Net-baryon number fluctuations in the Hybrid Quark-Meson-Nucleon model at finite density
arXiv:1711.05521 · doi:10.1103/PhysRevD.97.036011
Abstract
We study the mean-field thermodynamics and the characteristics of the net-baryon number fluctuations at the phase boundaries for the chiral and deconfinement transitions in the Hybrid Quark-Meson-Nucleon model. The chiral dynamics is described in the linear sigma model, whereas the quark confinement is manipulated by a medium-dependent modification of the particle distribution functions, where an additional scalar field is introduced. At low temperature and finite baryon density, the model predicts a first-, second-order chiral phase transition, or a crossover, depending on the expectation value of the scalar field, and a first-order deconfinement phase transition. We focus on the influence of the confinement over higher-order cumulants of the net-baryon number density. We find that whereas the cumulants show a substantial enhancement around the chiral phase transition, they are not as sensitive to the deconfinement transition.
accepted for publication
References in corpus (20)
- A Massive Pulsar in a Compact Relativistic Binary
- The equation of state in (2+1)-flavor QCD
- The Phase Structure of the Polyakov--Quark-Meson Model
- Susceptibilities and the Phase Structure of a Chiral Model with Polyakov Loops
- Signals of the QCD phase transition in core-collapse supernovae
- The phase structure of the Polyakov--quark-meson model beyond mean field
- A new quark-hadron hybrid equation of state for astrophysics - I. High-mass twin compact stars
- Susceptibilities near the QCD (tri)critical point
- The renormalization group and quark number fluctuations in the Polyakov loop extended quark-meson model at finite baryon density
- Baryons and the phase diagram for a large number of colors and flavors
- Light baryons below and above the deconfinement transition: medium effects and parity doubling
- Cold, dense nuclear matter in a SU(2) parity doublet model
- Quark-Nuclear Hybrid EoS with Excluded Volume Effects
- Nucleons and parity doubling across the deconfinement transition
- Nuclear Matter and Neutron stars in a Parity Doublet Model
- An effective model for the QCD phase transitions at finite baryon density
- Order parameters and color-flavor center symmetry in QCD
- Baryon number fluctuations in chiral effective models and their phenomenological implications
- QCD on a small circle
- Parity doubling of baryons in a chiral approach with three flavors
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- Constraint to chiral invariant masses of nucleons from GW170817 in an extended parity doublet model
- Toward a unified equation of state for multi-messenger astronomy
- Parity Doubling and the Dense Matter Phase Diagram under Constraints from Multi-Messenger Astronomy
- Chiral symmetry restoration and the matter formation in neutron stars
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- Chiral condensates for neutron stars in hadron-quark crossover: from a parity doublet nucleon model to an NJL quark model
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