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Long-Wavelength Modes of Cosmological Scalar Fields

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abstract

We give a numerical analysis of long-wavelength modes in the WKB approximation of cosmological scalar fields coupled to gravity via $\xi\phi^{2}R$. Massless fields are coupled conformally at $\xi=1/6$. Conformality can be preserved for fields of nonzero mass by shifting $\xi$. We discuss implications for density perturbations.

fields

gr-qc 1

years

2019 1

verdicts

CONDITIONAL 1

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