Finite temperature radiative corrections to neutron decay and related processes

1983 ◽  
Vol 222 (3) ◽  
pp. 517
1982 ◽  
Vol 209 (2) ◽  
pp. 372-388 ◽  
Author(s):  
Jean-Luc Cambier ◽  
Joel R. Primack ◽  
Marc Sher

1958 ◽  
Vol 112 (1) ◽  
pp. 267-270 ◽  
Author(s):  
S. M. Berman

1983 ◽  
Vol 28 (2) ◽  
pp. 340-348 ◽  
Author(s):  
John F. Donoghue ◽  
Barry R. Holstein

1984 ◽  
Vol 29 (12) ◽  
pp. 3004-3004 ◽  
Author(s):  
John F. Donoghue ◽  
Barry R. Holstein

2020 ◽  
Vol 9 (4) ◽  
Author(s):  
Miroslav Pardy ◽  

The totally ionized charged collisionless plasma at finite temperature is considered. Using the statistical and Schwinger field methods we derive the production of photons from the plasma by the Cerenkov mechanism. We derive the spectral formula of emitted photons by the plasma fluctuations. The calculation can be extended to the photon propagator involving radiative corrections.


2014 ◽  
Vol 23 (06) ◽  
pp. 1450059 ◽  
Author(s):  
Mahnaz Q. Haseeb ◽  
Obaidullah Jan ◽  
Omair Sarfaraz

Abundances of light nuclei formed during primordial nucleosynthesis are predicted by Standard Big Bang Model (SBBM). Here, we evaluate the second-order quantum electro dynamics (QED) corrections to the change in these parameters during primordial nucleosynthesis due to modifications to mass and coupling using finite temperature effects. These are the contributions from the dynamically generated masses for electrons and photons in the finite temperature background. Relative variations in neutron decay rate, total energy density of the universe, relative change in neutrino temperature etc. with two-loops corrections to electron mass, at the timescale when QED corrections were relevant, have been estimated.


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