A class of inflation models with non-minimal coupling
classification
✦ hep-ph
keywords
couplingchosenclassconditionconstantcosmologicaleinsteinfield
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We show that the potential of the scalar field in the Einstein frame is flat if the nonminimal coupling term is properly chosen that it satisfies the condition (V(phi)/K^2(phi)-> constant) as phi gets large. The cosmological implication of this theory is studied.
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