Modeling Type Ia supernovae with explosions in white dwarfs near and below the Chandrasekhar mass

被引：0

作者：

Roepke, Friedrich K. ^{[1
,2
]}

Lach, Florian ^{[1
,2
]}

Gronow, Sabrina ^{[1
,2
]}

Sim, Stuart A. ^{[3
]}

Callan, Fionntan P. ^{[3
]}

Collins, Christine E. ^{[3
,4
]}

机构：

[1] Heidelberg Univ, Zentrum Astron, Inst Theoret Astrophys, Heidelberg, Germany

[2] Heidelberger Inst Theoret Studien, Heidelberg, Germany

[3] Queens Univ Belfast, Sch Math & Phys, Astrophys Res Ctr, Belfast BT7 1NN, Antrim, North Ireland

[4] GSI Helmholtzzentrum Schwerionenforsch, Darmstadt, Germany

来源：

SIXTEENTH MARCEL GROSSMANN MEETING | 2023年

基金：

美国国家科学基金会;

关键词：

Type Ia supernovae; thermonuclear explosions; white dwarf stars; numerical simulations; SYNTHETIC OBSERVABLES; NUCLEOSYNTHESIS;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The progenitor evolution and the explosion mechanism of Type Ia supernovae remain unexplained. Nonetheless, substantial progress has been made over the past years with three-dimensional hydrodynamic simulations of different scenarios. Here, we review some recent work pertaining to the leading paradigms of modeling: thermonuclear explosions of white dwarf stars near and below the Chandrasekhar mass limit. We discuss implications of the different explosion channels and their predictions of observables.

引用

页码：4420 / 4426

页数：7

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