6533b85afe1ef96bd12ba04c
RESEARCH PRODUCT
CMB spectral distortions in generic two-field models
Kimmo KainulainenKimmo KainulainenJuuso LeskinenJuuso LeskinenSami NurmiSami NurmiTomo Takahashisubject
Cosmology and Nongalactic Astrophysics (astro-ph.CO)Field (physics)ART. NO. 023505Cosmic microwave backgroundFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics114 Physical sciences01 natural sciencesCosmologyHigh Energy Physics - Phenomenology (hep-ph)EARLY UNIVERSEDistortion0103 physical sciencesphysics of the early universeENERGY-RELEASEStatistical physicsSensitivity (control systems)inflation010303 astronomy & astrophysicsPhysicsInflation (cosmology)010308 nuclear & particles physicscosmological parameters from CMBRCURVATURE PERTURBATIONCONSTRAINTSAstronomy and AstrophysicsFunction (mathematics)115 Astronomy Space scienceMIXED INFLATONHigh Energy Physics - PhenomenologyDENSITY PERTURBATIONSAmplitudeCOSMOLOGYRADIATIONAstrophysics - Cosmology and Nongalactic AstrophysicsGENERATIONdescription
We investigate the CMB $\mu$ 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 $\mu$ distortion could efficiently break degeneracies of curvaton parameters especially when combined with future sensitivity of probing the tensor-to-scalar ratio $r$. For example, assuming bounds $\mu < 0.5 \times 10^{-8}$ and $r<0.01$, the curvaton contribution should either vanish or the curvaton should dominate primordial perturbations and its slow-roll parameter $\eta_{\chi}$ is constrained to the interval $-0.007 < \eta_{\chi}< 0.045$.
year | journal | country | edition | language |
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2017-07-05 | Journal of Cosmology and Astroparticle Physics |