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dc.contributor.authorLe, A.
dc.contributor.authorAtzeni, S.
dc.contributor.authorKwan, T. J. T.
dc.contributor.authorKagan, G.
dc.contributor.authorStoeckl, C.
dc.contributor.authorForrest, C. J.
dc.contributor.authorGlebov, V.
dc.contributor.authorRinderknecht, H. G.
dc.contributor.authorAmendt, P.
dc.contributor.authorCasey, D. T.
dc.contributor.authorMancini, R.
dc.contributor.authorTaitano, W. T.
dc.contributor.authorKeenan, B.
dc.contributor.authorSimakov, A. N.
dc.contributor.authorChacón, L.
dc.contributor.authorRegan, S. P.
dc.contributor.authorSangster, T. C.
dc.contributor.authorCampbell, E. M.
dc.contributor.authorSio, Hong Weng
dc.contributor.authorFrenje, Johan A
dc.contributor.authorGatu Johnson, Maria
dc.contributor.authorLi, Changhao
dc.contributor.authorParker, Cody E
dc.contributor.authorKabadi, Neel Vinayak
dc.contributor.authorBose, Anoushka R.
dc.contributor.authorSeguin, Fredrick Hampton
dc.contributor.authorPetrasso, Richard D
dc.date.accessioned2019-02-20T16:30:46Z
dc.date.available2019-02-20T16:30:46Z
dc.date.issued2019-01
dc.date.submitted2018-08
dc.identifier.issn0031-9007
dc.identifier.issn1079-7114
dc.identifier.urihttp://hdl.handle.net/1721.1/120512
dc.description.abstractFuel-ion species dynamics in hydrodynamiclike shock-driven DT³He-filled inertial confinement fusion implosion is quantitatively assessed for the first time using simultaneously measured D³He and DT reaction histories. These reaction histories are measured with the particle x-ray temporal diagnostic, which captures the relative timing between different nuclear burns with unprecedented precision (∼10  ps). The observed 50±10  ps earlier D³He reaction history timing (relative to DT) cannot be explained by average-ion hydrodynamic simulations and is attributed to fuel-ion species separation between the D, T, and ³He ions during shock convergence and rebound. At the onset of the shock burn, inferred ³He/T fuel ratio in the burn region using the measured reaction histories is much higher as compared to the initial gas-filled ratio. As T and ³He have the same mass but different charge, these results indicate that the charge-to-mass ratio plays an important role in driving fuel-ion species separation during strong shock propagation even for these hydrodynamiclike plasmas.en_US
dc.description.sponsorshipUnited States. Department of Energy (Grant DE-FC52-08NA28752)en_US
dc.publisherAmerican Physical Societyen_US
dc.relation.isversionofhttp://dx.doi.org/10.1103/PhysRevLett.122.035001en_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.titleObservations of Multiple Nuclear Reaction Histories and Fuel-Ion Species Dynamics in Shock-Driven Inertial Confinement Fusion Implosionsen_US
dc.typeArticleen_US
dc.identifier.citationSio, H. et al. "Observations of Multiple Nuclear Reaction Histories and Fuel-Ion Species Dynamics in Shock-Driven Inertial Confinement Fusion Implosions." Physical Review Letters 122, 3 (January 2019): 035001 © 2019 American Physical Societyen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Nuclear Science and Engineeringen_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.mitauthorSio, Hong Weng
dc.contributor.mitauthorFrenje, Johan A
dc.contributor.mitauthorGatu Johnson, Maria
dc.contributor.mitauthorLi, Changhao
dc.contributor.mitauthorParker, Cody E
dc.contributor.mitauthorKabadi, Neel Vinayak
dc.contributor.mitauthorBose, Anoushka R.
dc.contributor.mitauthorSeguin, Fredrick Hampton
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.updated2019-01-25T18:00:45Z
dc.language.rfc3066en
dc.rights.holderAmerican Physical Society
dspace.orderedauthorsSio, H.; Frenje, J. A.; Le, A.; Atzeni, S.; Kwan, T. J. T.; Gatu Johnson, M.; Kagan, G.; Stoeckl, C.; Li, C. K.; Parker, C. E.; Forrest, C. J.; Glebov, V.; Kabadi, N. V.; Bose, A.; Rinderknecht, H. G.; Amendt, P.; Casey, D. T.; Mancini, R.; Taitano, W. T.; Keenan, B.; Simakov, A. N.; Chacón, L.; Regan, S. P.; Sangster, T. C.; Campbell, E. M.; Seguin, F. H.; Petrasso, R. D.en_US
dspace.embargo.termsNen_US
dc.identifier.orcidhttps://orcid.org/0000-0001-7274-236X
dc.identifier.orcidhttps://orcid.org/0000-0001-6846-0378
dc.identifier.orcidhttps://orcid.org/0000-0002-2383-1275
dc.identifier.orcidhttps://orcid.org/0000-0002-3019-5887
dc.identifier.orcidhttps://orcid.org/0000-0003-0362-6984
dc.identifier.orcidhttps://orcid.org/0000-0002-1020-3501
mit.licensePUBLISHER_POLICYen_US


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