Thermodynamic pressure for massless QCD and the trace anomaly

Abstract

From statistical mechanics the trace of the thermal average of any energy-momentum tensor is $⟨T_{\mu }^{\mu }⟩=T\partial P/\partial T-4P$. The renormalization group formula $⟨T_{\mu }^{\mu }⟩=\beta (g_M)\partial P/\partial g_M$ for QCD with massless fermions requires the pressure to have the structure \begin{equation} P=T^{4}\sum_{n=0}^{\infty} ϕ_{n}(g_{M})\big[\ln\big({M\over 4πT}\big)\big]^{n},\end{equation} where the factor $4\pi$ is for later convenience. The functions ${\varphi }_n(g_M)$ for $n\ge 1$ may be calculated from ${\varphi }_0(g_M)$ using the recursion relation $n{\varphi }_n(g_M)=-\beta (g_M)d{\varphi }_{n-1}/d{g}_M$. This is checked against known perturbation theory results by using the terms of order $(g_M{)}^2,(g_M{)}^3$, $(g_M{)}^4$ in ${\varphi }_0(g_M)$ to obtain the known terms of order $(g_M{)}^4,(g_M{)}^5$, $(g_M{)}^6$ in ${\varphi }_1(g_M)$ and the known term of order $(g_M{)}^6$ in ${\varphi }_2(g_M)$. The above series may be summed and gives the same result as choosing $M=4\pi T$, viz. $T^4{\varphi }_0(g_{4\pi T})$.

arXiv comment4 pages. Error corrected in Sec III.A now gives complete agreement with Ref [11]

References in corpus (8)

• The pressure of hot QCD up to g^6 ln(1/g)
• Free Energy of QCD at High Temperature
• The Three-Loop Free Energy for Pure Gauge QCD
• The Three-Loop Free Energy for High-Temperature QED and QCD with Fermions
• The Free Energy of Hot Gauge Theories with Fermions Through g^5
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• Eliminating Infrared Divergences in the Pressure
• QCD Pressure and the Trace Anomaly

Cited by in corpus (1)

• Phases of a 10-D Holographic hard wall model