Citation

BibTex format

@article{Xie:2021:10.1103/PhysRevLett.126.241104,
author = {Xie, Y and Zhang, J and Silva, HO and de, Rham C and Witek, H and Yunes, N},
doi = {10.1103/PhysRevLett.126.241104},
journal = {Physical Review Letters},
pages = {1--7},
title = {Square peg in a circular hole: choosing the right ansatz for isolated black holes in generic gravitational theories},
url = {http://dx.doi.org/10.1103/PhysRevLett.126.241104},
volume = {126},
year = {2021}
}

RIS format (EndNote, RefMan)

TY  - JOUR
AB - The metric of a spacetime can be greatly simplified if the spacetime is circular. We prove that in generic effective theories of gravity, the spacetime of a stationary, axisymmetric, and asymptotically flat solution must be circular if the solution can be obtained perturbatively from a solution in the general relativity limit. This result applies to a broad class of gravitational theories that include arbitrary scalars and vectors in their light sector, so long as their nonstandard kinetic terms and nonmininal couplings to gravity are treated perturbatively.
AU - Xie,Y
AU - Zhang,J
AU - Silva,HO
AU - de,Rham C
AU - Witek,H
AU - Yunes,N
DO - 10.1103/PhysRevLett.126.241104
EP - 7
PY - 2021///
SN - 0031-9007
SP - 1
TI - Square peg in a circular hole: choosing the right ansatz for isolated black holes in generic gravitational theories
T2 - Physical Review Letters
UR - http://dx.doi.org/10.1103/PhysRevLett.126.241104
UR - https://www.webofscience.com/api/gateway?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000663310900004&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=a2bf6146997ec60c407a63945d4e92bb
UR - https://journals.aps.org/prl/abstract/10.1103/PhysRevLett.126.241104
UR - http://hdl.handle.net/10044/1/106032
VL - 126
ER -

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