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Inflation with multiple sound speeds: a model of multiple DBI type actions and non-Gaussianities

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arxiv 0904.0062 v1 pith:52VQSPQZ submitted 2009-04-01 hep-th astro-ph.COgr-qchep-ph

classification hep-thastro-ph.COgr-qchep-ph
keywords soundperturbationstypemultiplespeedsactionsentropyfield
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In this letter we study adiabatic and isocurvature perturbations in the frame of inflation with multiple sound speeds involved. We suggest this scenario can be realized by a number of generalized scalar fields with arbitrary kinetic forms. These scalars have their own sound speeds respectively, so the propagations of field fluctuations are individual. Specifically, we study a model constructed by two DBI type actions. We find that the critical length scale for the freezing of perturbations corresponds to the maximum sound horizon. Moreover, if the mass term of one field is much lighter than that of the other, the entropy perturbation could be quite large and so may give rise to a growth outside sound horizon. At cubic order, we find that the non-Gaussianity of local type is possibly large when entropy perturbations are able to convert into curvature perturbations. We also calculate the non-Gaussianity of equilateral type approximately.

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  1. Primordial black holes from sound speed resonance in the inflaton-curvaton mixed scenario

    astro-ph.CO 2019-08 conditional novelty 5.0 of 10

    Primordial black holes with a narrow mass spectrum can form from parametric resonance in the curvaton sector of an inflaton-curvaton model, possibly providing a dark matter candidate.

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