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A measurement of the equation of state of carbon envelopes of white dwarfs
ArticleAbstract: White dwarfs represent the final state of evolution for most stars1–3. Certain classes of white dwarPalabras claves:Autores:Alfredo A. Correa, Bachmann B., Benedict L.X., Collins G.W., Döppner T., DuBois J.L., Elsner F., Falcone R.W., Fontaine G., Gaffney J.A., Glenzer S.H., Hamel S., Johnson W.R., Kostinski N., Kraus D., Kritcher A.L., Lazicki A., MacDonald M.J., Maddox B., Martin M.E., Neumayer P., Nikroo A., Nilsen J., Remington B.A., Saumon D., Sterne P.A., Sweet W., Swift D.C., Whitley H.D.Fuentes:scopusMeasuring the shock impedance mismatch between high-density carbon and deuterium at the National Ignition Facility
ArticleAbstract: Fine-grained diamond, or high-density carbon (HDC), is being used as an ablator for inertial confinePalabras claves:Autores:Alfredo A. Correa, Ali S.J., Baker K.L., Benedict L.X., Berzak Hopkins L.F., Biener J., Celliers P.M., Collins G.W., Coppari F., Divol L., Eggert J.H., Fernandez-Panella A., Fratanduono D.E., Haan S.W., Hamel S., Meezan N.B., Millot M., Moody J.D., Moore A.S., Pape S.L., Ralph J.E., Ross J.S., Rygg J.R., Sterne P.A., Thomas C., Turnbull D.P., Wild C.Fuentes:scopus