Numerical solutions for asymptotically flat rotating black holes in the cubic
Galileon theory are presented. These black holes are endowed with a nontrivial
scalar field and exhibit a non-Schwarzschild behaviour: faster than $1/r$
convergence to Minkowski spacetime at spatial infinity and hence vanishing of
the Komar mass. The metrics are compared with the Kerr metric for various
couplings and angular velocities. Their physical properties are extracted and
show significant deviations from the Kerr case.
Description
Hairy rotating black holes in cubic Galileon theory
cite arxiv:1910.08451Comment: 31 pages, 9 figures; v2 minor improvements, added references, minor typos corrected, version published in Classical and Quantum Gravity
%0 Generic
%1 vanaelst2019hairy
%A Van Aelst, Karim
%A Gourgoulhon, Eric
%A Grandclément, Philippe
%A Charmousis, Christos
%D 2019
%K BlackHole Galileon extendedgravity myown rotating
%R 10.1088/1361-6382/ab6391
%T Hairy rotating black holes in cubic Galileon theory
%U http://arxiv.org/abs/1910.08451
%X Numerical solutions for asymptotically flat rotating black holes in the cubic
Galileon theory are presented. These black holes are endowed with a nontrivial
scalar field and exhibit a non-Schwarzschild behaviour: faster than $1/r$
convergence to Minkowski spacetime at spatial infinity and hence vanishing of
the Komar mass. The metrics are compared with the Kerr metric for various
couplings and angular velocities. Their physical properties are extracted and
show significant deviations from the Kerr case.
@misc{vanaelst2019hairy,
abstract = {Numerical solutions for asymptotically flat rotating black holes in the cubic
Galileon theory are presented. These black holes are endowed with a nontrivial
scalar field and exhibit a non-Schwarzschild behaviour: faster than $1/r$
convergence to Minkowski spacetime at spatial infinity and hence vanishing of
the Komar mass. The metrics are compared with the Kerr metric for various
couplings and angular velocities. Their physical properties are extracted and
show significant deviations from the Kerr case.},
added-at = {2020-01-28T11:41:40.000+0100},
author = {Van Aelst, Karim and Gourgoulhon, Eric and Grandclément, Philippe and Charmousis, Christos},
biburl = {https://www.bibsonomy.org/bibtex/22ee93879d42346f04a497fce140ad5ce/egourgoulhon},
description = {Hairy rotating black holes in cubic Galileon theory},
doi = {10.1088/1361-6382/ab6391},
interhash = {5db7c1a913b1d97571aa011e417166df},
intrahash = {2ee93879d42346f04a497fce140ad5ce},
keywords = {BlackHole Galileon extendedgravity myown rotating},
note = {cite arxiv:1910.08451Comment: 31 pages, 9 figures; v2 minor improvements, added references, minor typos corrected, version published in Classical and Quantum Gravity},
timestamp = {2020-01-28T11:41:40.000+0100},
title = {Hairy rotating black holes in cubic Galileon theory},
url = {http://arxiv.org/abs/1910.08451},
year = 2019
}