Non-Abelian Black Holes in Higher Derivative Gravity

Chin. Phys. Lett.

1999, Vol. 16

Issue (3): 164-166 DOI:

Original Articles

Non-Abelian Black Holes in Higher Derivative Gravity

DENG Chang-xue¹;HUANG Chao-guang^1,2

¹Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100039 ²Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing 100080

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DENG Chang-xue, HUANG Chao-guang 1999 Chin. Phys. Lett. 16 164-166

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Abstract The static spherically symmetric black hole solutions in R+αR² gravity coupled to a massive Yang-Mills field, namely, a Proca field are studied. Through the numerical integrations, it is shown that for positive α, there exist two distinct classes of solutions which have the horizon. One class approaches the Schwarzschild solution and the other may be interpreted as black holes with the new hair due to the αR² term.

Keywords: 04.70.Bw 97.60.Lf

Published: 01 March 1999

PACS:	04.70.Bw	(Classical black holes)
	97.60.Lf	(Black holes)

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https://cpl.iphy.ac.cn/ OR https://cpl.iphy.ac.cn/Y1999/V16/I3/0164

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