2008
DOI: 10.1088/1475-7516/2008/12/005
|View full text |Cite
|
Sign up to set email alerts
|

Black hole solutions in Einstein–Maxwell–Yang–Mills–Gauss–Bonnet theory

Abstract: We consider Maxwell and Yang-Mills (YM) fields together, interacting through gravity both in Einstein and Gauss-Bonnet (GB) theories. For this purpose we choose two different sets of Maxwell and metric ansaetze. In our first ansatz, asymptotically for r → 0 (and N > 4) the Maxwell field dominates over the YM field. In the other asymptotic region, r → ∞, however, the YM field becomes dominates. For N = 3 and N = 4, where the GB term is absent, we recover the well-known Bañados-Teitelboim-Zanelli (BTZ) and Reiss… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1
1

Citation Types

1
37
0

Year Published

2008
2008
2024
2024

Publication Types

Select...
9

Relationship

0
9

Authors

Journals

citations
Cited by 35 publications
(38 citation statements)
references
References 24 publications
1
37
0
Order By: Relevance
“…Nevertheless, Yasskin found the first analytic black hole solutions by using Wu-Yang ansatz [84]. Then, the black hole solutions in YM theory have been generalized to Gauss-Bonnet and Lovelock gravity in [85,86] and [87,88], respectively. In addition, black holes have been investigated in non-abelian generalization of BI NED in Einstein gravity [89] and regular black holes have been obtained in [90][91][92][93].…”
Section: Jhep10(2019)207mentioning
confidence: 99%
“…Nevertheless, Yasskin found the first analytic black hole solutions by using Wu-Yang ansatz [84]. Then, the black hole solutions in YM theory have been generalized to Gauss-Bonnet and Lovelock gravity in [85,86] and [87,88], respectively. In addition, black holes have been investigated in non-abelian generalization of BI NED in Einstein gravity [89] and regular black holes have been obtained in [90][91][92][93].…”
Section: Jhep10(2019)207mentioning
confidence: 99%
“…; 3 are spacetime indices, and ¼ 1, 2, 3 are isospace indices). The standard EH action for fðRÞ-YM theory becomes [41][42][43] …”
Section: B 4d-fðrþ Yang-mills Solutionsmentioning
confidence: 99%
“…Note that the metric (25) is conformally flat when C 0 g 2 0 = 1, which was also observed in [13]. We will not be interested in this solution.…”
Section: The Solutions and Their Propertiesmentioning
confidence: 63%