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We study the slow-roll inflation models, where the inflaton slow-rolls along a trajectory whose orthogonal directions are lifted by potentials with masses of order the Hubble parameter.
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This requires m σ > θ ˙ 0 m_{\sigma}>\dot{\theta}_{0} . The θ ˙ 0 \dot{\theta}_{0} will cause a displacement for the vev, we can redefine the σ \sigma and R R so that σ = 0 \sigma=0 is the effective minimum
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More detailed discussions on the computational advantages and disadvantages of both forms can be found in Ref. [ 11 ]
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E. Komatsu et al
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