English

CMB spectral distortions in generic two-field models

Cosmology and Nongalactic Astrophysics 2017-11-15 v2 High Energy Physics - Phenomenology

Abstract

We investigate the CMB μ\mu distortion in models where two uncorrelated sources contribute to primordial perturbations. We parameterise each source by an amplitude, tilt, running and running of the running. We perform a detailed analysis of the distribution signal as function of the model parameters, highlighting the differences compared to single-source models. As a specific example, we also investigate the mixed inflaton-curvaton scenario. We find that the μ\mu distortion could efficiently break degeneracies of curvaton parameters especially when combined with future sensitivity of probing the tensor-to-scalar ratio rr. For example, assuming bounds μ<0.5×108\mu < 0.5 \times 10^{-8} and r<0.01r<0.01, the curvaton contribution should either vanish or the curvaton should dominate primordial perturbations and its slow-roll parameter ηχ\eta_{\chi} is constrained to the interval 0.007<ηχ<0.045-0.007 < \eta_{\chi}< 0.045.

Keywords

Cite

@article{arxiv.1707.01300,
  title  = {CMB spectral distortions in generic two-field models},
  author = {Kimmo Kainulainen and Juuso Leskinen and Sami Nurmi and Tomo Takahashi},
  journal= {arXiv preprint arXiv:1707.01300},
  year   = {2017}
}

Comments

15 pages, 6 figures. v2: published version, minor changes

R2 v1 2026-06-22T20:38:21.698Z