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Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D, Particles, fields, gravitation, and cosmology· 2014

Equation of state in (<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mn>2</mml:mn><mml:mo>+</mml:mo><mml:mn>1</mml:mn></mml:mrow></mml:math>)-flavor QCD

Alexei Bazavov, Tanmoy Bhattacharya, C. DeTar, Heng-Tong Ding et al.

Short summary

This study presents the equation of state for (2+1)-flavor QCD, yielding an energy density of 0.18-0.5 GeV/fm³ (1.2-3.1 ε_nuclear) in the crossover region (145-163 MeV).

AI-generated from the title and abstract; the full text is not read.

Key points

  • Equation of state for (2+1)-flavor QCD calculated using improved staggered quark actions.
  • Thermodynamic quantities and speed of sound determined in the 130-400 MeV temperature range.
  • Energy density in the crossover region (145-163 MeV) is 0.18-0.5 GeV/fm³.
  • Analytic parameterization of pressure provided for phenomenological use.

AI-generated from the title and abstract; the full text is not read.

Abstract

We present results for the equation of state in ($2+1$)-flavor QCD using the highly improved staggered quark action and lattices with temporal extent ${N}_{\ensuremath{\tau}}=6$, 8, 10, and 12. We show that these data can be reliably extrapolated to the continuum limit and obtain a number of thermodynamic quantities and the speed of sound in the temperature range 130--400 MeV. We compare our results with previous calculations and provide an analytic parameterization of the pressure, from which other thermodynamic quantities can be calculated, for use in phenomenology. We show that the energy density in the crossover region, $145\text{ }\text{ }\mathrm{MeV}\ensuremath{\le}T\ensuremath{\le}163\text{ }\text{ }\mathrm{MeV}$, defined by the chiral transition, is ${\ensuremath{\epsilon}}_{c}=(0.18--0.5)\text{ }\text{ }\mathrm{GeV}/{\mathrm{fm}}^{3}$, i.e., $(1.2--3.1)\text{ }{\ensuremath{\epsilon}}_{\text{nuclear}}$. At high temperatures, we compare our results with resummed and dimensionally reduced perturbation theory calculations. As a byproduct of our analyses, we obtain the values of the scale parameters ${r}_{0}$ from the static quark potential and ${w}_{0}$ from the gradient flow.

The authors' abstract, as published at the source. Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D, Particles, fields, gravitation, and cosmology, 2014 · DOI ↗

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Field: Nuclear and High Energy Physics

Nuclear and High Energy PhysicsPhysics and Astronomy