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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:scopusDifferential heating: A versatile method for thermal conductivity measurements in high-energy-density matter
ArticleAbstract: We propose a method for thermal conductivity measurements of high energy density matter based on difPalabras claves:Autores:Alfredo A. Correa, Boehly T., Collins G.W., Fernandez-Panella A., Fratanduono D.E., Landen O., London R., Ping Y., Shepherd R., Sio H., Sterne P.A., Whitley H.D.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