| THE PHYSICS OF ELEMENTARY PARTICLES AND FIELDS |
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Cosmic String Universes Embedded with Viscosity |
| Koijam Manihar Singh1*, Kangujam Priyokumar Singh2**
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1Department of Mathematics, Sambalpur University, Orissa-768019, India
2Department of Mathematics IGC, Akampat, Imphal-795001, (Manipur University), India
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| Cite this article: |
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Koijam Manihar Singh, Kangujam Priyokumar Singh 2011 Chin. Phys. Lett. 28 101102 |
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Abstract We study string cosmological models with attached particles in LRS BI type space time. The dynamical and physical properties of such universes are studied, and the possibility that during the evolution of the universe the strings disappear, leaving only the particles, is also discussed. It is found that bulk viscosity plays a large role in the evolution of the universe. In these models we find critical instances of when there was a "Bounce". The studied models are found to be of an inflationary type, and since a desirable feature of a meaningful string cosmological model is the presence of an inflationary epoch in the very early stages of evolution, our models can be thought of as realistic universes.
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| Keywords:
11.27.+d
98.80.Cq
98.80.-k
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Received: 29 January 2011
Published: 28 September 2011
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| PACS: |
11.27.+d
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(Extended classical solutions; cosmic strings, domain walls, texture)
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98.80.Cq
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(Particle-theory and field-theory models of the early Universe (including cosmic pancakes, cosmic strings, chaotic phenomena, inflationary universe, etc.))
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98.80.-k
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(Cosmology)
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