{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2014:76XMASXZJBE7E5CCHZRYMYDHZ7","short_pith_number":"pith:76XMASXZ","canonical_record":{"source":{"id":"1401.6510","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-01-25T09:26:40Z","cross_cats_sorted":[],"title_canon_sha256":"de79d91c506f8936e907c2c99de738f9e2f14c105ea2b55b705ad8d4d046b4b6","abstract_canon_sha256":"93e9f89278d67cabc7b1d7e7a6a17d07b5bb0dd5437089027b7d74b2408acb62"},"schema_version":"1.0"},"canonical_sha256":"ffaec04af94849f274423e63866067cfc1fb608933c5a73cd0c97ed4ba2e6ec4","source":{"kind":"arxiv","id":"1401.6510","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1401.6510","created_at":"2026-05-18T03:00:25Z"},{"alias_kind":"arxiv_version","alias_value":"1401.6510v2","created_at":"2026-05-18T03:00:25Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1401.6510","created_at":"2026-05-18T03:00:25Z"},{"alias_kind":"pith_short_12","alias_value":"76XMASXZJBE7","created_at":"2026-05-18T12:28:16Z"},{"alias_kind":"pith_short_16","alias_value":"76XMASXZJBE7E5CC","created_at":"2026-05-18T12:28:16Z"},{"alias_kind":"pith_short_8","alias_value":"76XMASXZ","created_at":"2026-05-18T12:28:16Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2014:76XMASXZJBE7E5CCHZRYMYDHZ7","target":"record","payload":{"canonical_record":{"source":{"id":"1401.6510","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-01-25T09:26:40Z","cross_cats_sorted":[],"title_canon_sha256":"de79d91c506f8936e907c2c99de738f9e2f14c105ea2b55b705ad8d4d046b4b6","abstract_canon_sha256":"93e9f89278d67cabc7b1d7e7a6a17d07b5bb0dd5437089027b7d74b2408acb62"},"schema_version":"1.0"},"canonical_sha256":"ffaec04af94849f274423e63866067cfc1fb608933c5a73cd0c97ed4ba2e6ec4","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:00:25.208637Z","signature_b64":"Onjyo0sphIA6y8rOtwsnuo+g4oiXyTUkoTX+YHK9pCIPqp5XKmuh/hyWdHIdb1lFotFReuG1tlapce1Dp4a+Ag==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ffaec04af94849f274423e63866067cfc1fb608933c5a73cd0c97ed4ba2e6ec4","last_reissued_at":"2026-05-18T03:00:25.208023Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:00:25.208023Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1401.6510","source_version":2,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T03:00:25Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"nbsXTKs1Ht7d61J91GerW/8c98wMZirBD6WRbK3pKZwCykWjy8QG8YioWMIaFFj0U5II/9GtOYKv3w2KldwLDA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-01T21:20:37.799715Z"},"content_sha256":"3c238e9c060163910fea028ae52a23fa3baacf9297f68364f83233191166e997","schema_version":"1.0","event_id":"sha256:3c238e9c060163910fea028ae52a23fa3baacf9297f68364f83233191166e997"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2014:76XMASXZJBE7E5CCHZRYMYDHZ7","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Asymmetric Velocity Distributions from Halo Density Profiles in the Eddington Approach","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Greece), J. D. Vergados (TEI of Western Macedonia, Kozani","submitted_at":"2014-01-25T09:26:40Z","abstract_excerpt":"In the present paper we show how obtain the energy distribution f(E) in our vicinity starting from WIMP density profiles in a self consistent way by employing the Eddington approach and adding reasonable angular momentum dependent terms in the expression of the energy. We then show how we can obtain the velocity dispersion and the asymmetry parameter {\\beta} in terms of the parameters describing the angular momentum dependence. From this expression for f(E) we proceed to construct an axially symmetric WIMP velocity distributions, which for a gravitationally bound system automatically has an ve"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1401.6510","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T03:00:25Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"T3a6mt/+0b39xBmTTDyf4PzlKOK7R44fCgdsz0JRKXcgITBQaVunudzF0wGkiYtbjcHTxv6gSimkh8a9+ATxAg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-01T21:20:37.800069Z"},"content_sha256":"bd3fd0bf7769216d6194349b4ddb2800ff98280ebfa78409f658593bdeee0af1","schema_version":"1.0","event_id":"sha256:bd3fd0bf7769216d6194349b4ddb2800ff98280ebfa78409f658593bdeee0af1"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/76XMASXZJBE7E5CCHZRYMYDHZ7/bundle.json","state_url":"https://pith.science/pith/76XMASXZJBE7E5CCHZRYMYDHZ7/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/76XMASXZJBE7E5CCHZRYMYDHZ7/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":"2026-06-01T21:20:37Z","links":{"resolver":"https://pith.science/pith/76XMASXZJBE7E5CCHZRYMYDHZ7","bundle":"https://pith.science/pith/76XMASXZJBE7E5CCHZRYMYDHZ7/bundle.json","state":"https://pith.science/pith/76XMASXZJBE7E5CCHZRYMYDHZ7/state.json","well_known_bundle":"https://pith.science/.well-known/pith/76XMASXZJBE7E5CCHZRYMYDHZ7/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2014:76XMASXZJBE7E5CCHZRYMYDHZ7","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":"93e9f89278d67cabc7b1d7e7a6a17d07b5bb0dd5437089027b7d74b2408acb62","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-01-25T09:26:40Z","title_canon_sha256":"de79d91c506f8936e907c2c99de738f9e2f14c105ea2b55b705ad8d4d046b4b6"},"schema_version":"1.0","source":{"id":"1401.6510","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1401.6510","created_at":"2026-05-18T03:00:25Z"},{"alias_kind":"arxiv_version","alias_value":"1401.6510v2","created_at":"2026-05-18T03:00:25Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1401.6510","created_at":"2026-05-18T03:00:25Z"},{"alias_kind":"pith_short_12","alias_value":"76XMASXZJBE7","created_at":"2026-05-18T12:28:16Z"},{"alias_kind":"pith_short_16","alias_value":"76XMASXZJBE7E5CC","created_at":"2026-05-18T12:28:16Z"},{"alias_kind":"pith_short_8","alias_value":"76XMASXZ","created_at":"2026-05-18T12:28:16Z"}],"graph_snapshots":[{"event_id":"sha256:bd3fd0bf7769216d6194349b4ddb2800ff98280ebfa78409f658593bdeee0af1","target":"graph","created_at":"2026-05-18T03:00:25Z","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":"In the present paper we show how obtain the energy distribution f(E) in our vicinity starting from WIMP density profiles in a self consistent way by employing the Eddington approach and adding reasonable angular momentum dependent terms in the expression of the energy. We then show how we can obtain the velocity dispersion and the asymmetry parameter {\\beta} in terms of the parameters describing the angular momentum dependence. From this expression for f(E) we proceed to construct an axially symmetric WIMP velocity distributions, which for a gravitationally bound system automatically has an ve","authors_text":"Greece), J. D. Vergados (TEI of Western Macedonia, Kozani","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-01-25T09:26:40Z","title":"Asymmetric Velocity Distributions from Halo Density Profiles in the Eddington Approach"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1401.6510","kind":"arxiv","version":2},"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":"sha256:3c238e9c060163910fea028ae52a23fa3baacf9297f68364f83233191166e997","target":"record","created_at":"2026-05-18T03:00:25Z","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":"93e9f89278d67cabc7b1d7e7a6a17d07b5bb0dd5437089027b7d74b2408acb62","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-01-25T09:26:40Z","title_canon_sha256":"de79d91c506f8936e907c2c99de738f9e2f14c105ea2b55b705ad8d4d046b4b6"},"schema_version":"1.0","source":{"id":"1401.6510","kind":"arxiv","version":2}},"canonical_sha256":"ffaec04af94849f274423e63866067cfc1fb608933c5a73cd0c97ed4ba2e6ec4","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"ffaec04af94849f274423e63866067cfc1fb608933c5a73cd0c97ed4ba2e6ec4","first_computed_at":"2026-05-18T03:00:25.208023Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T03:00:25.208023Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"Onjyo0sphIA6y8rOtwsnuo+g4oiXyTUkoTX+YHK9pCIPqp5XKmuh/hyWdHIdb1lFotFReuG1tlapce1Dp4a+Ag==","signature_status":"signed_v1","signed_at":"2026-05-18T03:00:25.208637Z","signed_message":"canonical_sha256_bytes"},"source_id":"1401.6510","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:3c238e9c060163910fea028ae52a23fa3baacf9297f68364f83233191166e997","sha256:bd3fd0bf7769216d6194349b4ddb2800ff98280ebfa78409f658593bdeee0af1"],"state_sha256":"55e15ad775c93eb86dd80df533c11fa2cbb6cbdcd4cf94a3af443c646a0f17a4"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"IACU9zaCAPZVykeIKg/CDN64vz8g8rs0U/x7sPbrawwTa0X87RbzAds3jAYyKSOgEE7lB/dTZWSwcFC5516uAQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-01T21:20:37.802073Z","bundle_sha256":"3da3b24202dab57e45aeb78dc24e7da75a7dc59539c0a2d8f86fae01bf83ce96"}}