1110.2462 (Yuki Watanabe)
Yuki Watanabe
We compute the super-Hubble evolution of non-Gaussianity of primordial
curvature perturbations in two-field inflation models by employing two
formalisms: delta N and covariant formalisms. Although two formalisms treat the
evolution of fluctuations radically different, we show that the formulas of
f_{NL} parameter agree quantitatively with each other within 1 % accuracy. We
find that the amplitude of f_{NL} decays no faster than a^{-3} as the
inflationary trajectory reaches to the adiabatic limit.
View original:
http://arxiv.org/abs/1110.2462
No comments:
Post a Comment