In this paper we address the theory of type Ia supernovae from the moment of carbon runaway up to several hours after the explosion. We have concentrated on the boiling-pot model: a deflagration characterized by the (nearly-) simultaneous ignition of a number of bubbles that pervade the core of the white dwarf.Peer Reviewe
We study a type Ia supernova explosion using three-dimensional numerical simulations based on reacti...
We describe a mechanism by which a failed deflagration of a Chandrasekhar-mass carbon-oxygen white d...
Type Ia supenovae are commonly thought to be the outcome of the thermonuclear explosion of a white d...
In this paper we address the theory of type Ia supernovae from the moment of carbon runaway up to se...
In this paper we address the theory of type Ia supernovae from the moment of carbon runaway up to se...
The observable properties of a Type Ia supernova are sensitive to how the nuclear runaway ignites in...
Supernovae are some of the brightest and most energetic explosions in the universe. In the mid- to l...
Abstract. A self-consistent model of white dwarf burning in Supernova Ia events is presented which i...
Because calibrated light curves of Type Ia supernovae have become a major tool to determine the loca...
A self-consistent model of white dwarf burning in Supernova Ia events is presented which includes th...
Theoretically, thermonuclear runaway of a white dwarf (WD) could set in for various evolutionary sce...
The observed sub-class of “superluminous” Type Ia supernovae lacks a convincing theoretical explanat...
International audienceContext. It is widely accepted that the onset of the explosive carbon burning ...
Abstract: Type Ia supernovae are thought to result from thermonuclear explosions of carbon-oxygen wh...
Observational evidences point to a common explosion mechanism of Type Ia supernovae based on a delay...
We study a type Ia supernova explosion using three-dimensional numerical simulations based on reacti...
We describe a mechanism by which a failed deflagration of a Chandrasekhar-mass carbon-oxygen white d...
Type Ia supenovae are commonly thought to be the outcome of the thermonuclear explosion of a white d...
In this paper we address the theory of type Ia supernovae from the moment of carbon runaway up to se...
In this paper we address the theory of type Ia supernovae from the moment of carbon runaway up to se...
The observable properties of a Type Ia supernova are sensitive to how the nuclear runaway ignites in...
Supernovae are some of the brightest and most energetic explosions in the universe. In the mid- to l...
Abstract. A self-consistent model of white dwarf burning in Supernova Ia events is presented which i...
Because calibrated light curves of Type Ia supernovae have become a major tool to determine the loca...
A self-consistent model of white dwarf burning in Supernova Ia events is presented which includes th...
Theoretically, thermonuclear runaway of a white dwarf (WD) could set in for various evolutionary sce...
The observed sub-class of “superluminous” Type Ia supernovae lacks a convincing theoretical explanat...
International audienceContext. It is widely accepted that the onset of the explosive carbon burning ...
Abstract: Type Ia supernovae are thought to result from thermonuclear explosions of carbon-oxygen wh...
Observational evidences point to a common explosion mechanism of Type Ia supernovae based on a delay...
We study a type Ia supernova explosion using three-dimensional numerical simulations based on reacti...
We describe a mechanism by which a failed deflagration of a Chandrasekhar-mass carbon-oxygen white d...
Type Ia supenovae are commonly thought to be the outcome of the thermonuclear explosion of a white d...