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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:scopusAb initio modeling of nonequilibrium electron-ion dynamics of iron in the warm dense matter regime
ArticleAbstract: The spatiotemporal electron and ion relaxation dynamics of iron induced by femtosecond laser pulsesPalabras claves:Autores:Alfredo A. Correa, Fernandez-Panella A., Hamel S., Ogitsu T., Pemmaraju C.D., Ping Y., Prendergast D.G.Fuentes:scopusMolecular Dynamics Simulations of Warm Dense Carbon
ArticleAbstract: We present classical and DFT-based molecular dynamics (MD) simulations of carbon in the warm dense mPalabras claves:Classical molecular dynamics, Density functional molecular dynamics, Equation of stateAutores:Alfredo A. Correa, Benedict L.X., Hamel S., Sanchez D.M., Whitley H.D.Fuentes:scopus