We propose a new class of spontaneous baryogenesis models that does not produce baryon isocurvature perturbations. The baryon chemical potential in these models is independent of the field value of the baryon-generating scalar, hence the scalar field fluctuations are blocked from propagating into the baryon isocurvature. We demonstrate this mechanism in simple examples where spontaneous baryogenesis is driven by a non-canonical scalar field. The suppression of the baryon isocurvature allows spontaneous baryogenesis to be compatible even with high-scale inflation. © 2017 IOP Publishing Ltd and Sissa Medialab srl .
Spontaneous baryogenesis without baryon isocurvature
De Simone, Andrea;KOBAYASHI, Takeshi
2017-01-01
Abstract
We propose a new class of spontaneous baryogenesis models that does not produce baryon isocurvature perturbations. The baryon chemical potential in these models is independent of the field value of the baryon-generating scalar, hence the scalar field fluctuations are blocked from propagating into the baryon isocurvature. We demonstrate this mechanism in simple examples where spontaneous baryogenesis is driven by a non-canonical scalar field. The suppression of the baryon isocurvature allows spontaneous baryogenesis to be compatible even with high-scale inflation. © 2017 IOP Publishing Ltd and Sissa Medialab srl .File | Dimensione | Formato | |
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Simone_2017_J._Cosmol._Astropart._Phys._2017_036.pdf
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