Articles written in Pramana – Journal of Physics
Volume 3 Issue 5 November 1974 pp 311-322 Nuclear And Particle Physics
This is a continuation of our earlier investigation (Gurtu
Volume 59 Issue 3 September 2002 pp 433-443
The eigen frequencies of radial pulsations of neutron stars are calculated in a strong magnetic field. At low densities we use the magnetic BPS equation of state (EOS) similar to that obtained by Lai and Shapiro while at high densities the EOS obtained from the relativistic nuclear mean field theory is taken and extended to include strong magnetic field. It is found that magnetized neutron stars support higher maximum mass whereas the effect of magnetic field on radial stability for observed neutron star masses is minimal.
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