{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:FYMX5KW53POBI3NJ4FLCFQBT34","short_pith_number":"pith:FYMX5KW5","schema_version":"1.0","canonical_sha256":"2e197eaadddbdc146da9e15622c033df188a51989bfca6e79daeff5dca10da81","source":{"kind":"arxiv","id":"1709.08522","version":2},"attestation_state":"computed","paper":{"title":"Production of deuterons, tritons, $^{3}$He nuclei and their anti-nuclei in pp collisions at $\\mathbf{\\sqrt{{\\textit s}}}$ = 0.9, 2.76 and 7 TeV","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"nucl-ex","authors_text":"ALICE Collaboration","submitted_at":"2017-09-25T14:41:07Z","abstract_excerpt":"Invariant differential yields of deuterons and anti-deuterons in pp collisions at $\\sqrt{s}$ = 0.9, 2.76 and 7 TeV and the yields of tritons, $^{3}$He nuclei and their anti-nuclei at $\\sqrt{s}$ = 7 TeV have been measured with the ALICE detector at the CERN Large Hadron Collider. The measurements cover a wide transverse momentum ($p_{\\text{T}}$) range in the rapidity interval $|y|<0.5$, extending both the energy and the $p_{\\text{T}}$ reach of previous measurements up to 3 GeV/$c$ for $A=2$ and 6 GeV/$c$ for $A=3$. The coalescence parameters of (anti-)deuterons and $^{3}\\overline{\\text{He}}$ nu"},"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":"1709.08522","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"nucl-ex","submitted_at":"2017-09-25T14:41:07Z","cross_cats_sorted":["hep-ex"],"title_canon_sha256":"591915b8ebc0b3e818c37a97d6c20f9f4f92673ab639722b492a35690417411c","abstract_canon_sha256":"7a9e05652ba9238cf6a0b0fc97d07cdbf869582022b8a05df083814ac6ccc3c3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:54:56.602412Z","signature_b64":"Ygqc95+tF+SIYHPe0GtIpneeasVw8FQr8yXhGzZSyqDZystcm7gXa2ubDNm9inqo1pzEXpz2MlEayWmeNaDAAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2e197eaadddbdc146da9e15622c033df188a51989bfca6e79daeff5dca10da81","last_reissued_at":"2026-05-17T23:54:56.601881Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:54:56.601881Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Production of deuterons, tritons, $^{3}$He nuclei and their anti-nuclei in pp collisions at $\\mathbf{\\sqrt{{\\textit s}}}$ = 0.9, 2.76 and 7 TeV","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"nucl-ex","authors_text":"ALICE Collaboration","submitted_at":"2017-09-25T14:41:07Z","abstract_excerpt":"Invariant differential yields of deuterons and anti-deuterons in pp collisions at $\\sqrt{s}$ = 0.9, 2.76 and 7 TeV and the yields of tritons, $^{3}$He nuclei and their anti-nuclei at $\\sqrt{s}$ = 7 TeV have been measured with the ALICE detector at the CERN Large Hadron Collider. The measurements cover a wide transverse momentum ($p_{\\text{T}}$) range in the rapidity interval $|y|<0.5$, extending both the energy and the $p_{\\text{T}}$ reach of previous measurements up to 3 GeV/$c$ for $A=2$ and 6 GeV/$c$ for $A=3$. The coalescence parameters of (anti-)deuterons and $^{3}\\overline{\\text{He}}$ nu"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1709.08522","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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1709.08522","created_at":"2026-05-17T23:54:56.601966+00:00"},{"alias_kind":"arxiv_version","alias_value":"1709.08522v2","created_at":"2026-05-17T23:54:56.601966+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1709.08522","created_at":"2026-05-17T23:54:56.601966+00:00"},{"alias_kind":"pith_short_12","alias_value":"FYMX5KW53POB","created_at":"2026-05-18T12:31:15.632608+00:00"},{"alias_kind":"pith_short_16","alias_value":"FYMX5KW53POBI3NJ","created_at":"2026-05-18T12:31:15.632608+00:00"},{"alias_kind":"pith_short_8","alias_value":"FYMX5KW5","created_at":"2026-05-18T12:31:15.632608+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.08338","citing_title":"Revisiting predictions for cosmic-ray antinucleon fluxes from Galactic Dark Matter","ref_index":61,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FYMX5KW53POBI3NJ4FLCFQBT34","json":"https://pith.science/pith/FYMX5KW53POBI3NJ4FLCFQBT34.json","graph_json":"https://pith.science/api/pith-number/FYMX5KW53POBI3NJ4FLCFQBT34/graph.json","events_json":"https://pith.science/api/pith-number/FYMX5KW53POBI3NJ4FLCFQBT34/events.json","paper":"https://pith.science/paper/FYMX5KW5"},"agent_actions":{"view_html":"https://pith.science/pith/FYMX5KW53POBI3NJ4FLCFQBT34","download_json":"https://pith.science/pith/FYMX5KW53POBI3NJ4FLCFQBT34.json","view_paper":"https://pith.science/paper/FYMX5KW5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1709.08522&json=true","fetch_graph":"https://pith.science/api/pith-number/FYMX5KW53POBI3NJ4FLCFQBT34/graph.json","fetch_events":"https://pith.science/api/pith-number/FYMX5KW53POBI3NJ4FLCFQBT34/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FYMX5KW53POBI3NJ4FLCFQBT34/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FYMX5KW53POBI3NJ4FLCFQBT34/action/storage_attestation","attest_author":"https://pith.science/pith/FYMX5KW53POBI3NJ4FLCFQBT34/action/author_attestation","sign_citation":"https://pith.science/pith/FYMX5KW53POBI3NJ4FLCFQBT34/action/citation_signature","submit_replication":"https://pith.science/pith/FYMX5KW53POBI3NJ4FLCFQBT34/action/replication_record"}},"created_at":"2026-05-17T23:54:56.601966+00:00","updated_at":"2026-05-17T23:54:56.601966+00:00"}