Effects of the Tsallis distribution in the linear sigma model
arXiv:1411.7123 · doi:10.1142/S0218301315500858
Abstract
The effects of the Tsallis distribution which has two parameters, and ,on physical quantities are studied using the linear sigma model in chiral phase transitions. The Tsallis distribution approaches the Boltzmann-Gibbs distribution as approaches . The parameter dependences of the condensate and mass for various are shown, where is called temperature. The critical temperature and energy density are described with digamma function, and the dependences of these quantities and the extension of Stefan-Boltzmann limit of the energy density are shown. The following facts are clarified. The chiral symmetry restoration at occurs at low temperature, compared with the restoration at .The sigma mass and pion mass reflect the restoration. The critical temperature decreases monotonically as increases. The small deviation from the Boltzmann-Gibbs distribution results in the large deviations of physical quantities, especially the energy density. It is displayed from the energetic point of view that the small deviation from the Boltzmann-Gibbs distribution is realized for . The physical quantities are affected by the Tsallis distribution even when is small.
11 pages, 6figures; some parts were modified
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- Chiral phase transition in the linear sigma model within Hartree factorization in the Tsallis nonextensive statistics
- Chiral phase transition within the linear sigma model in the Tsallis nonextensive statistics based on density operator
- Bounds on the Tsallis Parameter from a deformed Neutrino Sector in the Early Universe
- Relation between the escort average in microcanonical ensemble and the escort average in canonical ensemble in the Tsallis statistics
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- Non-extensive Effects on the QCD Equation of State and Fluctuations of Conserved Charges within Polyakov Quark Meson Model