On the progenitors of Type Ia supernovae

被引：179

作者：

Livio, Mario ^{[1
,2
]}

Mazzali, Paolo ^{[2
,3
]}

机构：

[1] Univ Nevada, Dept Phys & Astron, 4505 South Maryland Pkwy, Las Vegas, NV 89154 USA

[2] Weizmann Inst Sci, Fac Phys, Dept Particle Phys & Astrophys, IL-76100 Rehovot, Israel

[3] Liverpool John Moores Univ, Astrophys Res Inst, IC2,Liverpool Sci Pk,146 Brownlow Hill, Liverpool L3 5RF, Merseyside, England

来源：

PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS | 2018年 / 736卷

关键词：

Type la supernovae; White dwarfs; Binary stars; Thermonuclear detonation; Thermonuclear deflagration; ACCRETING WHITE-DWARFS; CORE-DEGENERATE SCENARIO; PARTICLE HYDRODYNAMICS SIMULATIONS; BOLOMETRIC LIGHT CURVES; DELAY-TIME DISTRIBUTION; HYDROGEN SHELL FLASHES; X-RAY SOURCES; ABUNDANCE STRATIFICATION; CIRCUMSTELLAR MATERIAL; COMMON ENVELOPE;

D O I：

10.1016/j.physrep.2018.02.002

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

We review all the models proposed for the progenitor systems of Type Ia supernovae and discuss the strengths and weaknesses of each scenario when confronted with observations. We show that all scenarios encounter at least a few serious difficulties, if taken to represent a comprehensive model for the progenitors of all Type la supernovae (SNe la). Consequently, we tentatively conclude that there is probably more than one channel leading SNe Ia. While the single-degenerate scenario (in which a single white dwarf accretes mass from a normal stellar companion) has been studied in some detail, the other scenarios will need a similar level of scrutiny before any firm conclusions can be drawn. (C) 2018 Elsevier B.V. All rights reserved.

引用

页码：1 / 23

页数：23

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