Effect of superstrong magnetic field on electron screening at the crusts of neutron stars

The influences of electron screening (ES) and electron energy correction (EEC) are investigated by superstrong magnetic field (SMF). We also discuss in detail the discrepant factor between our results and those of Fushiki, Gudmundsson and Pethick (FGP) in SMF. The results show that SMF has only a slight effect on ES when B < 10(9) T on the surfaces of most neutron stars. Whereas for some magnetars, SMF influence ES greatly when B > 10(9) T. For instance, due to SMF the ES potential may be increased about 23.6% and the EEC may be increased about 4 orders of magnitude at rho/mu(e) = 1.0 x 10(6) mol/cm(3) and T-9 = 1. On the other hand, the discrepant factor shows that our results are in good agreement with FGP's when B < 10(9) T. But the difference will be increased with increasing SMF.