Beyond y and \mu: the shape of the CMB spectral distortions in the intermediate epoch, 1.5x10^4 < z < 2x10^5
Rishi Khatri, Rashid A. Sunyaev

TL;DR
This paper models intermediate CMB spectral distortions caused by energy injections at redshifts 1.5x10^4 to 2x10^5, revealing their unique features and potential to distinguish different early Universe processes.
Contribution
It provides numerical solutions, analytic approximations, and publicly available software for intermediate spectral distortions, enhancing understanding beyond pure y and bc-type distortions.
Findings
Intermediate distortions contain richer information than pure y and bc-type distortions.
Spectral shape depends sensitively on redshift of energy injection.
Intermediate distortions cannot be replicated by mixtures of y and bc-type distortions.
Abstract
We calculate numerical solutions and analytic approximations for the intermediate-type spectral distortions. Detection of a \mu-type distortion (saturated comptonization) in the CMB will constrain the time of energy injection to be at a redshift 2x10^6> z > 2x10^5, while a detection of a y-type distortion (minimal comptonization) will mean that there was heating of CMB at redshift z< 1.5x10^4. We point out that the partially comptonized spectral distortions, generated in the redshift range 1.5x10^4 < z x 2x10^5, are much richer in information than the pure y and \mu-type distortions. The spectrum created during this period is intermediate between y and \mu-type distortions and depends sensitively on the redshift of energy injection. These intermediate-type distortions cannot be mimicked by a mixture of y and \mu-type distortions at all frequencies and vice versa. The measurement of…
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