Radial Oscillations of Rotating Strange Stars in Strong Magnetic Fields

Radial Oscillations of Rotating Strange Stars in Strong Magnetic Fields

In this paper we study radial oscillations of rotating strange stars in strong magnetic fields in the Density Dependent Quark Mass (DDQM) model. We see that increase of frequency i.e. difference in frequency of rotating and non-rotating stars is more for higher magnetic fields. The change is small f...

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Veröffentlicht in:arXiv.org 2000-12
Hauptverfasser: Singh, S, N Chandrika Devi, Gupta, V K, Gupta, Asha, Anand, J D
Format: Artikel
Sprache:eng
Schlagworte:
Low mass stars
Magnetic fields
Oscillations
Quarks
Stars
Stellar magnetic fields
Stellar rotation
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Zusammenfassung:In this paper we study radial oscillations of rotating strange stars in strong magnetic fields in the Density Dependent Quark Mass (DDQM) model. We see that increase of frequency i.e. 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 1.4 solar mass star.
ISSN:2331-8422