Radiative Gas Dynamics
by David Weinberg
Publisher: Ohio State University 2007
This course is a graduate-level introduction to gas dynamical processes in astrophysics. Its goal is to teach you the basic concepts and equations of gas dynamics (a.k.a. fluid dynamics or hydrodynamics) and to illustrate the application of gas dynamics to astrophysics.
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by Georg Raffelt - arXiv
The role of neutrinos in stars is introduced for students with little prior astrophysical exposure. We begin with neutrinos as an energy-loss channel in ordinary stars and how stars provide information on neutrinos and possible other particles.
by R. Brout, S. Massar, R. Parentani, P. Spindel - arXiv
The mechanisms which give rise to Hawking radiation are revealed by analyzing pair production. Three problems are considered: pair production in an external electric field, thermalization of a uniformly accelerated detector and accelerated mirrors.
by Dany Page, et al. - arXiv
Neutron stars provide a fertile environment for exploring superfluidity. It is not surprising that Cooper pairing occurs in dense matter since nucleon pairing is observed in nuclei as energy differences between even-even and odd-even nuclei.
by F. Smarandache, V. Christianto - MathTiger
The present book discusses, among other things, various quantization phenomena found in Astrophysics and some related issues including Brownian Motion. Most chapters in this book come from published papers in various peer-reviewed journals.