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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:scopusHigh-temperature ion-thermal behavior from average-atom calculations
ArticleAbstract: Atom-in-jellium calculations of the Einstein frequency were used to calculate the mean displacementPalabras claves:Autores:Alfredo A. Correa, Benedict L.X., Bennett B.I., Bethkenhagen M., Hamel S., Lockard T., Sterne P.A., Swift D.C.Fuentes:scopusReduction of electron-phonon coupling in warm dense iron
ArticleAbstract: The electron-ion relaxation dynamics in warm dense iron were investigated by time-resolved x-ray absPalabras claves:Autores:Alfredo A. Correa, Bae L.J., Barbrel B., Beckwith M.A., Cho B.I., Engelhorn K., Falcone R.W., Fernandez-Panella A., Hamel S., Heimann P.A., Lee J.W., Ogitsu T., Pemmaraju D., Ping Y., Prendergast D.G.Fuentes:scopus