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Relativistic strange stars with anisotropy and B-parameter in pseudo spheroidal space time

Published online by Cambridge University Press:  20 March 2013

P. K. Chattopadhyay  and
B. C. Paul
P. K. Chattopadhyay
Affiliation:
Department of Physics, Alipurduar College, Jalpaiguri, 736122, West Bengal, India email:pkl_76@rediffmail.com
B. C. Paul
Affiliation:
Department of Physics, North Bengal University, Siliguri, 734013, West Bengal, India email: bcpaul@iucaa.ernet.in
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Abstract

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A class of compact cold stars in the presence of strange matter is obtained for a pseudo-spheroidal geometry. Considering the strange matter equation of state $p = \frac{1}{3}(\rho-4B)$ with pressure anisotropy described by Vaidya-Tikekar metric, we determine the parameter B both inside and on the surface of the star for different values of anisotropy parameter α. In the anisotropic case, we note that a stable model of a compact star may be realized.

Keywords

equation of state
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S291: Neutron Stars and Pulsars: Challenges and Opportunities after 80 years , August 2012 , pp. 362 - 364
Copyright
Copyright © International Astronomical Union 2013

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