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2024年10月30日
Chinese Physics C> 2018, Vol. 42> Issue(6) : 065102 DOI: 10.1088/1674-1137/42/6/065102

LOCV calculation of the equations of state and properties of rapidly rotating neutron stars

  • 1.

     Department of Physics, University of Zanjan, Zanjan, 45371-38791, Iran

  • In this paper, we have investigated the structural properties of rotating neutron stars using the numerical RNS code and equations of state which have been calculated within the lowest order constrained variational (LOCV) approach. In order to calculate the equation of state of nuclear matter, we have used UV14 +TNI and AV18 potentials. We have computed the maximum mass of the neutron star and the corresponding equatorial radius at different angular velocities. We have also computed the structural properties of Keplerian rotating neutron stars for the maximum mass configuration, MK, RK, fK and jmax.
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  • References

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A. H. Farajian, M. Bigdeli and S. Belbasi. LOCV calculation of the equations of state and properties of rapidly rotating neutron stars[J]. Chinese Physics C, 2018, 42(6): 065102. doi: 10.1088/1674-1137/42/6/065102
A. H. Farajian, M. Bigdeli and S. Belbasi. LOCV calculation of the equations of state and properties of rapidly rotating neutron stars[J]. Chinese Physics C, 2018, 42(6): 065102.  doi: 10.1088/1674-1137/42/6/065102 shu
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Received: 2018-02-16
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LOCV calculation of the equations of state and properties of rapidly rotating neutron stars

  • 1. Department of Physics, University of Zanjan, Zanjan, 45371-38791, Iran
  • Received Date: 2018-02-16
  • Available Online: 2018-06-05

Abstract: In this paper, we have investigated the structural properties of rotating neutron stars using the numerical RNS code and equations of state which have been calculated within the lowest order constrained variational (LOCV) approach. In order to calculate the equation of state of nuclear matter, we have used UV14 +TNI and AV18 potentials. We have computed the maximum mass of the neutron star and the corresponding equatorial radius at different angular velocities. We have also computed the structural properties of Keplerian rotating neutron stars for the maximum mass configuration, MK, RK, fK and jmax.

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