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The Very Early Universe

Published online by Cambridge University Press:  25 April 2016

K. Sato

Extract

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In recent years, the research on the very early universe has shown quite remarkable developments. As is well known, this development was brought about by the introduction of the Grand Unified Theories (GUTs) into cosmology. These theories have not only enabled us to trace the evolution of the Universe back to the very early stage at temperatures of 1016 GeV or higher, but also introduced various new aspects into cosmology, such as baryogenesis, phase transitions and topological defects (monopoles, etc.). In particular, inflation, which grew out of the study of GUT phase transition, is the most important and fascinating outcome.

Type
Research Article
Information
Transactions of the International Astronomical Union , Volume 20 , Issue 1 , 1988 , pp. 656 - 658
Copyright
Copyright © Kluwer 1988 

References

1 – See for example: 1986, Inner Space/Outer Space, Chicago Univ. Press.Google Scholar
2 – Linde, A.D.: 1984, Rep. Prog. Phys. 47, pp. 925.CrossRefGoogle Scholar
3 – Turner, M.S. and Widrow, L.M.: 1986, Phys. Rev. Lett. 57, pp. 2237.CrossRefGoogle Scholar
4 – Jensen, L.G. and Stein-Schabes, J.A.: 1987, Phys. Rev. D35, pp. 1046.Google Scholar
5 – Sato, K.: 1987, Proc. of the IAU Symposium 130, “The structure of the Universe”, to be published.Google Scholar
6 – Linde, A.D.: 1986, Phys. Lett. 175B, pp. 395.CrossRefGoogle Scholar
7 – Starobinski, A.: 1983, JETP Lett. 30, pp. 66.Google Scholar
– Stein-Schabes, J.A.: 1987, Phys. Rev. D35, pp. 2345.Google Scholar
– Barrow, J.D. and Gron, O.: 1986, Phys. Lett. 182B, pp. 25.Google Scholar
8 – Steinhardt, P.J. and Turner, M.S.: 1984, Phys. Rev. D29, pp. 2162.CrossRefGoogle Scholar
9 Kuzmin, V.A., Rubakov, V.A. and Shaposhnikov, M.E.: 1985, Phys. Lett. 155B, pp. 36.CrossRefGoogle Scholar
10 – See for example:Google Scholar
Fukugita, M. and Ukawa, A.: 1986, Phys. Rev. Lett. 57, pp. 503.CrossRefGoogle Scholar
Guputa, R., et al.: 1986, Phys. Rev. Lett. 57, pp. 2621.CrossRefGoogle Scholar
Karsch, F., et al.: 1987, Phys. Lett. 188B, pp. 353.CrossRefGoogle Scholar
11 – Witten, E.: 1984, Phys Rev. D30, pp. 272.CrossRefGoogle Scholar
12 – Carr, B.J. and Turner, M.S.: 1987, Mod. Phys. Lett. A2, pp. 1.Google Scholar
13 – Alcock, C. and Farhi, E.: 1985, Phys. Rev. D32, pp. 1273.CrossRefGoogle Scholar
Madsen, J., et al.: 1986, Phys. Rev. D34, pp. 2947.CrossRefGoogle Scholar
14 – Applegate, J.H., Hogan, C.J. and Scherrer, R.J.: 1987, Phys. Rev. D35, pp. 1151.CrossRefGoogle Scholar
15 – Turner, M.S.: 1987, Proc. of the IAU Symp. 130, “The structure of the Universe”, to be published.Google Scholar
16 – See for example: Turok, N.: 1987, Proc. of the IAU Symp. 130, “The structure of the Universe”, to be published.Google Scholar