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dc.contributor.authorLe Pape, S.
dc.contributor.authorBerzak Hopkins, L. F.
dc.contributor.authorDivol, L.
dc.contributor.authorPak, A.
dc.contributor.authorDewald, E. L.
dc.contributor.authorBhandarkar, S.
dc.contributor.authorBennedetti, L. R.
dc.contributor.authorBunn, T.
dc.contributor.authorBiener, J.
dc.contributor.authorCrippen, J.
dc.contributor.authorCasey, D.
dc.contributor.authorEdgell, D.
dc.contributor.authorFittinghoff, D. N.
dc.contributor.authorGoyon, C.
dc.contributor.authorHaan, S.
dc.contributor.authorHatarik, R.
dc.contributor.authorHavre, M.
dc.contributor.authorHo, D. D-M.
dc.contributor.authorIzumi, N.
dc.contributor.authorJaquez, J.
dc.contributor.authorKhan, S. F.
dc.contributor.authorKyrala, G. A.
dc.contributor.authorMa, T.
dc.contributor.authorMackinnon, A. J.
dc.contributor.authorMacPhee, A. G.
dc.contributor.authorMacGowan, B. J.
dc.contributor.authorMeezan, N. B.
dc.contributor.authorMilovich, J.
dc.contributor.authorMillot, M.
dc.contributor.authorMichel, P.
dc.contributor.authorNagel, S. R.
dc.contributor.authorNikroo, A.
dc.contributor.authorPatel, P.
dc.contributor.authorRalph, J.
dc.contributor.authorRoss, J. S.
dc.contributor.authorRice, N. G.
dc.contributor.authorStrozzi, D.
dc.contributor.authorStadermann, M.
dc.contributor.authorVolegov, P.
dc.contributor.authorYeamans, C.
dc.contributor.authorWeber, C.
dc.contributor.authorWild, C.
dc.contributor.authorCallahan, D.
dc.contributor.authorHurricane, O. A.
dc.contributor.authorGatu Johnson, Maria
dc.date.accessioned2018-06-19T14:53:53Z
dc.date.available2018-06-19T14:53:53Z
dc.date.issued2018-06
dc.date.submitted2018-05
dc.identifier.issn0031-9007
dc.identifier.issn1079-7114
dc.identifier.urihttp://hdl.handle.net/1721.1/116411
dc.description.abstractA series of cryogenic, layered deuterium-tritium (DT) implosions have produced, for the first time, fusion energy output twice the peak kinetic energy of the imploding shell. These experiments at the National Ignition Facility utilized high density carbon ablators with a three-shock laser pulse (1.5 MJ in 7.5 ns) to irradiate low gas-filled (0.3  mg/cc of helium) bare depleted uranium hohlraums, resulting in a peak hohlraum radiative temperature ∼290  eV. The imploding shell, composed of the nonablated high density carbon and the DT cryogenic layer, is, thus, driven to velocity on the order of 380  km/s resulting in a peak kinetic energy of ∼21  kJ, which once stagnated produced a total DT neutron yield of 1.9×10¹⁶ (shot N170827) corresponding to an output fusion energy of 54 kJ. Time dependent low mode asymmetries that limited further progress of implosions have now been controlled, leading to an increased compression of the hot spot. It resulted in hot spot areal density (ρr∼0.3  g/cm²) and stagnation pressure (∼360  Gbar) never before achieved in a laboratory experiment.en_US
dc.publisherAmerican Physical Societyen_US
dc.relation.isversionofhttp://dx.doi.org/10.1103/PhysRevLett.120.245003en_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.titleFusion Energy Output Greater than the Kinetic Energy of an Imploding Shell at the National Ignition Facilityen_US
dc.typeArticleen_US
dc.identifier.citationLe Pape, S. et al. "Fusion Energy Output Greater than the Kinetic Energy of an Imploding Shell at the National Ignition Facility." Physical Review Letters 120, 24 (June 2018): 245003 © 2018 American Physical Societyen_US
dc.contributor.departmentMassachusetts Institute of Technology. Plasma Science and Fusion Centeren_US
dc.contributor.mitauthorGatu Johnson, Maria
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.updated2018-06-15T18:00:36Z
dc.language.rfc3066en
dc.rights.holderAmerican Physical Society
dspace.orderedauthorsLe Pape, S.; Berzak Hopkins, L. F.; Divol, L.; Pak, A.; Dewald, E. L.; Bhandarkar, S.; Bennedetti, L. R.; Bunn, T.; Biener, J.; Crippen, J.; Casey, D.; Edgell, D.; Fittinghoff, D. N.; Gatu-Johnson, M.; Goyon, C.; Haan, S.; Hatarik, R.; Havre, M.; Ho, D. D-M.; Izumi, N.; Jaquez, J.; Khan, S. F.; Kyrala, G. A.; Ma, T.; Mackinnon, A. J.; MacPhee, A. G.; MacGowan, B. J.; Meezan, N. B.; Milovich, J.; Millot, M.; Michel, P.; Nagel, S. R.; Nikroo, A.; Patel, P.; Ralph, J.; Ross, J. S.; Rice, N. G.; Strozzi, D.; Stadermann, M.; Volegov, P.; Yeamans, C.; Weber, C.; Wild, C.; Callahan, D.; Hurricane, O. A.en_US
dspace.embargo.termsNen_US
dc.identifier.orcidhttps://orcid.org/0000-0002-2383-1275
mit.licensePUBLISHER_POLICYen_US


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