arXiv · astro-ph/9804090
Finite Temperature effects on baryon transport scattering in the early Universe
Abstract
We have computed finite temperature corrections to the electron-hadron scattering cross sections. These are based upon the renormalized electron mass and the modified density of states due to the presence of a background thermal bath. It is found that the electron-hadron thermal transport scattering cross section can be much larger than the zero temperature one. In the case of electron-neutron transport scattering, we find σ_{ne}(T) / σ_{ne} (T=0) \simeq 5 at T \simeq 0.1 MeV.
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In-Saeng Suh, G. J. Mathews. 1998-04-08. Finite Temperature effects on baryon transport scattering in the early Universe. https://doi.org/10.1103/physrevd.58.025001
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