Circular Geodesics Stability in a Static Black Hole in New Massive Gravity
Keyword(s):
We study the existence and stability of circular geodesics in a family of asymptotically AdS static black holes in New Massive Gravity theory. We show that the mathematical sign of the hair parameter determines the existence of such geodesics. For a positive hair parameter, the stability regions follow the usual pattern, with the innermost geodesic being null, unstable, and separated from the horizon, followed by a region of unstable timelike geodesics and then a region of stable timelike geodesics, which extends in the asymptotic region.
2003 ◽
Vol 12
(01)
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pp. 121-127
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2019 ◽
Vol 28
(09)
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pp. 1950113
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2020 ◽
Vol 29
(03)
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pp. 2050025
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2019 ◽
Vol 28
(12)
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pp. 1950160
2020 ◽
Vol 29
(12)
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pp. 2050081
1998 ◽
Vol 13
(03)
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pp. 239-252
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2015 ◽
Vol 24
(03)
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pp. 1550022
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2014 ◽
Vol 2014
(2)
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pp. 23E02-0
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Keyword(s):