International Journal of Astronomy and Astrophysics

Vol.3 No.3(2013), Paper ID 36508, 10 pages

DOI:10.4236/ijaa.2013.33026

 

Computing Differentially Rotating Neutron Stars Obeying Realistic Equations of State by Using Hartle’s Perturbation Method

 

Anastasios Katelouzos, Vassilis Geroyannis

 

Department of Physics, University of Patras, Patras, Greece
Department of Physics, University of Patras, Patras, Greece

 

Copyright © 2013 Anastasios Katelouzos, Vassilis Geroyannis et al. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

 

How to Cite this Article


A. Katelouzos and V. Geroyannis, "Computing Differentially Rotating Neutron Stars Obeying Realistic Equations of State by Using Hartle’s Perturbation Method," International Journal of Astronomy and Astrophysics, Vol. 3 No. 3, 2013, pp. 217-226. doi: 10.4236/ijaa.2013.33026.

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