Oscillations and convective motion in stars with URCA shells

Details Oscillations and convective motion in stars with URCA shells Oscillations and convective motion in stars with URCA shells

2000-04-19

arxiv.org/abs/astro-ph/0004281v1

Astronomy and Astrophysics

Astrophysics

8 pages, 3 figures. Proc. 10th Workshop "Nuclear Astrophysics", Rindberg Castle, Tegensee, Germany; March 20-25, 2000

Scientific paper

It is shown that in presence of URCA shell pulsational energy losses due to
neutrino emission and nonequilibrium beta heating are much less than energy
losses by excitation of short-wavelength acoustic waves. Convective motion in
presence of URCA shell is considered, and equations generalizing the mean free
path model of convection are derived.

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