Mathematical Problems Of Radiative Equilibrium
by Eberhard Hopf
Publisher: Cambridge University Press 1934
Number of pages: 123
Schwarzschild's classical work on absorption and diffusion in the sun's atmosphere, and the continuation of these investigations through A. Eddington, J.H. Jeans, R.A. Milne and others, have rendered the theory of radiative equilibrium a definite chapter of mathematical astrophysics. Besides the known results (theory of Milne's standard model, infinitely deep slab with no radiation incident on its surface) the reader will also find more or less detailed discussions of other models.
Home page url
Download or read it online for free here:
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 Boris Pioline - arXiv
In these lecture notes, the author reviews some recent developments on the relation between the macroscopic entropy of four-dimensional BPS black holes and the microscopic counting of states, beyond the thermodynamical, large charge limit.
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.
by Jacco Vink - arXiv
Supernova remnants are beautiful astronomical objects that are also of high scientific interest, because they provide insights into supernova explosion mechanisms, and because they are the likely sources of Galactic cosmic rays.