2001
DOI: 10.1103/physrevlett.86.1422
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Gravitationally Bound Monopoles

Abstract: We construct monopole solutions in SU(2) Einstein-Yang-Mills-Higgs theory carrying magnetic charge n. For vanishing and small Higgs self-coupling, these multimonopole solutions are gravitationally bound. Their mass per unit charge is lower than the mass of the n = 1 monopole. For large Higgs self-coupling only a repulsive phase exists.

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Cited by 46 publications
(91 citation statements)
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“…While in flat space SU(2) monopoles as well as SU (5) monopoles -as was demonstrated by us in this paper -are either repelling or non-interacting (in the BPS limit), it was shown in the SU(2) case [12] that gravity is able to overcome the repulsion for sufficiently small Higgs boson masses. We thus limit our analysis of axially symmetric SU(5) monopoles to this important point.…”
Section: B Axially Symmetric Solutionsmentioning
confidence: 84%
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“…While in flat space SU(2) monopoles as well as SU (5) monopoles -as was demonstrated by us in this paper -are either repelling or non-interacting (in the BPS limit), it was shown in the SU(2) case [12] that gravity is able to overcome the repulsion for sufficiently small Higgs boson masses. We thus limit our analysis of axially symmetric SU(5) monopoles to this important point.…”
Section: B Axially Symmetric Solutionsmentioning
confidence: 84%
“…These latter result from the regularity of the solutions at the horizon and a suitable gauge condition [12]. In order to have asymptotically flat, finite energy solutions the bcs at infinity (r = ∞) read:…”
Section: The Modelmentioning
confidence: 99%
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“…For monopoles and dyons, in the case of vanishing Higgs potential, this second branch reaches a critical value of α, where it bifurcates with the branch of extremal Reissner-Nordström black holes with the same charge(s) [7,16,17]. 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.…”
Section: Introductionmentioning
confidence: 99%
“…When gravity is coupled to Yang-Mills-Higgs theory, gravitating monopoles [16,17], dyons [18], monopoleantimonopole pairs [19,20,21,22], and further configurations arise [23]. These solutions depend on a dimensionless coupling constant α, which is proportional to the square root of Newton's constant and the Higgs vacuum expectation value.…”
Section: Introductionmentioning
confidence: 99%