Black hole minimum size and scalar charge in shift-symmetric theories

Black hole minimum size and scalar charge in shift-symmetric theories
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DOI:
10.1088/1361-6382/acdd42
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发表时间:
2022-11
影响因子:
3.5
通讯作者:
Farid Thaalba;Georgios Antoniou;T. Sotiriou
Farid Thaalba;Georgios Antoniou;T. Sotiriou
中科院分区:
物理与天体物理3区
文献类型:
--
作者:
Farid Thaalba;Georgios Antoniou;T. Sotiriou

文献摘要

相似文献

众所周知,对于位移对称标量,只有高斯-邦纳(GB)不变量的线性耦合才能引入黑洞头发。这样的多毛黑洞有一个最小质量,由这种相互作用的耦合决定,和一个标量电荷,唯一地由它们的质量和自旋决定,对于一个固定的耦合值。在这里,我们探讨如何额外的移位对称的相互作用影响的黑洞的结构,最小质量的值,和标量电荷。
It is known that, for shift-symmetric scalars, only a linear coupling with the Gauss–Bonnet (GB) invariant can introduce black hole hair. Such hairy black holes have a minimum mass, determined by the coupling of this interaction, and a scalar charge that is uniquely determined by their mass and spin for a fixed value of that coupling. Here we explore how additional shift-symmetric interactions affect the structure of the black hole, the value of the minimum mass, and the scalar charge.