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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:scopusStructure measurements of compressed liquid boron at megabar pressures
ArticleAbstract: We report on the first measurements of the structure of compressed liquid boron, as it crosses the mPalabras claves:Autores:Alfredo A. Correa, Davis P., Divol L., Döppner T., Fortmann C., Glenzer S.H., Ma T., Neumayer P., Pape S.L., Plagemann K.U., Redmer R., Schwegler E.Fuentes:scopus