Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000apj...538..870a&link_type=abstract
The Astrophysical Journal, Volume 538, Issue 2, pp. 870-875.
Astronomy and Astrophysics
Astronomy
5
Magnetic Fields, Stars: Oscillations
Scientific paper
The eigenfrequencies of radial pulsations of quark stars are calculated in a general relativistic formalism given by Chandrasekhar in the density-dependent quark mass model in strong magnetic fields. It is found that the squares of the frequencies are always decreasing functions of the central density of the strange star. The maximum mass, the radius, and gravitational redshift of the star are increasing functions of the magnetic field.
Anand J. D.
Chandrika Devi N.
Gupta Vijay K.
Singh Sumeetpal S.
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