WARM-POLYTROPIC INFLATIONARY UNIVERSE MODEL
2013 ◽
Vol 22
(08)
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pp. 1350041
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In this paper, we study warm inflationary universe models in the context of a polytropic gas. We derive the characteristics of this model in slow-roll approximation and develop our model in two cases: (1) for a constant dissipative parameter Γ; (2) Γ as a function of scalar field ϕ. In these cases, we will obtain exact solution for the scalar field and Hubble parameter. We will also obtain explicit expressions for the tensor-scalar ratio R, scalar spectrum index ns and its running αs in slow-roll approximation.
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1990 ◽
Vol 05
(28)
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pp. 2311-2317
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2017 ◽
Vol 26
(04)
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pp. 1750030
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1992 ◽
Vol 07
(09)
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pp. 2033-2044
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2018 ◽
Vol 15
(10)
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pp. 1850167
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2005 ◽
Vol 14
(05)
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pp. 861-872
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2012 ◽
Vol 27
(18)
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pp. 1250101
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