Radial Oscillations of Neutron Stars in Strong Magnetic Fields

Details Radial Oscillations of Neutron Stars in Strong Magnetic Fields Radial Oscillations of Neutron Stars in Strong Magnetic Fields

2001-01-29

arxiv.org/abs/astro-ph/0101504v1

Pramana 59:433-444,2002

Astronomy and Astrophysics

Astrophysics

latex2e file with five postscript figures

Scientific paper

10.1007/s12043-002-0041-4

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 magnetised neutron stars support higher maximum mass where as the effect of magnetic field on radial stability for observed neutron star masses is minimal.

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