Relaxation of the chiral imbalance in dense matter of a neutron star

Relaxation of the chiral imbalance in dense matter of a neutron star

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hammont clear acrylic boxes Using the quantum field theory methods, we calculate the helicity flip of an electron scattering off protons in dense matter of a neutron star.The influence of the electroweak interaction between electrons and background nucleons cotopaxi bibs on the helicity flip is examined.We also derive the kinetic equation for the chiral imbalance.

The derived kinetic equation is compared with the results obtained by other authors.