","first_computed_at":"2026-05-17T23:58:05.311825Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-17T23:58:05.311825Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"AkY0RD2iw5noiv7SAZq9XfL7L2UyUnpqjBBoXnCtK2sjS5Do8+JIst4jvo6nLSXdFTbmf4MoSf4qf+Pa1+fCDw==","signature_status":"signed_v1","signed_at":"2026-05-17T23:58:05.312183Z","signed_message":"canonical_sha256_bytes"},"source_id":"1711.11085","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:29409cd6b90139a5b609042fcdeb865dd1db1f1382c0d793088a632d74c780fe","sha256:c043faf25f3e97341db4d00a3bb5a727910e4508d1a394198c9889c4717cc47d"],"state_sha256":"1c8752f3baa84154915975b2e7c617e72f465ee01ba5fb9f0a8361b947a5febb"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"N+Tm+Mwb/ds3RuFfOBQ+u4xvXRIJySjAmMVWWD1CbaMLHSkZcGz9UIo5OTsnzooaYHyWzUaoWRAx4RhNmWrVDg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-01T17:15:18.061853Z","bundle_sha256":"0052720fe43723a0a8d8a9a64291c922980f118d040e60060d6bc9926ed268ef"}}