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arXiv · 1702.07345

Warm Modified Chaplygin Gas Shaft Inflation

Abdul Jawad·Amara Ilyas·Shamaila Rani
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Abstract

In this paper, we examine the possible realization of a new family of inflation called "shaft inflation" by assuming the modified Chaplygin gas model and tachyon scalar field. We also consider the special form of dissipative coefficient as $Γ={a_0}\frac{T^{3}}{ϕ^{2 }}$ and calculate the various inflationary parameters in the scenario of strong and weak dissipative regimes. In order to examine the behavior of inflationary parameters, the planes of $n_s - ϕ,~n_s - r$ and $n_s - α_s$ (where $n_s,~α_s,~r$ and $ϕ$ represent spectral index, its running, tensor to scalar ratio and scalar field respectively) are being developed which lead to the constraints: $r< 0.11$, $n_s=0.96\pm0.025$ and $α_s =-0.019\pm0.025$. It is quite interesting that these results of inflationary parameters are compatible with BICEP$2$, WMAP $(7+9)$ and recent Planck data.

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Abdul Jawad, Amara Ilyas, Shamaila Rani. 2017-02-23. Warm Modified Chaplygin Gas Shaft Inflation. https://doi.org/10.1140/epjc%2Fs10052-017-4691-2

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