Standard model Higgs field and hidden sector cosmology

作者: Tommi Tenkanen

DOI: 10.1103/PHYSREVD.100.083515

关键词:

摘要: We consider scenarios where the inflaton field decays dominantly to a hidden dark matter (DM) sector. By studying typical behavior of Standard Model (SM) Higgs during inflation, we derive relation between primordial tensor-to-scalar ratio $r$ and amplitude residual DM isocurvature perturbations $\beta$ which is typically generated if thermally decoupled from SM different expansion histories find that Universe was radiation- or matter-dominated after future discovery will rule out all simple this type because generating observable not possible without violating bounds on $r$. Seen another way, generically threat models both reside in However, necessarily case for an early kination-dominated epoch, as then can source sizeable $\beta$. also discuss why cannot observed curvature perturbation at large scales any above cases but how still be dominant small scales.

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