Equation of state for hot dense matter using a relativistic screened hydrogenic model

Mendoza, M.A.; Garcia Rubiano, Jesus; Gil de la Fe, Juan Miguel; Rodríguez, Rafael; Florido, Ricardo; Martel, Pablo y Mínguez Torres, Emilio (2011). Equation of state for hot dense matter using a relativistic screened hydrogenic model. En: "38th EPS Conference on Plasma Physics", 27/06/2011 - 01/07/2011, Strasbourg, Francia. ISBN 2-914771-68-1.

Descripción

Título: Equation of state for hot dense matter using a relativistic screened hydrogenic model
Autor/es:
  • Mendoza, M.A.
  • Garcia Rubiano, Jesus
  • Gil de la Fe, Juan Miguel
  • Rodríguez, Rafael
  • Florido, Ricardo
  • Martel, Pablo
  • Mínguez Torres, Emilio
Tipo de Documento: Ponencia en Congreso o Jornada (Artículo)
Título del Evento: 38th EPS Conference on Plasma Physics
Fechas del Evento: 27/06/2011 - 01/07/2011
Lugar del Evento: Strasbourg, Francia
Título del Libro: Proceedings of the 38th EPS Conference on Plasma Physics
Fecha: 2011
ISBN: 2-914771-68-1
Materias:
Escuela: E.T.S.I. Industriales (UPM)
Departamento: Ingeniería Nuclear [hasta 2014]
Licencias Creative Commons: Reconocimiento - Sin obra derivada - No comercial

Texto completo

[img]
Vista Previa
PDF (Document Portable Format) - Se necesita un visor de ficheros PDF, como GSview, Xpdf o Adobe Acrobat Reader
Descargar (786kB)

Resumen

The study of matter under conditions of high density, pressure, and temperature is a valuable subject for inertial confinement fusion (ICF), astrophysical phenomena, high-power laser interaction with matter, etc. In all these cases, matter is heated and compressed by strong shocks to high pressures and temperatures, becomes partially or completely ionized via thermal or pressure ionization, and is in the form of dense plasma. The thermodynamics and the hydrodynamics of hot dense plasmas cannot be predicted without the knowledge of the equation of state (EOS) that describes how a material reacts to pressure and how much energy is involved. Therefore, the equation of state often takes the form of pressure and energy as functions of density and temperature. Furthermore, EOS data must be obtained in a timely manner in order to be useful as input in hydrodynamic codes. By this reason, the use of fast, robust and reasonably accurate atomic models, is necessary for computing the EOS of a material.

Más información

ID de Registro: 11743
Identificador DC: http://oa.upm.es/11743/
Identificador OAI: oai:oa.upm.es:11743
URL Oficial: http://ocs.ciemat.es/EPS2011PAP/html/contrib.html
Depositado por: Memoria Investigacion
Depositado el: 15 Nov 2012 10:58
Ultima Modificación: 22 Sep 2014 10:51
  • Open Access
  • Open Access
  • Sherpa-Romeo
    Compruebe si la revista anglosajona en la que ha publicado un artículo permite también su publicación en abierto.
  • Dulcinea
    Compruebe si la revista española en la que ha publicado un artículo permite también su publicación en abierto.
  • Recolecta
  • e-ciencia
  • Observatorio I+D+i UPM
  • OpenCourseWare UPM