МULTIDIMENSIONAL GLOBAL MONOPOLE AND NONSINGULAR COSMOLOGY

We consider a spherically symmetric global monopole in general relativity in (D = d + 2)-dimensional space-time. For γ < d - 1, where 7 is a parameter characterizing the gravitational field strength, the monopole is shown to be asymptotically flat up to a solid angle defect. In the range d - 1 < γ < 2d(d + 1)/(d + 2), the monopole space-time contains a cosmological horizon. Outside the horizon, the metric corresponds to a cosmo-logical model of the Kantowski-Sachs type, where spatial sections have the topology R x Sd. In the important case where the horizon is far from the monopole core, the temporal evolution of the Kantowski-Sachs metric is described analytically. The Kantowski-Sachs space-time contains a subspace with a (d + 1)-dimensional Friedmann-Robertson-Walker metric, whose possible cosmological application is discussed. Some estimates in the d = 3 case show that this class of nonsingular cosmologies can be viable. In particular, the symmetry-breaking potential at late times can give rise to both dark matter and dark energy. Other results, generalizing those known in the 4-dimensional space-time, are derived, in particular, the existence of a large class of singular solutions with multiple zeros of the Higgs field magnitude.

Authors
Bronnikov K.A. 1 , Meierovich2
Publisher
MEZHDUNARODNAYA KNIGA / Федеральное государственное бюджетное учреждение "Российская академия наук"
Number of issue
1
Language
English
Pages
5-13
Status
Published
Volume
124
Year
2003
Organizations
  • 1 Center for Gravitation and Fundamental Metrology, Russian Research Institute for Metrological Service; Institute of Gravitation and Cosmology, Peoples Friendship University of Russia
  • 2 Kapitza Institute for Physical Problems, Russian Academy of Sciences
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