Spin-sum Correction To Inverse Compton Scattering Cross Section In Strong Background Magnetic Field

Astrophysical models need calculations in cross section. It is believed that inverse Comptonrnscattering in strong magnetic fields near the surfaces of Neutron stars is one of the possiblernmechanisms responsible for X-ray and -ray emissions. Spin sum is one fundamental variable inrncalculations of scattering cross sections involving charged fermions in magnetic field. In thisrnthesis we explicitly calculate the spin-sum of the solutions of Dirac equation and using it werncalculate spin-sum corrected total cross of the inverse Compton scattering in the presence ofrnuniform and strong magnetic field

Get Full Work

Report copyright infringement or plagiarism