{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2008:VFED4US2HL2NBCB566V6KLOBTO","short_pith_number":"pith:VFED4US2","schema_version":"1.0","canonical_sha256":"a9483e525a3af4d0883df7abe52dc19b8873a71c8d7c1f2b86e8c666a944c866","source":{"kind":"arxiv","id":"0806.1191","version":2},"attestation_state":"computed","paper":{"title":"Composite dark matter from a model with composite Higgs boson","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Chris Kouvaris, Maxim Yu. Khlopov","submitted_at":"2008-06-06T15:37:41Z","abstract_excerpt":"In a previous paper \\cite{Khlopov:2007ic}, we showed how the minimal walking technicolor model (WTC) can provide a composite dark matter candidate, by forming bound states between a -2 electrically charged techniparticle and a $^4He^{++}$. We studied the properties of these \\emph{techni-O-helium} $tOHe$ \"atoms\", which behave as warmer dark matter rather than cold. In this paper we extend our work on several different aspects. We study the possibility of a mixed scenario where both $tOHe$ and bound states between +2 and -2 electrically charged techniparticles coexist in the dark matter density."},"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":"0806.1191","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph","submitted_at":"2008-06-06T15:37:41Z","cross_cats_sorted":[],"title_canon_sha256":"740fa2d47c2a42167a8faea67343cb59a9198af95385473e4b7a0d2007849a1b","abstract_canon_sha256":"81737a4f8f460e7af042f425dc37a4f4b165134e0c95dbdc777537b9f25aadff"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:30:14.204753Z","signature_b64":"H/xEN3ApIZ2aph2a5obZUexn5zKpnicY890vN/yUjf6QNcKZ9X9VcFiZf21OxreWP36Itc5JBsoVzaUFOizABA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a9483e525a3af4d0883df7abe52dc19b8873a71c8d7c1f2b86e8c666a944c866","last_reissued_at":"2026-07-04T15:30:14.203464Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:30:14.203464Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Composite dark matter from a model with composite Higgs boson","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Chris Kouvaris, Maxim Yu. Khlopov","submitted_at":"2008-06-06T15:37:41Z","abstract_excerpt":"In a previous paper \\cite{Khlopov:2007ic}, we showed how the minimal walking technicolor model (WTC) can provide a composite dark matter candidate, by forming bound states between a -2 electrically charged techniparticle and a $^4He^{++}$. We studied the properties of these \\emph{techni-O-helium} $tOHe$ \"atoms\", which behave as warmer dark matter rather than cold. In this paper we extend our work on several different aspects. We study the possibility of a mixed scenario where both $tOHe$ and bound states between +2 and -2 electrically charged techniparticles coexist in the dark matter density."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0806.1191","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/0806.1191/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"0806.1191","created_at":"2026-07-04T15:30:14.204342+00:00"},{"alias_kind":"arxiv_version","alias_value":"0806.1191v2","created_at":"2026-07-04T15:30:14.204342+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0806.1191","created_at":"2026-07-04T15:30:14.204342+00:00"},{"alias_kind":"pith_short_12","alias_value":"VFED4US2HL2N","created_at":"2026-07-04T15:30:14.204342+00:00"},{"alias_kind":"pith_short_16","alias_value":"VFED4US2HL2NBCB5","created_at":"2026-07-04T15:30:14.204342+00:00"},{"alias_kind":"pith_short_8","alias_value":"VFED4US2","created_at":"2026-07-04T15:30:14.204342+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2604.22462","citing_title":"Machine Learning for Multi-messenger Probes of New Physics and Cosmology: A Review and Perspective","ref_index":114,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/VFED4US2HL2NBCB566V6KLOBTO","json":"https://pith.science/pith/VFED4US2HL2NBCB566V6KLOBTO.json","graph_json":"https://pith.science/api/pith-number/VFED4US2HL2NBCB566V6KLOBTO/graph.json","events_json":"https://pith.science/api/pith-number/VFED4US2HL2NBCB566V6KLOBTO/events.json","paper":"https://pith.science/paper/VFED4US2"},"agent_actions":{"view_html":"https://pith.science/pith/VFED4US2HL2NBCB566V6KLOBTO","download_json":"https://pith.science/pith/VFED4US2HL2NBCB566V6KLOBTO.json","view_paper":"https://pith.science/paper/VFED4US2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0806.1191&json=true","fetch_graph":"https://pith.science/api/pith-number/VFED4US2HL2NBCB566V6KLOBTO/graph.json","fetch_events":"https://pith.science/api/pith-number/VFED4US2HL2NBCB566V6KLOBTO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VFED4US2HL2NBCB566V6KLOBTO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VFED4US2HL2NBCB566V6KLOBTO/action/storage_attestation","attest_author":"https://pith.science/pith/VFED4US2HL2NBCB566V6KLOBTO/action/author_attestation","sign_citation":"https://pith.science/pith/VFED4US2HL2NBCB566V6KLOBTO/action/citation_signature","submit_replication":"https://pith.science/pith/VFED4US2HL2NBCB566V6KLOBTO/action/replication_record"}},"created_at":"2026-07-04T15:30:14.204342+00:00","updated_at":"2026-07-04T15:30:14.204342+00:00"}