{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:FOH2FWBFHRV66RPDAGCSHFEWVE","short_pith_number":"pith:FOH2FWBF","schema_version":"1.0","canonical_sha256":"2b8fa2d8253c6bef45e30185239496a90000a1089fbe44695777c9275ebbb5cb","source":{"kind":"arxiv","id":"1601.02412","version":2},"attestation_state":"computed","paper":{"title":"Model-independent determination of the astrophysical S-factor in laser-induced fusion plasmas","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.plasm-ph"],"primary_cat":"nucl-ex","authors_text":"A. Bonasera, A. C. Bernstein, D. Lattuada, E. Gaul, F. Consoli, G. Dyer, H. J. Quevedo, J. B. Natowitz, K. Hagel, K. Schmidt, M. Barbarino, M. Barbui, M. E. Donovan, M. Warren, P. Andreoli, R. De Angelis, S. Kimura, T. Ditmire, W. Bang","submitted_at":"2016-01-11T12:08:56Z","abstract_excerpt":"In this work, we present a new and general method for measuring the astrophysical S-factor of nuclear reactions in laser-induced plasmas and we apply it to d(d,n)$^{3}$He. The experiment was performed with the Texas Petawatt laser, which delivered 150-270 fs pulses of energy ranging from 90 to 180 J to D$_{2}$ or CD$_{4}$ molecular clusters. After removing the background noise, we used the measured time-of-flight data of energetic deuterium ions to obtain their energy distribution. We derive the S-factor using the measured energy distribution of the ions, the measured volume of the fusion plas"},"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":"1601.02412","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-ex","submitted_at":"2016-01-11T12:08:56Z","cross_cats_sorted":["physics.plasm-ph"],"title_canon_sha256":"92779c13d5db799e08d30b8006796468e90be3692031bf928d246746c4a78867","abstract_canon_sha256":"f8ad3c5fbcefabff769c63b42c51e4826dc76386ba6309c506eee3e552280b41"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:16:14.827527Z","signature_b64":"szFFd2PIdJx/YM/HG4QFxcyu386b0zvl9HzN+2i4tUEm2N5ruXxIe0Fc9pT6zr0G8JsqL1uM1pxQhEzShIETBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2b8fa2d8253c6bef45e30185239496a90000a1089fbe44695777c9275ebbb5cb","last_reissued_at":"2026-05-18T01:16:14.826869Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:16:14.826869Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Model-independent determination of the astrophysical S-factor in laser-induced fusion plasmas","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.plasm-ph"],"primary_cat":"nucl-ex","authors_text":"A. Bonasera, A. C. Bernstein, D. Lattuada, E. Gaul, F. Consoli, G. Dyer, H. J. Quevedo, J. B. Natowitz, K. Hagel, K. Schmidt, M. Barbarino, M. Barbui, M. E. Donovan, M. Warren, P. Andreoli, R. De Angelis, S. Kimura, T. Ditmire, W. Bang","submitted_at":"2016-01-11T12:08:56Z","abstract_excerpt":"In this work, we present a new and general method for measuring the astrophysical S-factor of nuclear reactions in laser-induced plasmas and we apply it to d(d,n)$^{3}$He. The experiment was performed with the Texas Petawatt laser, which delivered 150-270 fs pulses of energy ranging from 90 to 180 J to D$_{2}$ or CD$_{4}$ molecular clusters. After removing the background noise, we used the measured time-of-flight data of energetic deuterium ions to obtain their energy distribution. We derive the S-factor using the measured energy distribution of the ions, the measured volume of the fusion plas"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1601.02412","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":"1601.02412","created_at":"2026-05-18T01:16:14.826980+00:00"},{"alias_kind":"arxiv_version","alias_value":"1601.02412v2","created_at":"2026-05-18T01:16:14.826980+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1601.02412","created_at":"2026-05-18T01:16:14.826980+00:00"},{"alias_kind":"pith_short_12","alias_value":"FOH2FWBFHRV6","created_at":"2026-05-18T12:30:15.759754+00:00"},{"alias_kind":"pith_short_16","alias_value":"FOH2FWBFHRV66RPD","created_at":"2026-05-18T12:30:15.759754+00:00"},{"alias_kind":"pith_short_8","alias_value":"FOH2FWBF","created_at":"2026-05-18T12:30:15.759754+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FOH2FWBFHRV66RPDAGCSHFEWVE","json":"https://pith.science/pith/FOH2FWBFHRV66RPDAGCSHFEWVE.json","graph_json":"https://pith.science/api/pith-number/FOH2FWBFHRV66RPDAGCSHFEWVE/graph.json","events_json":"https://pith.science/api/pith-number/FOH2FWBFHRV66RPDAGCSHFEWVE/events.json","paper":"https://pith.science/paper/FOH2FWBF"},"agent_actions":{"view_html":"https://pith.science/pith/FOH2FWBFHRV66RPDAGCSHFEWVE","download_json":"https://pith.science/pith/FOH2FWBFHRV66RPDAGCSHFEWVE.json","view_paper":"https://pith.science/paper/FOH2FWBF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1601.02412&json=true","fetch_graph":"https://pith.science/api/pith-number/FOH2FWBFHRV66RPDAGCSHFEWVE/graph.json","fetch_events":"https://pith.science/api/pith-number/FOH2FWBFHRV66RPDAGCSHFEWVE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FOH2FWBFHRV66RPDAGCSHFEWVE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FOH2FWBFHRV66RPDAGCSHFEWVE/action/storage_attestation","attest_author":"https://pith.science/pith/FOH2FWBFHRV66RPDAGCSHFEWVE/action/author_attestation","sign_citation":"https://pith.science/pith/FOH2FWBFHRV66RPDAGCSHFEWVE/action/citation_signature","submit_replication":"https://pith.science/pith/FOH2FWBFHRV66RPDAGCSHFEWVE/action/replication_record"}},"created_at":"2026-05-18T01:16:14.826980+00:00","updated_at":"2026-05-18T01:16:14.826980+00:00"}