Electromagnetic Properties of Lepton in Neutron Star

When light propagate through the neutron star, it changes its properties based on the temperature, density and the magnetic field. The electrons propagating through this environment changes its mass, charge and wavefunction. This modification in the properties of charged particles and the electromagnetic signals has a combined effect on the rate of production of electrons via beta decay which in turn affect the nucleosynthesis and luminosity of the star. This information can be used to understand the neutron star in a little more detail.