Addendum: Existence and absence of Killing horizons in static solutions with symmetries (2024 Class. Quantum Grav. 41 245013)

IF 3.6 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Hideki Maeda and Cristián Martínez
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引用次数: 0

Abstract

In a recent paper (Maeda and Martínez 2024 Class. Quantum Grav.41 245013), we discussed regular extensions of static solutions, or more precisely solutions admitting a hypersurface-orthogonal Killing vector, with an -dimensional Einstein base manifold beyond a non-degenerate Killing horizon in general relativity in dimensions. Under the assumption that components of the energy-momentum tensor for the matter field, which are interpreted in static regions as the energy density ρ, radial pressure , and tangential pressure p2, satisfy linear relations and near the horizon, we proved proposition 6 asserting that solutions for can be extended beyond the Killing horizon and the metric in the regular single-null coordinates is at least there. Although we implicitly assumed there that the values of and in the extended dynamical region remain unchanged, regular extensions are possible even with different values as long as holds there. We present a concrete example of this regular extension in the four-dimensional spherically symmetric case using the Semiz class-I and Whittaker perfect-fluid solutions.
附录:对称静态解中杀戮视界的存在与不存在(2024类)。量子重力。41 245013)
在最近的一篇论文(Maeda和Martínez 2024类。我们讨论了静态解的正则扩展,或者更准确地说,在广义相对论的非简并杀戮视界之外,具有一个维度爱因斯坦基流形的超表面正交杀戮向量的解。假设物质场的能量动量张量的分量(在静态区域被解释为能量密度ρ、径向压力和切向压力p2)在视界附近满足线性关系,我们证明了命题6,它的解可以扩展到Killing视界之外,并且正则单零坐标中的度规至少存在。虽然我们隐式地假设和的值在扩展的动力区域内保持不变,但只要保持在那里,即使有不同的值,也可以进行正则扩展。我们给出了在四维球对称情况下使用Semiz i类和Whittaker完美流体解的正则扩展的一个具体例子。
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来源期刊
Classical and Quantum Gravity
Classical and Quantum Gravity 物理-天文与天体物理
CiteScore
7.00
自引率
8.60%
发文量
301
审稿时长
2-4 weeks
期刊介绍: Classical and Quantum Gravity is an established journal for physicists, mathematicians and cosmologists in the fields of gravitation and the theory of spacetime. The journal is now the acknowledged world leader in classical relativity and all areas of quantum gravity.
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