Strange Star Equation of State With a Modified Richardson Potential

Details Strange Star Equation of State With a Modified Richardson Potential Strange Star Equation of State With a Modified Richardson Potential

2005-09-23

arxiv.org/abs/astro-ph/0509703v2

Adv.Space Res. 38 (2006) 2912-2914

Astronomy and Astrophysics

Astrophysics

4 pages, no figure, to appear in the Proceedings of COSPAR Colloquium "Spectra & Timing of Compact X-ray Binaries," January 17

Scientific paper

10.1016/j.asr.2006.01.026

Richardson potential is an phenomenological interquark interaction taking care of two aspects of QCD, namely the asymptotic freedom and the confinement. The original potential has a scale parameter having value around 400 MeV and is well tested in hadronic property calculations. This potential was then used in strange star calculation. Strange stars are very compact stars composed of strange quark matter i.e. a very high density strange quark phase consisting of deconfined u, d and s quarks. Here the value of the scale parameter was taken as 100 MeV. The argument was that for a deconfined quark system like a strange star, the scale parameter may have a value quite different from that used in hadronic sector. To remove this discrepancy we introduced two scale parameters in the potential, one for the asymptotic freedom part and the other for the confining part. With suitable values of the parameters, this modified potential has been successfully used in both baryonic property and strange star calculations. The Equation of States obtained with the modified potential are also used to obtain mass-radius relations for the strange stars.

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