strong external field
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2020 ◽  
Vol 537 ◽  
pp. 110855 ◽  
Author(s):  
M.A. Kozhushner ◽  
V.S. Posvyanskii ◽  
B.V. Lidskii ◽  
V.L. Bodneva ◽  
O.J. Ilegbusi ◽  
...  

2018 ◽  
Vol 168 ◽  
pp. 04003
Author(s):  
Aftab Ahmad ◽  
Naser Ahmadiniaz ◽  
Olindo Corradini ◽  
Sang Pyo Kim ◽  
Christian Schubert

In this contribution, we present our recent compact master formulas for the multiphoton amplitudes of a scalar propagator in a constant background field using the worldline fomulation of quantum field theory. The constant field has been included nonperturbatively, which is crucial for strong external fields. A possible application is the scattering of photons by electrons in a strong magnetic field, a process that has been a subject of great interest since the discovery of astrophysical objects like radio pulsars, which provide evidence that magnetic fields of the order of 1012G are present in nature. The presence of a strong external field leads to a strong deviation from the classical scattering amplitudes. We explicitly work out the Compton scattering amplitude in a magnetic field, which is a process of potential relevance for astrophysics. Our final result is compact and suitable for numerical integration.


Open Physics ◽  
2013 ◽  
Vol 11 (9) ◽  
Author(s):  
Damien Middleton ◽  
Katravulapally Tejaswi ◽  
Lampros Nikolopoulos

AbstractA set of rate equations have been tested against a more robust set of Time-Dependent Density Matrix (TDDM) equations [D. P. W. Middleton, L. A. A. Nikolopoulos, J. Mod. Opti. 59, 1650 (2012)] by using them to determine the populations of ion species and autoionising states (AIS) in noble gas atoms when interacting with a strong external field. Two field shapes were tested here — sinusoidal and square — and a variety of pulse characteristics were examined, i.e. intensity, duration and photon energy, for the neon atomic system. It was found that the rate equations were sufficiently accurate only when the external field is way off-resonant with the AIS. Moreover, analytical solutions of the rate equations in the square pulse case agree with the numerical solutions for a time-dependent pulse containing many cycles. An attempt to model a stochastic field was also made and it was found that the use of such a field diminished and broadened the ion yield ratio due to the presence of an added bandwidth.


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