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作 者:Abdul Jawad Faiza Gulshan Shamaila Rani
机构地区:[1]Department of Mathematics, COMSATS Institute of Information Technology [2]Department of Mathematics, Lahore Leads University
出 处:《Communications in Theoretical Physics》2017年第8期272-284,共13页理论物理通讯(英文版)
摘 要:We discuss the warm inflation in the presence of standard scalar field model and modified Chaplyggin gas in brahe-world scenario. We consider weak and strong dissipative regimes with generalized dissipative coefficient. We extract various inflationary parameters. For example, we analyze the behavior of different ratios (ratio of dissipative co-efficient and Hubble parameter Г/3H, ratio of temperature and Hubble parameter T/ H, scalar-to-tensor ratio 'r) with respect to spectral index ns for the weak and strong dissipative regimes through parametric plotting. It is found that T/H and Г/3H satisfied the required conditions in both dissipative regimes. It is also noted that the spectral index (ns) ns=0.96+0.10-0.10 It is remarked here that our results are consistence with observational data WMAP7, WMAP9, and recent Planck data.
关 键 词:brane-world model standard scalar field model modified chaplygin gas inflationary parameters
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