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Multicomponent models in nuclear astrophysics
2008
Parabolic and Navier–Stokes equations
unpublished
Preserved Fulltext
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.
doi:10.4064/bc81-0-9
fatcat:5frwidy34nd3nkaoetr6pkhuby