Sur l’effondrement dynamique des étoiles quantiques pseudo-relativistes

Mathieu Lewin[1]

  • [1] CNRS & Université de Cergy-Pontoise (UMR 8088) 95000 Cergy-Pontoise France

Séminaire Laurent Schwartz — EDP et applications (2011-2012)

  • page 1-20
  • ISSN: 2266-0607

Abstract

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Dans cet exposé, je présente plusieurs modèles quantiques non linéaires permettant de décrire certaines étoiles. Je m’intéresse tout particulièrement à l’effondrement gravitationnel des étoiles trop lourdes, un phénomène modélisé par des solutions qui explosent en temps fini. Je montre l’existence de telles solutions et je décris plusieurs de leurs propriétés au temps d’explosion.

How to cite

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Lewin, Mathieu. "Sur l’effondrement dynamique des étoiles quantiques pseudo-relativistes." Séminaire Laurent Schwartz — EDP et applications (2011-2012): 1-20. <http://eudml.org/doc/251178>.

@article{Lewin2011-2012,
abstract = {Dans cet exposé, je présente plusieurs modèles quantiques non linéaires permettant de décrire certaines étoiles. Je m’intéresse tout particulièrement à l’effondrement gravitationnel des étoiles trop lourdes, un phénomène modélisé par des solutions qui explosent en temps fini. Je montre l’existence de telles solutions et je décris plusieurs de leurs propriétés au temps d’explosion.},
affiliation = {CNRS & Université de Cergy-Pontoise (UMR 8088) 95000 Cergy-Pontoise France},
author = {Lewin, Mathieu},
journal = {Séminaire Laurent Schwartz — EDP et applications},
language = {fre},
pages = {1-20},
publisher = {Institut des hautes études scientifiques & Centre de mathématiques Laurent Schwartz, École polytechnique},
title = {Sur l’effondrement dynamique des étoiles quantiques pseudo-relativistes},
url = {http://eudml.org/doc/251178},
year = {2011-2012},
}

TY - JOUR
AU - Lewin, Mathieu
TI - Sur l’effondrement dynamique des étoiles quantiques pseudo-relativistes
JO - Séminaire Laurent Schwartz — EDP et applications
PY - 2011-2012
PB - Institut des hautes études scientifiques & Centre de mathématiques Laurent Schwartz, École polytechnique
SP - 1
EP - 20
AB - Dans cet exposé, je présente plusieurs modèles quantiques non linéaires permettant de décrire certaines étoiles. Je m’intéresse tout particulièrement à l’effondrement gravitationnel des étoiles trop lourdes, un phénomène modélisé par des solutions qui explosent en temps fini. Je montre l’existence de telles solutions et je décris plusieurs de leurs propriétés au temps d’explosion.
LA - fre
UR - http://eudml.org/doc/251178
ER -

References

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