Constraining supergravity inflation with non-minimal Kähler operators using formalism
arXiv:1402.1251 · doi:10.1007/JHEP04(2014)105
Abstract
In this paper I provide a general framework based on formalism to study the features of unavoidable higher dimensional non-renormalizable Kähler operators for supergravity (SUGRA) during primordial inflation from the combined constraint on non-Gaussianity, sound speed and CMB dipolar asymmetry as obtained from the recent Planck data. In particular I study the nonlinear evolution of cosmological perturbations on large scales which enables us to compute the curvature perturbation, , without solving the exact perturbed field equations. Further I compute the non-Gaussian parameters , and for local type of non-Gaussianities and CMB dipolar asymmetry parameter, , using the formalism for a generic class of sub-Planckian models induced by the Hubble-induced corrections for a minimal supersymmetric D-flat direction where inflation occurs at the point of inflection within the visible sector. Hence by using multi parameter scan I constrain the non-minimal couplings appearing in non-renormalizable Kähler operators within, , for the speed of sound, , and tensor to scalar, . Finally applying all of these constraints I will fix the lower as well as the upper bound of the non-Gaussian parameters within, , and , and CMB dipolar asymmetry parameter within the range, .
arXiv comment26 pages, 5 figures, Accepted for publication in JHEP
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