2006
DOI: 10.1007/1-4020-3430-x_08
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The QCD Equation of State and Quark Star Properties

Abstract: We review our quasiparticle model for the thermodynamics of strongly interacting matter at high temperature, and its extrapolation to non-zero chemical potential. Some implications of the resulting soft equation of state of quark matter at low temperatures are pointed out.

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Cited by 3 publications
(3 citation statements)
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“…In this section, we introduce the result from this approach: Equation (30). We introduce the light and strange chiral condensates, thermodynamic quantities, quark number density and susceptibility, and finally the chiral phase transition.…”
Section: Resultsmentioning
confidence: 99%
See 1 more Smart Citation
“…In this section, we introduce the result from this approach: Equation (30). We introduce the light and strange chiral condensates, thermodynamic quantities, quark number density and susceptibility, and finally the chiral phase transition.…”
Section: Resultsmentioning
confidence: 99%
“…, which can be adjusted to reproduce the lattice QCD calculations [30] and reflect the non-perturbative effects.…”
Section: The Su(3) Approachesmentioning
confidence: 99%
“…An evaluation of ( 29) for the present model for the QCD pressure would require its extension to a finite µ q , which we will perform in a subsequent work. In the present model, we used our knowledge of the composition as a function of temperature to define a proxy for (29) by interpolating between the two known limits (30) and (31) with the partial pressure of the HRG, x HRG (T) = P MHRG (T)/P tot (T), as…”
Section: Quark Number Susceptibilitiesmentioning
confidence: 99%