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We supplement the analytic solution obtained by Matthews O. M., et. al.,2005, MNRAS, \textbf{356}, 66 to investigate the steady-state structure ofradiation pressure dominated disc under the influence of a stellar magneticfield which deploys a torque. The solutions converge to the non-magneticShakura N. I., Sunyaev R. A., 1973, A\& A, \textbf{24}, 337 form when magneticfield of the star tends to zero and also at large radii. Effects of varying themass accretion rates and the spin period of a typical neutron star on the discparameters are presented. We further report that the presence of a magneticcorrection term $k$ reduces the radial extent upto which radiation pressure andelectron scattering continue to be the major source of pressure and opacityrespectively. We also report that magnetic effects amplify the viscoustimescale several times in the inner disc.

Effects of magnetic field on the radiation pressure dominated discs around neutron stars