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Phase Transitions and Magnetic Monopole Production in the Very Early Universe
Open accessAbstract
In grand unified models, the abundance of superheavy magnetic monopoles in the universe can be suppressed if (1) the phase transition which creates the monopoles occurs after much supercooling; and (2) immediately after the phase transition, the effective monopole mass is large compared with the temperature. These requirements impose constraints on the history of the early universe. The Georgi-Glashow SU(5) group probably breaks to SU(4) \ensuremath{\bigotimes} U(1) before it reaches SU(3) \ensuremath{\bigotimes} SU(2) \ensuremath{\bigotimes} U(1).
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Citations
Cited by
Inflationary universe: A possible solution to the horizon and flatness problems
Guth, A. H. (1981) · Physical Review D · doi:10.1103/physrevd.23.347 · Cited by 9,983
Self-citationCosmology for Grand Unified Theories with Radiatively Induced Symmetry Breaking
Albrecht, A., & Steinhardt, P. J. (1982) · Physical Review Letters · doi:10.1103/physrevlett.48.1220 · Cited by 4,981
Gauge-invariant cosmological perturbations
Bardeen, J. M. (1980) · Physical Review D · doi:10.1103/physrevd.22.1882 · Cited by 2,393
Supercooled phase transitions in the very early universe
Hawking, S. W., & Moss, I. L. (1982) · Physics Letters B · doi:10.1016/0370-2693(82)90946-7 · Cited by 816
Could the universe have recovered from a slow first-order phase transition?
Guth, A. H., & Weinberg, E. J. (1983) · Nuclear Physics B · doi:10.1016/0550-3213(83)90307-3 · Cited by 576
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Metadata
- Authors
- Guth, A. H., & Tye, S. H. H.
- Venue
- Physical Review Letters
- Publisher
- American Physical Society (APS)
- Published
- 1980-03-10
- Volume
- 44
- Issue
- 10
- Pages
- 631-635
- ISSN
- 0031-9007 (ISSN-L)
- OpenAlex
- W2055148549
- Cited by
- 320
- References
- 0
- FWCI
- 31.80
- Type
- journal article
- Language
- en
- Open access
- green
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