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The cosmic gamma-ray background in the MeV range
P. Ruiz-Lapuente, M. Casse, E. Vangioni-Flam
The -ray background from supernovae is calculated on the basis of the reconstructed efficiency of supernova explosions from star formation at various redshifts. The calculations…
Mixing through shear instabilities
M. Brüggen, W. Hillebrandt
In this paper we present the results of numerical simulations of the Kelvin-Helmholtz instability in a stratified shear layer. This shear instability is believed to be responsible…
Type Ia Supernova Explosion Models
W. Hillebrandt, J. C. Niemeyer
Because calibrated light curves of Type Ia supernovae have become a major tool to determine the local expansion rate of the Universe and also its geometrical structure, considerabl…
Thermonuclear Explosions of Chandrasekhar-Mass White Dwarfs
W. Hillebrandt, M. Reinecke, J. C. Niemeyer
We present a new way of modeling turbulent thermonuclear deflagration fronts in Chandrasekhar-mass white dwarfs, consisting of carbon and oxygen, undergoing a type Ia supernova exp…