2005
DOI: 10.1016/j.physletb.2005.01.038
|View full text |Cite
|
Sign up to set email alerts
|

New regular solutions with axial symmetry in Einstein–Yang–Mills theory

Abstract: We construct new regular solutions in Einstein-Yang-Mills theory. They are static, axially symmetric and asymptotically flat. They are characterized by a pair of integers (k, n), where k is related to the polar angle and n to the azimuthal angle. The known spherically and axially symmetric EYM solutions have k = 1. For k > 1 new solutions arise, which form two branches. They exist above a minimal value of n, that increases with k. The solutions on the lower mass branch are related to certain solutions of Einst… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1

Citation Types

0
61
0

Year Published

2005
2005
2017
2017

Publication Types

Select...
5
2
1

Relationship

5
3

Authors

Journals

citations
Cited by 31 publications
(61 citation statements)
references
References 29 publications
0
61
0
Order By: Relevance
“…Our solutions are akin to the static, axially symmetric EYM configurations in d = 4, studied exhaustively in [26], [27,28]. The regular and black hole solutions presented are natural generalisations of the known [10] d = 5 EYM spherically symmetric globally regular and black hole solutions.…”
Section: Discussionmentioning
confidence: 89%
See 1 more Smart Citation
“…Our solutions are akin to the static, axially symmetric EYM configurations in d = 4, studied exhaustively in [26], [27,28]. The regular and black hole solutions presented are natural generalisations of the known [10] d = 5 EYM spherically symmetric globally regular and black hole solutions.…”
Section: Discussionmentioning
confidence: 89%
“…As compared to the d = 4 case [27,28], we expect the existence of a much richer set of nonspherically symmetric EYM solutions in d = 5.…”
Section: Discussionmentioning
confidence: 95%
“…There a backbending in α is observed, with the occurrence of the second branch of solutions. With decreasing α, the solutions smoothly reach the corresponding (generalized) Bartnik-McKinnon solutions 8,25,52 in the limit α → 0. Along this branch, the mass of the (m, n) configurations is higher than the mass of the corresponding solution on the branch linked to the global AdS space.…”
mentioning
confidence: 91%
“…Also, despite the generic presence of a net magnetic flux, they can be viewed as the natural AdS generalizations of the asymptotically flat EYM solitons in 24 . However, as discussed in 25 , the EYM system with Λ = 0 possesses a variety of other globally regular solutions, describing composite configurations, with several constituents b . In the notation of 25 , these solutions are characterized by a pair of positive integers (m, n), where m is related to the polar angle and n to the azimuthal angle.…”
mentioning
confidence: 99%
“…For monopole-antimonopole pair solutions and other composite solutions, in contrast, the second branch extends back to α = 0, where a pure Einstein-Yang-Mills solution is reached (after scaling w.r.t. α) [24,25,26,27].…”
Section: Introductionmentioning
confidence: 99%