### Abstract

Numerical evidence is presented for the existence of a new family of static, globally regular 'cosmological' solutions of the spherically symmetric Einstein-Yang-Mills-Higgs equations. These solutions are characterized by two natural numbers (m ≥ 1, n ≥ 0), the number of nodes of the Yang-Mills and Higgs field respectively. The corresponding spacetimes are static with spatially compact sections with 3-sphere topology. (C) 2000 Published by Elsevier Science B.V.

Original language | English |
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Pages (from-to) | 397-402 |

Number of pages | 6 |

Journal | Physics Letters B |

Volume | 489 |

Issue number | 3-4 |

DOIs | |

Publication status | Published - Sep 21 2000 |

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### ASJC Scopus subject areas

- Nuclear and High Energy Physics

### Cite this

*Physics Letters B*,

*489*(3-4), 397-402. https://doi.org/10.1016/S0370-2693(00)00931-X

**Static cosmological solutions of the Einstein-Yang-Mills-Higgs equations.** / Breitenlohner, P.; Forgács, P.; Maison, D.

Research output: Contribution to journal › Article

*Physics Letters B*, vol. 489, no. 3-4, pp. 397-402. https://doi.org/10.1016/S0370-2693(00)00931-X

}

TY - JOUR

T1 - Static cosmological solutions of the Einstein-Yang-Mills-Higgs equations

AU - Breitenlohner, P.

AU - Forgács, P.

AU - Maison, D.

PY - 2000/9/21

Y1 - 2000/9/21

N2 - Numerical evidence is presented for the existence of a new family of static, globally regular 'cosmological' solutions of the spherically symmetric Einstein-Yang-Mills-Higgs equations. These solutions are characterized by two natural numbers (m ≥ 1, n ≥ 0), the number of nodes of the Yang-Mills and Higgs field respectively. The corresponding spacetimes are static with spatially compact sections with 3-sphere topology. (C) 2000 Published by Elsevier Science B.V.

AB - Numerical evidence is presented for the existence of a new family of static, globally regular 'cosmological' solutions of the spherically symmetric Einstein-Yang-Mills-Higgs equations. These solutions are characterized by two natural numbers (m ≥ 1, n ≥ 0), the number of nodes of the Yang-Mills and Higgs field respectively. The corresponding spacetimes are static with spatially compact sections with 3-sphere topology. (C) 2000 Published by Elsevier Science B.V.

UR - http://www.scopus.com/inward/record.url?scp=0034699362&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=0034699362&partnerID=8YFLogxK

U2 - 10.1016/S0370-2693(00)00931-X

DO - 10.1016/S0370-2693(00)00931-X

M3 - Article

AN - SCOPUS:0034699362

VL - 489

SP - 397

EP - 402

JO - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics

JF - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics

SN - 0370-2693

IS - 3-4

ER -