scholarly journals Influence of strong field vacuum polarization on gravitational-electromagnetic wave interaction

2010 ◽  
Vol 82 (2) ◽  
Author(s):  
M. Forsberg ◽  
D. Papadopoulos ◽  
G. Brodin
1972 ◽  
Vol 50 (8) ◽  
pp. 826-842 ◽  
Author(s):  
M. P. Bachynski ◽  
B. W. Gibbs

Investigations of strong-field electromagnetic wave interactions with plasmas have been conducted. In the nonresonant frequency regions, the electron velocity distribution function is Maxwellian and considerations based on Maxwellian theory agree with experiment. At resonant and near-resonant frequencies considerations based on an electron velocity distribution which is non-Maxwellian explain the observations if enhanced electron diffusion is absent. However, at near-resonant frequencies, enhanced electron diffusion due to strong fields can be of great significance in reducing the electron density.


1995 ◽  
Author(s):  
Liyue Mu ◽  
William R. Donaldson ◽  
Jeff C. Adams ◽  
R. Aaron Falk

2021 ◽  
Vol 2021 (9) ◽  
Author(s):  
Felix Karbstein

Abstract We show that the leading derivative corrections to the Heisenberg-Euler effective action can be determined efficiently from the vacuum polarization tensor evaluated in a homogeneous constant background field. After deriving the explicit parameter-integral representation for the leading derivative corrections in generic electromagnetic fields at one loop, we specialize to the cases of magnetic- and electric-like field configurations characterized by the vanishing of one of the secular invariants of the electromagnetic field. In these cases, closed-form results and the associated all-orders weak- and strong-field expansions can be worked out. One immediate application is the leading derivative correction to the renowned Schwinger-formula describing the decay of the quantum vacuum via electron-positron pair production in slowly-varying electric fields.


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