The effect of dynamical quark mass in the calculation of strange quark star structure
| Autor: | B. Ziaei, Gholam Hossein Bordbar |
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| Rok vydání: | 2012 |
| Předmět: |
Physics
Quantum chromodynamics Quark Particle physics Strange quark Equation of state High Energy Physics::Lattice High Energy Physics::Phenomenology Nuclear Theory Structure (category theory) FOS: Physical sciences Astronomy and Astrophysics Astrophysics Star (graph theory) Gravitation High Energy Physics - Phenomenology High Energy Physics - Phenomenology (hep-ph) Astrophysics - Solar and Stellar Astrophysics Space and Planetary Science Density dependent High Energy Physics::Experiment Solar and Stellar Astrophysics (astro-ph.SR) |
| DOI: | 10.48550/arxiv.1201.3228 |
| Popis: | We have discussed dynamical behavior of strange quark matter components, in particular the effects of density dependent quark mass on the equation of state of strange quark matter. Dynamical masses of quarks have been computed within Nambu-Jona-Lasinio (NJL) model, then we have done the strange quark matter calculations employing the MIT bag model with these dynamical masses. For the sake of comparing dynamical mass interaction with QCD quark-quark interaction, we have considered the one-gluon-exchange term as the effective interaction between quarks for MIT bag model. Our dynamical approach illustrates an improvement for the obtained values of equation of state. We have also investigated the structure of strange quark star using Tolman-Oppenheimer-Volkoff (TOV) equations for all applied models. Our results show that the dynamical mass interaction leads to lower values for the gravitational mass. Comment: 18 pages, 1 table, 7 figures |
| Databáze: | OpenAIRE |
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