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2013

No-Scale Ripple Inflation Revisited

Li, Tianjun, Li, Zhijin, Nanopoulos, Dimitri V.

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We revisit the no-scale ripple inflation model, where no-scale supergravity is modified by an additional term for the inflaton field in the Kahler potential.

This term not only breaks one SU(N,1) symmetry explicitly, but also plays an important role for inflation.
We generalize the superpotential in the no-scale ripple inflation model slightly.
There exists a discrete Z_2 symmetry/parity in the scalar potential in general, which can be preserved or violated by the non-canonical nomalized inflaton kinetic term.

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