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      Perturbative and non-perturbative aspects of the non-abelian Boltzmann-Langevin equation

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          Abstract

          We study the Boltzmann-Langevin equation which describes the dynamics of hot Yang-Mills fields with typical momenta of order of the magnetic screening scale g^2 T. It is transformed into a path integral and Feynman rules are obtained. We find that the leading log Langevin equation can be systematically improved in a well behaved expansion in log(1/g)^-1. The result by Arnold and Yaffe that the leading log Langevin equation is still valid at next-to-leading-log order is confirmed. We also confirm their result for the next-to-leading-log damping coefficient, or color conductivity, which is shown to be gauge fixing independent for a certain class of gauges. The frequency scale g^2T does not contribute to this result, but it does contribute, by power counting, to the transverse gauge field propagator. Going beyond a perturbative expansion we find 1-loop ultraviolet divergences which cannot be removed by renormalizing the parameters in the Boltzmann-Langevin equation.

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          Free Energy of QCD at High Temperature

          Effective-field-theory methods are used to separate the free energy for a nonabelian gauge theory at high temperature \(T\) into the contributions from the momentum scales \(T\), \(gT\), and \(g^2T\), where \(g\) is the coupling constant at the scale \(2 \pi T\). The effects of the scale \(T\) enter through the coefficients in the effective lagrangian for the 3-dimensional effective theory obtained by dimensional reduction. These coefficients can be calculated as power series in \(g^2\). The contribution to the free energy from the scale \(gT\) can be calculated using perturbative methods in the effective theory. It can be expressed as an expansion in \(g\) starting at order \(g^3\). The contribution from the scale \(g^2T\) must be calculated using nonperturbative methods, but nevertheless it can be expanded in powers of \(g\) beginning at order \(g^6\). We calculate the free energy explicitly to order \(g^5\). We also outline the calculations necessary to obtain the free energy to order \(g^6\).
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            Really Computing Non-perturbative Real Time Correlation Functions

            It has been argued by Grigoriev and Rubakov that one can simulate real time processes involving baryon number non-conservation at high temperature using real time evolution of classical equations, and summing over initial conditions with a classical thermal weight. It is known that such a naive algorithm is plagued by ultraviolet divergences. In quantum theory the divergences are regularized, but the corresponding graphs involve the contributions from the hard momentum region and also the new scale \(\sim gT\) comes into play. We propose a modified algorithm which involves solving the classical equations of motion for the effective hard thermal loop Hamiltonian with an ultraviolet cutoff \(\mu \gg gT\) and integrating over initial conditions with a proper thermal weight. Such an algorithm should provide a determination of the infrared behavior of real time correlation function \( _T\) determining the baryon violation rate. Hopefully, the results obtained in this modified algorithm would be cutoff-independent.
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              Hadronic Spectral Functions in Lattice QCD

              QCD spectral functions of hadrons in the pseudo-scalar and vector channels are extracted from lattice Monte Carlo data of the imaginary time Green's functions. The maximum entropy method works well for this purpose, and the resonance and continuum structures in the spectra are obtained in addition to the ground state peaks.
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                Author and article information

                Journal
                18 May 2002
                2002-09-11
                Article
                10.1016/S0550-3213(02)00841-6
                hep-ph/0205202
                b85c8e45-4899-402b-885d-6523f46fa930
                History
                Custom metadata
                BI-TP 2002/08
                Nucl.Phys. B647 (2002) 512-538
                Some discussions and notations clarified
                hep-ph

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