arXiv · hep-ph/0510009
Long-Wavelength Modes of Cosmological Scalar Fields
Abstract
We give a numerical analysis of long-wavelength modes in the WKB approximation of cosmological scalar fields coupled to gravity via $ξϕ^{2}R$. Massless fields are coupled conformally at $ξ=1/6$. Conformality can be preserved for fields of nonzero mass by shifting $ξ$. We discuss implications for density perturbations.
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Marcin Jankiewicz, Thomas W. Kephart. 2005-10-18. Long-Wavelength Modes of Cosmological Scalar Fields. https://doi.org/10.1103/physrevd.73.123514
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