Oscillations and convective motion in stars with URCA shells

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dc.creatorBisnovatyi-Kogan, G. S.
dc.date2000-04-19
dc.date.accessioned2026-07-07T01:53:14Z
dc.date.available2026-07-07T01:53:14Z
dc.descriptionIt 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.
dc.description8 pages, 3 figures. Proc. 10th Workshop "Nuclear Astrophysics", Rindberg Castle, Tegensee, Germany; March 20-25, 2000
dc.identifierhttps://arxiv.org/abs/astro-ph/0004281
dc.identifierhttp://arxiv.org/abs/astro-ph/0004281
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/894
dc.subjectAstrophysics
dc.titleOscillations and convective motion in stars with URCA shells
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