Abstract
Recent studies have indicated that in a certain critical coupling phase the Einstein-matter-gauge equations may be reduced to a Bogomol'nyi-Einstein system and the solutions are cosmic strings with finite separation. In this paper, we view the spacetime as known and treat the dynamics as being determined by the matter-gauge sector in an asymptotically Euclidean geometry. It is shown that the model admits a continuous family of infinite energy solutions which decay to the symmetric vacuum faster than any exponential functions.
Original language | English (US) |
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Pages (from-to) | 301-315 |
Number of pages | 15 |
Journal | Proceedings of the Royal Society of Edinburgh: Section A Mathematics |
Volume | 122 |
Issue number | 3-4 |
DOIs | |
State | Published - 1992 |
ASJC Scopus subject areas
- General Mathematics