Color Superconductivity and Radius of Quark Star in Extended NJL Model by Using the Dimensional Regularization
arXiv:hep-ph/0511286 · doi:10.1088/0305-4470/39/21/S30
Abstract
A radius of a dense star on the color superconducting phase is investigated in an extended NJL type model with two flavors of quarks. Since the model is non-renormalizable, the results depend on the regularization procedure. Here we apply the dimensional regularization and evaluate the radius of a dense star. Evaluating the TOV equation, we show the relationship between mass and radius of the dense star in the dimensional regularization.
arXiv comment4 pages.To appear in the proceedings of 7th Workshop on Quantum Field Theory Under the Influence of External Conditions (QFEXT 05), Barcelona, Catalonia, Spain, 5-9 Sep 2005. References are add
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Cited by in corpus (7)
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- Dimensionally regularized Boltzmann-Gibbs Statistical Mechanics and two-body Newton's gravitation
- Color superconductivity in the static Einstein Universe
- Newton's gravitation-force's classical average proof of a Verlinde's conjecture
- Quark matter influence on observational properties of compact stars