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dc.contributor.authorHoffman, N. M.
dc.contributor.authorAmendt, P. A.
dc.contributor.authorAtzeni, S.
dc.contributor.authorGlebov, V. Yu.
dc.contributor.authorStoeckl, C.
dc.contributor.authorSeka, W.
dc.contributor.authorMarshall, F. J.
dc.contributor.authorDelettrez, J. A.
dc.contributor.authorSangster, T. C.
dc.contributor.authorBetti, R.
dc.contributor.authorGoncharov, V. N.
dc.contributor.authorMeyerhofer, D. D.
dc.contributor.authorSkupsky, S.
dc.contributor.authorBellei, C.
dc.contributor.authorPino, J.
dc.contributor.authorWilks, S. C.
dc.contributor.authorKagan, Grigory Alexandrovich
dc.contributor.authorMolvig, Kim
dc.contributor.authorNikroo, A.
dc.contributor.authorRosenberg, Michael Jonathan
dc.contributor.authorRinderknecht, Hans George
dc.contributor.authorZylstra, Alex Bennett
dc.contributor.authorLi, Chikang
dc.contributor.authorSeguin, Fredrick Hampton
dc.contributor.authorSio, Hong Weng
dc.contributor.authorGatu Johnson, Maria
dc.contributor.authorFrenje, Johan A.
dc.contributor.authorPetrasso, Richard D.
dc.date.accessioned2014-08-11T14:13:49Z
dc.date.available2014-08-11T14:13:49Z
dc.date.issued2014-05
dc.date.submitted2013-11
dc.identifier.issn0031-9007
dc.identifier.issn1079-7114
dc.identifier.urihttp://hdl.handle.net/1721.1/88656
dc.description.abstractClear evidence of the transition from hydrodynamiclike to strongly kinetic shock-driven implosions is, for the first time, revealed and quantitatively assessed. Implosions with a range of initial equimolar D[superscript 3]He gas densities show that as the density is decreased, hydrodynamic simulations strongly diverge from and increasingly overpredict the observed nuclear yields, from a factor of ∼2 at 3.1  mg/cm[superscript 3] to a factor of 100 at 0.14  mg/cm[superscript 3]. (The corresponding Knudsen number, the ratio of ion mean-free path to minimum shell radius, varied from 0.3 to 9; similarly, the ratio of fusion burn duration to ion diffusion time, another figure of merit of kinetic effects, varied from 0.3 to 14.) This result is shown to be unrelated to the effects of hydrodynamic mix. As a first step to garner insight into this transition, a reduced ion kinetic (RIK) model that includes gradient-diffusion and loss-term approximations to several transport processes was implemented within the framework of a one-dimensional radiation-transport code. After empirical calibration, the RIK simulations reproduce the observed yield trends, largely as a result of ion diffusion and the depletion of the reacting tail ions.en_US
dc.description.sponsorshipUnited States. Dept. of Energy (Grant DE-NA0001857)en_US
dc.description.sponsorshipUnited States. Dept. of Energy (Grant DE-FC52-08NA28752)en_US
dc.description.sponsorshipUniversity of Rochester. Fusion Science Center (5-24431)en_US
dc.description.sponsorshipNational Laser User’s Facility (DE-NA0002035)en_US
dc.description.sponsorshipUniversity of Rochester. Laboratory for Laser Energetics (415935-G)en_US
dc.description.sponsorshipLawrence Livermore National Laboratory (B597367)en_US
dc.publisherAmerican Physical Societyen_US
dc.relation.isversionofhttp://dx.doi.org/10.1103/PhysRevLett.112.185001en_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.titleExploration of the Transition from the Hydrodynamiclike to the Strongly Kinetic Regime in Shock-Driven Implosionsen_US
dc.typeArticleen_US
dc.identifier.citationRosenberg, M. J., H. G. Rinderknecht, N. M. Hoffman, P. A. Amendt, S. Atzeni, A. B. Zylstra, C. K. Li, et al. “Exploration of the Transition from the Hydrodynamiclike to the Strongly Kinetic Regime in Shock-Driven Implosions.” Physical Review Letters 112, no. 18 (May 2014). © 2014 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.mitauthorRosenberg, Michael Jonathanen_US
dc.contributor.mitauthorRinderknecht, Hans Georgeen_US
dc.contributor.mitauthorZylstra, Alex Bennetten_US
dc.contributor.mitauthorLi, Chikangen_US
dc.contributor.mitauthorSeguin, Fredrick Hamptonen_US
dc.contributor.mitauthorSio, Hong Wengen_US
dc.contributor.mitauthorGatu Johnson, Mariaen_US
dc.contributor.mitauthorFrenje, Johan A.en_US
dc.contributor.mitauthorPetrasso, Richard D.en_US
dc.contributor.mitauthorKagan, Grigory Alexandrovich
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.updated2014-07-23T20:49:13Z
dc.language.rfc3066en
dc.rights.holderAmerican Physical Society
dspace.orderedauthorsRosenberg, M. J.; Rinderknecht, H. G.; Hoffman, N. M.; Amendt, P. A.; Atzeni, S.; Zylstra, A. B.; Li, C. K.; Seguin, F. H.; Sio, H.; Johnson, M. Gatu; Frenje, J. A.; Petrasso, R. D.; Glebov, V. Yu.; Stoeckl, C.; Seka, W.; Marshall, F. J.; Delettrez, J. A.; Sangster, T. C.; Betti, R.; Goncharov, V. N.; Meyerhofer, D. D.; Skupsky, S.; Bellei, C.; Pino, J.; Wilks, S. C.; Kagan, G.; Molvig, K.; Nikroo, A.en_US
dc.identifier.orcidhttps://orcid.org/0000-0001-7274-236X
dc.identifier.orcidhttps://orcid.org/0000-0002-6919-4881
dc.identifier.orcidhttps://orcid.org/0000-0003-0489-7479
dc.identifier.orcidhttps://orcid.org/0000-0003-4969-5571
dc.identifier.orcidhttps://orcid.org/0000-0002-1020-3501
mit.licensePUBLISHER_POLICYen_US
mit.metadata.statusComplete


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