Pauli blocking effects in thermalization of relativistic plasma

• Published in: Physics letters. A 2020-09, Vol.384 (27), p.126679, Article 126679
• Main Authors: Prakapenia, M.A., Vereshchagin, G.V.
• Format: Article
• Language: English
• Subjects: Binary interactions; Collision integral; Relativistic plasma; Triple interactions; Uehling-Uhlenbeck equations
• ISSN: 0375-9601; 1873-2429
• DOI: 10.1016/j.physleta.2020.126679

•The effects of Pauli blocking on thermalization process of relativistic plasma are studied.•Conditions for strong Pauli blocking are identified and simulations in wide range of parameters are presented.•Avalanche-like thermalization process is identified as a footprint of strongly degenerate plasma. We investigate the effects of Pauli blocking on thermalization process of relativistic plasma by solving relativistic Uehling-Uhlenbeck equations with QED collision integral for all binary and triple processes. With this purpose we consider nonequilibrium initial state of plasma to be strongly degenerate. We found that when electron-positron annihilation is efficient, initial plasma degeneracy is quickly destroyed. As a result in a wide range of final temperatures ranging from nonrelativistic to mildly relativistic 0.1mec2≤kBT≤10mec2 thermalization is not affected by Pauli blocking. Conversely, when electron-positron annihilation process is inefficient, thermalization process in such degenerate plasma is strongly affected by Pauli blocking. This is possible either in a nonrelativistic plasma, with equilibrium temperature kBT≤0.3mec2, or in photon-electron plasma. In these cases all reaction rates are strongly suppressed by Pauli blocking and thermalization does not occur until electrons can populate energy states above the Fermi energy. Soon after this happens thermalization proceeds suddenly in an avalanche-like process. Such rapid thermalization can be a unique footprint of strongly degenerate plasma.