Quasi-radial oscillations of rotating strange stars in strong magnetic fields

Details Quasi-radial oscillations of rotating strange stars in strong magnetic fields Quasi-radial oscillations of rotating strange stars in strong magnetic fields

Oct 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002jphg...28.2525s&link_type=abstract

Journal of Physics G: Nuclear and Particle Physics, Volume 28, Issue 10, pp. 2525-2537 (2002).

Physics

2

Scientific paper

In this paper we study quasi-radial oscillations of slowly rotating strange stars in strong magnetic fields in the density-dependent quark mass (DDQM) model. We see that the difference in frequency of rotating and non-rotating stars is more for higher magnetic fields. The change is small for low-mass stars but it increases with the mass of the star. This change of frequency is significant for maximum mass whereas it is marginal for a 1.4Msolar star.

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