Multicomponent models in nuclear astrophysics
Volume 81 / 2008
Banach Center Publications 81 (2008), 133-156
MSC: Primary 76N10; Secondary 80A32.
DOI: 10.4064/bc81-0-9
Abstract
We consider hydrodynamical models describing the evolution of a gaseous star in which the presence of thermonuclear reactions between several species leads to a multicomponent formulation. In the case of binary mixtures, recent 3D results are evoked. In the one-dimensional situation, we can prove global estimates and stabilization for some simplified model.
