Mixing of blackbodies: entropy production and dissipation of sound waves in the early Universe
Rishi Khatri, Rashid A. Sunyaev, Jens Chluba

TL;DR
This paper investigates how mixing blackbody spectra in the early Universe due to sound wave dissipation causes spectral distortions and entropy production, providing a thermodynamic perspective on these processes.
Contribution
It offers a simplified thermodynamic framework to understand spectral distortions and entropy creation from sound wave dissipation in the early Universe.
Findings
2/3 of dissipated energy increases average temperature
1/3 of energy creates y-type spectral distortion
Mixing of blackbodies leads to entropy production
Abstract
Mixing of blackbodies with different temperatures creates a spectral distortion which, at lowest order, is a y-type distortion, indistinguishable from the thermal y-type distortion produced by the scattering of CMB photons by hot electrons residing in clusters of galaxies. This process occurs in the radiation-pressure dominated early Universe, when the primordial perturbations excite standing sound waves on entering the sound horizon. Photons from different phases of the sound waves, having different temperatures, diffuse through the electron-baryon plasma and mix together. This diffusion, with the length defined by Thomson scattering, dissipates sound waves and creates spectral distortions in the CMB. Of the total dissipated energy, 2/3 raises the average temperature of the blackbody part of spectrum, while 1/3 creates a distortion of y-type. It is well known that at redshifts 10^5< z<…
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