Multi-dimensional fluid flow plays a paramount role in the explosions of massive stars as
core-collapse supernovae. In recent years, three-dimensional (3D) simulations of these …

SN 2011fe was the nearest and best-observed type Ia supernova in a generation, and
brought previous incomplete datasets into sharp contrast with the detailed new data. In …

This paper summarizes a 10-year theoretical and numerical effort to understand the
deflagration-to-detonation transition (DDT). To simulate DDT from first principles, it is …

Although the parietal cortex has been implicated in the neural processes underlying visual
attention, the nature of its contribution is not well understood. We tracked attention in the …

The explosion of sub-Chandrasekhar mass white dwarfs via the double detonation scenario
is a potential explanation for type Ia supernovae. In this scenario, a surface detonation in a …

We investigate whether pure deflagration models of Chandrasekhar-mass carbon–oxygen
white dwarf stars can account for one or more subclass of the observed population of Type …

Large-scale, three-dimensional numerical simulations of the deflagration stage of a
thermonuclear supernova explosion show the formation and evolution of a highly …

In our quest to identify the progenitors of Type Ia supernovae (SNe Ia), we first update the
nucleosynthesis yields for both near-Chandrasekhar-(Ch) and sub-Ch-mass white dwarfs …

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 …

Aims. We present synthetic bolometric and broad-band UBVRI light curves of SNe Ia for four
selected 3D deflagration models of thermonuclear supernovae. Methods. The light curves …