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dc.contributor.authorHerrmann, H. W.
dc.contributor.authorKim, Y. H.
dc.contributor.authorHale, G.
dc.contributor.authorRubery, M.
dc.contributor.authorParis, M.
dc.contributor.authorBacher, A.
dc.contributor.authorBrune, C. R.
dc.contributor.authorForrest, C.
dc.contributor.authorGlebov, V. Yu.
dc.contributor.authorJanezic, R.
dc.contributor.authorMcNabb, D.
dc.contributor.authorNikroo, A.
dc.contributor.authorPino, J.
dc.contributor.authorSangster, T. C.
dc.contributor.authorSeka, W.
dc.contributor.authorStoeckl, C.
dc.contributor.authorZylstra, Alex Bennett
dc.contributor.authorGatu Johnson, Maria
dc.contributor.authorFrenje, Johan A
dc.contributor.authorLi, Chikang
dc.contributor.authorSeguin, Fredrick Hampton
dc.contributor.authorSio, Hong Weng
dc.contributor.authorPetrasso, Richard D
dc.date.accessioned2017-06-02T17:57:44Z
dc.date.available2017-06-02T17:57:44Z
dc.date.issued2016-07
dc.date.submitted2016-04
dc.identifier.issn0031-9007
dc.identifier.issn1079-7114
dc.identifier.urihttp://hdl.handle.net/1721.1/109553
dc.description.abstractLight nuclei were created during big-bang nucleosynthesis (BBN). Standard BBN theory, using rates inferred from accelerator-beam data, cannot explain high levels of [superscript 6]Li in low-metallicity stars. Using high-energy-density plasmas we measure the T([superscript 3]He,γ)[superscript 6]Li reaction rate, a candidate for anomalously high [superscript 6]Li production; we find that the rate is too low to explain the observations, and different than values used in common BBN models. This is the first data directly relevant to BBN, and also the first use of laboratory plasmas, at comparable conditions to astrophysical systems, to address a problem in nuclear astrophysics.en_US
dc.description.sponsorshipUnited States. Department of Energy (DE-NA0001857)en_US
dc.description.sponsorshipUnited States. Department of Energy (DE-FC52-08NA28752)en_US
dc.description.sponsorshipUnited States. Department of Energy (DEFG02-88ER40387)en_US
dc.description.sponsorshipUnited States. Department of Energy (DE-NA0001837)en_US
dc.description.sponsorshipUnited States. Department of Energy (DE-AC52- 06NA25396)en_US
dc.description.sponsorshipLawrence Livermore National Laboratory (B597367)en_US
dc.description.sponsorshipLawrence Livermore National Laboratory (415935- G)en_US
dc.description.sponsorshipUniversity of Rochester. Fusion Science Center (524431)en_US
dc.description.sponsorshipNational Laser User’s Facility (DE-NA0002035)en_US
dc.description.sponsorshipNational Science Foundation (U.S.). Graduate Research Fellowship Program (Grant 1122374)en_US
dc.description.sponsorshipLos Alamos National Laboratory. Laboratory Directed Research and Development Program (20150717PRD2)en_US
dc.publisherAmerican Physical Societyen_US
dc.relation.isversionofhttp://dx.doi.org/10.1103/PhysRevLett.117.035002en_US
dc.rightsArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.en_US
dc.sourceAmerican Physical Societyen_US
dc.titleUsing Inertial Fusion Implosions to Measure the T + [superscript 3]He Fusion Cross Section at Nucleosynthesis-Relevant Energiesen_US
dc.title.alternativeUsing Inertial Fusion Implosions to Measure the T + 3He Fusion Cross Section at Nucleosynthesis-Relevant Energiesen_US
dc.typeArticleen_US
dc.identifier.citationZylstra, A. B. et al. “Using Inertial Fusion Implosions to Measure the T + He 3 Fusion Cross Section at Nucleosynthesis-Relevant Energies.” Physical Review Letters 117.3 (2016): n. pag. © 2016 American Physical Societyen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.departmentMassachusetts Institute of Technology. Plasma Science and Fusion Centeren_US
dc.contributor.mitauthorZylstra, Alex Bennett
dc.contributor.mitauthorGatu Johnson, Maria
dc.contributor.mitauthorFrenje, Johan A
dc.contributor.mitauthorLi, Chikang
dc.contributor.mitauthorSeguin, Fredrick Hampton
dc.contributor.mitauthorSio, Hong Weng
dc.contributor.mitauthorPetrasso, Richard D
dc.relation.journalPhysical Review Lettersen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2016-07-11T22:00:08Z
dc.language.rfc3066en
dc.rights.holderAmerican Physical Society
dspace.orderedauthorsZylstra, A. B.; Herrmann, H. W.; Johnson, M. Gatu; Kim, Y. H.; Frenje, J. A.; Hale, G.; Li, C. K.; Rubery, M.; Paris, M.; Bacher, A.; Brune, C. R.; Forrest, C.; Glebov, V. Yu.; Janezic, R.; McNabb, D.; Nikroo, A.; Pino, J.; Sangster, T. C.; Séguin, F. H.; Seka, W.; Sio, H.; Stoeckl, C.; Petrasso, R. D.en_US
dspace.embargo.termsNen_US
dc.identifier.orcidhttps://orcid.org/0000-0003-0489-7479
dc.identifier.orcidhttps://orcid.org/0000-0002-6919-4881
dc.identifier.orcidhttps://orcid.org/0000-0001-7274-236X
dc.identifier.orcidhttps://orcid.org/0000-0002-1020-3501
mit.licensePUBLISHER_POLICYen_US
mit.metadata.statusComplete


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