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Titlebook: Dark Matter in Astro- and Particle Physics; Proceedings of the I H. V. Klapdor-Kleingrothaus Conference proceedings 2001 Springer-Verlag Be

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书目名称Dark Matter in Astro- and Particle Physics
副标题Proceedings of the I
编辑H. V. Klapdor-Kleingrothaus
视频video
图书封面Titlebook: Dark Matter in Astro- and Particle Physics; Proceedings of the I H. V. Klapdor-Kleingrothaus Conference proceedings 2001 Springer-Verlag Be
描述Dark matter in the Universe has become one of the most exciting and central fields of astrophysics, particle physics and cosmology. The lectures and talks in this book emphasize the experimental and theoretical status and perspectives of the ongoing search for dark matter, and the future potential of the field into the next millennium, stressing in particular the interplay between astro- and particle physics.
出版日期Conference proceedings 2001
关键词Baryon; Beta decay; Boson; Galaxy; Gravity; Neutrino; Particle Physics; astroparticles; astrophysics; cosmolo
版次1
doihttps://doi.org/10.1007/978-3-642-56643-1
isbn_softcover978-3-642-62608-1
isbn_ebook978-3-642-56643-1
copyrightSpringer-Verlag Berlin Heidelberg 2001
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Preheating, Thermalization and SupergravityThis contribution collects new recent results on preheating after inflation. We discuss tachyonic preheating in the SUSY motivated hybrid inflation; development of equilibrium after preheating; theory of fermionic preheating and the problem of gravitino overproduction from preheating.
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Conference proceedings 2001alks in this book emphasize the experimental and theoretical status and perspectives of the ongoing search for dark matter, and the future potential of the field into the next millennium, stressing in particular the interplay between astro- and particle physics.
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ures and talks in this book emphasize the experimental and theoretical status and perspectives of the ongoing search for dark matter, and the future potential of the field into the next millennium, stressing in particular the interplay between astro- and particle physics.978-3-642-62608-1978-3-642-56643-1
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https://doi.org/10.1007/978-3-322-93659-2198, 6503, and 7184 are analyzed. For these galaxies the radial velocity dispersions of the stars have been measured. If the parameters of the decompositions are chosen according to the ‘maximum’ disk hypothesis, the Toomre . stability parameter is sytematically less than one, which is a strong argu
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