当前位置:
X-MOL 学术
›
Classical Quant. Grav.
›
论文详情
Our official English website, www.x-mol.net, welcomes your
feedback! (Note: you will need to create a separate account there.)
Generalized Vaidya solutions in bimetric gravity
Classical and Quantum Gravity ( IF 3.6 ) Pub Date : 2020-07-02 , DOI: 10.1088/1361-6382/ab971a Marcus Högås , Mikica Kocic , Francesco Torsello , Edvard Mörtsell
Classical and Quantum Gravity ( IF 3.6 ) Pub Date : 2020-07-02 , DOI: 10.1088/1361-6382/ab971a Marcus Högås , Mikica Kocic , Francesco Torsello , Edvard Mörtsell
In general relativity, the endpoint of spherically symmetric gravitational collapse is a Schwarzschild--[(A)dS] black hole. In bimetric gravity, it has been speculated that a static end state must also be Schwarzschild--[(A)dS]. To this end, we present a set of exact solutions, including collapsing massless dust particles. For these, the speculation is confirmed.
中文翻译:
双度量重力中的广义 Vaidya 解
在广义相对论中,球对称引力坍缩的终点是一个史瓦西--[(A)dS]黑洞。在双度量引力中,有人推测静态终态也必须是 Schwarzschild--[(A)dS]。为此,我们提出了一组精确的解决方案,包括塌陷无质量的尘埃粒子。对于这些,猜测得到证实。
更新日期:2020-07-02
中文翻译:
双度量重力中的广义 Vaidya 解
在广义相对论中,球对称引力坍缩的终点是一个史瓦西--[(A)dS]黑洞。在双度量引力中,有人推测静态终态也必须是 Schwarzschild--[(A)dS]。为此,我们提出了一组精确的解决方案,包括塌陷无质量的尘埃粒子。对于这些,猜测得到证实。