We present results for a suite of 14 three-dimensional, high-resolution hydrodynamical
simulations of delayed-detonation models of Type Ia supernova (SN Ia) explosions. This …

We give an overview of recent efforts to model Type Ia supernovae and related astrophysical
transients resulting from thermonuclear explosions in white dwarfs. In particular we point out …

We present 2D hydrodynamics simulations of near-Chandrasekhar-mass white dwarf (WD)
models for Type Ia supernovae (SNe Ia) using the turbulent deflagration model with a …

A recent study indicated that the inner cores of rapidly accreting () CO white dwarfs may
rotate differentially, with a shear rate near the threshold value for the onset of the dynamical …

In this review, the methodology of large eddy simulations (LES) is introduced and
applications in astrophysics are discussed. As theoretical framework, the scale …

We discuss the effects of rotation on the evolution of accreting carbon-oxygen white dwarfs,
with the emphasis on possible consequences in Type Ia supernova (SN Ia) progenitors …

Aims. We present the first full-star three-dimensional explosion simulations of thermonuclear
supernovae including parameterized deflagration-to-detonation transitions that occur once …

The nature of carbon burning flames in Type Ia supernovae is explored as they interact with
Kolmogorov turbulence. One-dimensional calculations using the Linear Eddy Model of …

Late time synthetic spectra of type Ia supernovae, based on three-dimensional deflagration
models, are presented. We mainly focus on one model,“c3_3d_256_10s”, for which the …

The large range of time and length scales involved in Type Ia supernovae (SNe Ia) requires
the use of flame models. As a prelude to exploring various options for flame models, we …