• Vinita Tuli

      Articles written in Pramana – Journal of Physics

    • Radial oscillations of neutron stars in strong magnetic fields

      VK Gupta Vinita Tuli S Singh JD Anand Ashok Goyal

      More Details Abstract Fulltext PDF

      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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