A rotating black hole solution for shape dynamics

Henrique Gomes

doi:10.1088/0264-9381/31/17/175014

A rotating black hole solution for shape dynamics

2014-08-20

11

OA

AI

DOI：10.1088/0264-9381/31/17/175014

原文链接

查看原文

摘要

En 中文

Shape dynamics is a classical theory of gravity which agrees with general relativity in many important aspects, but which possesses different gauge symmetries and can present some fundamental global differences with respect to Einstein space-times. Here, we present a general procedure for ( locally) mapping stationary, axisymmetric general relativity solutions onto their shape dynamic counterparts. We focus in particular on the rotating black hole solution for shape dynamics and show that many of the properties of the spherically symmetric solution are preserved in the extension to the axisymmetric case: it is also free of physical singularities, it does not form a space-time at the horizon, and it possesses an inversion symmetry about the horizon which leads to us to interpret the solution as a wormhole.

Keyword:

shape dynamics

black hole

classical gravity

general relativity

conformal invariance

wormhole

A rotating black hole solution for shape dynamics

摘要

AI总结

期刊

机构

引用论文