Constraints on μ-distortion fluctuations and primordial non-Gaussianity from Planck data
- Max Planck Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85741, Garching (Germany)
We use the Planck HFI channel maps to make an all sky map of μ-distortion fluctuations. Our μ-type distortion map is dominated by the y-type distortion contamination from the hot gas in the low redshift Universe and we can thus only place upper limits on the μ-type distortion fluctuations. For the amplitude of μ-type distortions on 10' scales we get the limit on root mean square (rms) value μ{sub rms}{sup 10'}< 6.4× 10{sup −6}, a limit 14 times stronger than the COBE-FIRAS (95% confidence) limit on the mean of ( μ )<90× 10{sup −6}. Using our maps we also place strong upper limits on the auto angular power spectrum of μ, C{sub ℓ}{sup μμ} and the cross angular power spectrum of μ with the CMB temperature anisotropies, C{sub ℓ}{sup μ T}. The strongest observational limits are on the largest scales, ℓ(ℓ+1)/(2π)C{sub ℓ}{sup μμ}|{sub ℓ=2−26}<(2.3± 1.0)× 10{sup −12} and ℓ(ℓ+1)/(2π)C{sub ℓ}{sup μ T}|{sub ℓ=2−26}<(2.6± 2.6)× 10{sup −12} K. Our observational limits can be used to constrain new physics which can create spatially varying energy release in the early Universe between redshifts 5× 10{sup 4∼<} z∼< 2× 10{sup 6}. We specifically apply our observational results to constrain the primordial non-Gaussianity of the local type, when the source of μ-distortion is Silk damping, for very squeezed configurations with the wavenumber for the short wavelength mode 46 ∼< k{sub S} ∼< 10{sup 4} Mpc{sup −1} and for the long wavelength mode k{sub L}≈ 10{sup −3} Mpc{sup −1}. Our limits on the primordial non-Gaussianity parameters are f{sub NL}<10{sup 5}, τ{sub NL}<1.4× 10{sup 11} for k{sub S}/k{sub L}≈ 5× 10{sup 4}− 10{sup 7}. We also give a new derivation of the evolution of the μ-distortion fluctuations through the y-distortion era and the recombination epoch until today resulting in very simple expressions for the cross and auto power spectra in the squeezed limit. We also introduce mixing of Bose-Einstein spectra due to Silk damping and y{sup BE}-type distortions. The μ-type distortion map and masks are now publicly available.
- OSTI ID:
- 22525374
- Journal Information:
- Journal of Cosmology and Astroparticle Physics, Vol. 2015, Issue 09; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 1475-7516
- Country of Publication:
- United States
- Language:
- English
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