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Cardoso, V., Dias, O.J.C. & Rocha, Jorge V. (2010). Phase diagram for non-axisymmetric plasma balls. Journal of High Energy Physics.

C. V. et al.,  "Phase diagram for non-axisymmetric plasma balls", in Journal of High Energy Physics, 2010

@article{v.2010_1732210541516,
	author = "Cardoso, V. and Dias, O.J.C. and Rocha, Jorge V.",
	title = "Phase diagram for non-axisymmetric plasma balls",
	journal = "Journal of High Energy Physics",
	year = "2010",
	volume = "",
	number = "",
	doi = "10.1007/JHEP01(2010)021",
	url = "https://link.springer.com/article/10.1007%2FJHEP01%282010%29021"
}

TY  - JOUR
TI  - Phase diagram for non-axisymmetric plasma balls
T2  - Journal of High Energy Physics
AU  - Cardoso, V.
AU  - Dias, O.J.C.
AU  - Rocha, Jorge V.
PY  - 2010
SN  - 1126-6708
DO  - 10.1007/JHEP01(2010)021
UR  - https://link.springer.com/article/10.1007%2FJHEP01%282010%29021
AB  - Plasma balls and rings emerge as fluid holographic duals of black holes and black rings in the hydrodynamic/gravity correspondence for the Scherk-Schwarz AdS system. Recently, plasma balls spinning above a critical rotation were found to be unstable against m-lobed perturbations. In the phase diagram of stationary solutions the threshold of the instability signals a bifurcation to a new phase of non-axisymmetric configurations. We find explicitly this family of solutions and represent them in the phase diagram. We discuss the implications of our results for the gravitational system. Rotating non-axisymmetric black holes necessarily radiate gravitational waves. We thus emphasize that it would be important, albeit possibly out of present reach, to have a better understanding of the hydrodynamic description of gravitational waves and of the gravitational interaction between two bodies. We also argue that it might well be that a non-axisymmetric m-lobed instability is also present in Myers-Perry black holes for rotations below the recently found ultraspinning instability.
ER  -