Hydrostatic Equilibrium with Degenerate Fermions, Type-II Supernova, and Neutrino Burst
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چکیده
where K, γ are constants. This is not true always, but is in certain limits we will consider later. For specific type of gas (or whatever), we have different K and γ. This is where microscopic physics comes in. We continue the discussions at the level of macroscopic physics with K and γ taken as some constants, and come back to their specific values for the case of degenerate fermions later. The above second-order differential equation can be solved semi-analytically, using the following changes in the variables:
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تاریخ انتشار 1998