{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:A7O57KVYNMGS35KHZAPB4MOCZ6","short_pith_number":"pith:A7O57KVY","schema_version":"1.0","canonical_sha256":"07dddfaab86b0d2df547c81e1e31c2cfa7083f117cdb8d4805eeaa6c1b96b3f2","source":{"kind":"arxiv","id":"1801.01871","version":1},"attestation_state":"computed","paper":{"title":"Exotic energy injection with ExoCLASS: Application to the Higgs portal model and evaporating black holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Julien Lesgourgues, Michael Kr\\\"amer, Patrick St\\\"ocker, Vivian Poulin","submitted_at":"2018-01-05T18:51:27Z","abstract_excerpt":"We devise a new user-friendly tool interfaced with the Boltzmann code CLASS to deal with any kind of exotic electromagnetic energy injection in the universe and its impact on anisotropies of the Cosmic Microwave Background. It makes use of the results from standard electromagnetic cascade calculations develop in the context of WIMP annihilation, generalized to incorporate any injection history. We first validate it on a specific WIMP scenario, the Higgs Portal model, confirming that the standard effective on-the-spot treatment is accurate enough. We then analyze the more involved example of ev"},"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":"1801.01871","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2018-01-05T18:51:27Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"0b271eb02ed6af637ca7a79fa4b51bc80943dd260607dc5b5f61d87ba7d1700a","abstract_canon_sha256":"73fe48bd47432a7f974fc0ff044addf406c7110450ee5c204eb59852c1f8529c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:20:04.861906Z","signature_b64":"81DYhpPnmKindGgJv1nM8PF/e44y8G9SXYx+1W7Rq7KnmrqlbiMAqmO2ktLIPw5cuxCwFyoRgm4otxQjdYO4DQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"07dddfaab86b0d2df547c81e1e31c2cfa7083f117cdb8d4805eeaa6c1b96b3f2","last_reissued_at":"2026-05-18T00:20:04.861226Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:20:04.861226Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Exotic energy injection with ExoCLASS: Application to the Higgs portal model and evaporating black holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Julien Lesgourgues, Michael Kr\\\"amer, Patrick St\\\"ocker, Vivian Poulin","submitted_at":"2018-01-05T18:51:27Z","abstract_excerpt":"We devise a new user-friendly tool interfaced with the Boltzmann code CLASS to deal with any kind of exotic electromagnetic energy injection in the universe and its impact on anisotropies of the Cosmic Microwave Background. It makes use of the results from standard electromagnetic cascade calculations develop in the context of WIMP annihilation, generalized to incorporate any injection history. We first validate it on a specific WIMP scenario, the Higgs Portal model, confirming that the standard effective on-the-spot treatment is accurate enough. We then analyze the more involved example of ev"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1801.01871","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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1801.01871","created_at":"2026-05-18T00:20:04.861312+00:00"},{"alias_kind":"arxiv_version","alias_value":"1801.01871v1","created_at":"2026-05-18T00:20:04.861312+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1801.01871","created_at":"2026-05-18T00:20:04.861312+00:00"},{"alias_kind":"pith_short_12","alias_value":"A7O57KVYNMGS","created_at":"2026-05-18T12:32:13.499390+00:00"},{"alias_kind":"pith_short_16","alias_value":"A7O57KVYNMGS35KH","created_at":"2026-05-18T12:32:13.499390+00:00"},{"alias_kind":"pith_short_8","alias_value":"A7O57KVY","created_at":"2026-05-18T12:32:13.499390+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":6,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2605.15197","citing_title":"Primordial Black Hole from Tensor-induced Density Fluctuation: First-order Phase Transitions and Domain Walls","ref_index":217,"is_internal_anchor":true},{"citing_arxiv_id":"2002.12778","citing_title":"Constraints on Primordial Black Holes","ref_index":188,"is_internal_anchor":true},{"citing_arxiv_id":"2604.19198","citing_title":"Cosmological constraints on TeV-scale dark matter subcomponents decaying between recombination and reionisation","ref_index":54,"is_internal_anchor":false},{"citing_arxiv_id":"2604.18007","citing_title":"In-depth analysis of the clustering of dark matter particles around primordial black holes. Part III: CMB constraints","ref_index":61,"is_internal_anchor":false},{"citing_arxiv_id":"2604.06858","citing_title":"Memory-Burden Suppression of Hawking Radiation and Neutrino Constraints on Primordial Black Holes","ref_index":61,"is_internal_anchor":false},{"citing_arxiv_id":"2605.08080","citing_title":"CMB Limits on the Absorption of Light Vector and Axial-Vector Dark Matter","ref_index":78,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/A7O57KVYNMGS35KHZAPB4MOCZ6","json":"https://pith.science/pith/A7O57KVYNMGS35KHZAPB4MOCZ6.json","graph_json":"https://pith.science/api/pith-number/A7O57KVYNMGS35KHZAPB4MOCZ6/graph.json","events_json":"https://pith.science/api/pith-number/A7O57KVYNMGS35KHZAPB4MOCZ6/events.json","paper":"https://pith.science/paper/A7O57KVY"},"agent_actions":{"view_html":"https://pith.science/pith/A7O57KVYNMGS35KHZAPB4MOCZ6","download_json":"https://pith.science/pith/A7O57KVYNMGS35KHZAPB4MOCZ6.json","view_paper":"https://pith.science/paper/A7O57KVY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1801.01871&json=true","fetch_graph":"https://pith.science/api/pith-number/A7O57KVYNMGS35KHZAPB4MOCZ6/graph.json","fetch_events":"https://pith.science/api/pith-number/A7O57KVYNMGS35KHZAPB4MOCZ6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/A7O57KVYNMGS35KHZAPB4MOCZ6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/A7O57KVYNMGS35KHZAPB4MOCZ6/action/storage_attestation","attest_author":"https://pith.science/pith/A7O57KVYNMGS35KHZAPB4MOCZ6/action/author_attestation","sign_citation":"https://pith.science/pith/A7O57KVYNMGS35KHZAPB4MOCZ6/action/citation_signature","submit_replication":"https://pith.science/pith/A7O57KVYNMGS35KHZAPB4MOCZ6/action/replication_record"}},"created_at":"2026-05-18T00:20:04.861312+00:00","updated_at":"2026-05-18T00:20:04.861312+00:00"}