gradient expansion
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2021 ◽  
Vol 104 (12) ◽  
Author(s):  
E. V. Gorbar ◽  
K. Schmitz ◽  
O. O. Sobol ◽  
S. I. Vilchinskii

2021 ◽  
Vol 2021 (11) ◽  
Author(s):  
Xiao-Li Luo ◽  
Jian-Hua Gao

Abstract We derive the chiral kinetic equation in 8 dimensional phase space in non- Abelian SU(N) gauge field within the Wigner function formalism. By using the “covariant gradient expansion”, we disentangle the Wigner equations in four-vector space up to the first order and find that only the time-like component of the chiral Wigner function is independent while other components can be explicit derivative. After further decomposing the Wigner function or equations in color space, we present the non-Abelian covariant chiral kinetic equation for the color singlet and multiplet phase-space distribution functions. These phase-space distribution functions have non-trivial Lorentz transformation rules when we define them in different reference frames. The chiral anomaly from non-Abelian gauge field arises naturally from the Berry monopole in Euclidian momentum space in the vacuum or Dirac sea contribution. The anomalous currents as non-Abelian counterparts of chiral magnetic effect and chiral vortical effect have also been derived from the non-Abelian chiral kinetic equation.


2021 ◽  
Vol 104 (6) ◽  
Author(s):  
Michal P. Heller ◽  
Alexandre Serantes ◽  
Michał Spaliński ◽  
Viktor Svensson ◽  
Benjamin Withers

2020 ◽  
Vol 102 (12) ◽  
Author(s):  
O. O. Sobol ◽  
A. V. Lysenko ◽  
E. V. Gorbar ◽  
S. I. Vilchinskii

Author(s):  
Marco Frasca ◽  
Riccardo Maria Liberati ◽  
Massimiliano Rossi

A technique devised some years ago permits to study a theory in a regime of strong perturbations. This translate into a gradient expansion that, at the leading order, can recover the BKL solution. We solve exactly the leading order equations in a spherical symmetric case and we show that the 4-velocity in such a case is multiplied by an exponential warp factor when the perturbation is properly applied. This factor is always greater than one. We will give a closed form solution of this factor for a simple case. Some numerical examples are also given.


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