کد مقاله | کد نشریه | سال انتشار | مقاله انگلیسی | نسخه تمام متن |
---|---|---|---|---|
1848800 | 1528811 | 2015 | 7 صفحه PDF | دانلود رایگان |
We investigate the chaotic inflationary model using the two-loop effective potential of a self-interacting scalar field theory in curved spacetime. We use the potential which contains a non-minimal scalar curvature coupling and a quartic scalar self-interaction and which was found in Ref. [1]. We analyze the Lyapunov stability of de Sitter solution and show the stability bound. Calculating the inflationary parameters, we systematically explore the spectral index nsns and the tensor-to-scalar ratio r , with varying the four parameters, the scalar-curvature coupling ξ0ξ0, the scalar quartic coupling λ0λ0, the renormalization scale μ and the e-folding number N . It is found that the two-loop correction on nsns is much larger than the leading-log correction, which has previously been studied in Ref. [2]. We show that the model is consistent with the observation by Planck with WMAP [3] and [4] and a recent joint analysis of BICEP2 [5].
Journal: Physics Letters B - Volume 745, 18 May 2015, Pages 105–111