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Chiral soliton model at finite temperature and density

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arxiv 1301.6227 v2 pith:PG7XLMDP submitted 2013-01-26 hep-ph nucl-th

classification hep-phnucl-th
keywords solitonchiralenergytemperaturetransitionconstituentdensityfinite
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abstract

In mean field approximation, we study a chiral soliton of the linear sigma model with two flavors at finite temperature and density. The stable soliton solutions are calculated with some appropriate boundary conditions. Energy and radius of the soliton are determined in a hot medium of constituent quarks. It is found that for $T<T_c$, the energy of the soliton $E^*$ is less than the energy of three constituent quarks $3M_q$, but with the increasing of temperature, the difference between $E^*$ and $3M_q$ becomes smaller and smaller, once $T>T_c$, there is a sharp delocalization phase transition from hadron matter to quark matter coincident with the restoration of chiral symmetry. In the transition region, the thermodynamic properties show large discontinuities which is an indication for a first-order phase transition.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. The nucleon properties in finite temperature and density with Gaussian fluctuations

    hep-th 2024-12 conditional novelty 6.0 of 10

    Gaussian fluctuations make the quark meson model predict a non-monotonic nucleon mass and a faster-growing nucleon radius as temperature and density increase.

  2. The nucleon properties in finite temperature and density with vector meson

    hep-ph 2024-12 conditional novelty 5.0 of 10

    Adding omega vector repulsion to the quark-meson soliton model increases nucleon mass and radius and reduces the energy gap to three free quarks, signaling instability.

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