Is there a big-bubble problem in extended inflation\?

Physics

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Particle-Theory And Field-Theory Models Of The Early Universe, Gravity In More Than Four Dimensions, Kaluza-Klein Theory, Unified Field Theories, Alternative Theories Of Gravity

Scientific paper

We present a generalization of the thin-wall formalism to calculate the evolution of true-vacuum bubbles in ``extended'' inflaton. For inflation quartic couplings of the order M/MPl, gravity will lead to the recollapse of bubbles during most of the extended-inflation period thereby altering the bubble size distribution. The completion of the phase transition will proceed through tiny bubbles satisfying homogeneity constraints of the microwave background for arbitrary values of ω. Thus, it is possible to construct models that agree with experiments even for the original version of extended inflation.

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