2013
DOI: 10.1103/physrevd.87.025010
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Instabilities of an anisotropically expanding non-Abelian plasma:3D+3Vdiscretized hard-loop simulations

Abstract: We study the (3+1)-dimensional evolution of non-Abelian plasma instabilities in the presence of a longitudinally expanding background of hard particles using the discretized hard loop framework. The free streaming background dynamically generates a momentum-space anisotropic distribution which is unstable to the rapid growth of chromomagnetic and chromoelectric fields. These fields produce longitudinal pressure that works to isotropize the system. Extrapolating our results to energies probed in ultrarelativist… Show more

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Cited by 63 publications
(89 citation statements)
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“…The early-time behavior is then described by plasma instabilities, which have been intensively analyzed over the past years [19][20][21][22]. Classical-statistical simulations show that gluons become highly occupied ∼ 1/α s (Q) after a proper time ∼ Q −1 log 2 (α −1 s ) for expanding systems [23][24][25].…”
Section: Jhep05(2014)054mentioning
confidence: 99%
“…The early-time behavior is then described by plasma instabilities, which have been intensively analyzed over the past years [19][20][21][22]. Classical-statistical simulations show that gluons become highly occupied ∼ 1/α s (Q) after a proper time ∼ Q −1 log 2 (α −1 s ) for expanding systems [23][24][25].…”
Section: Jhep05(2014)054mentioning
confidence: 99%
“…Quantities such as the dilepton production rate [96,97], photon production rate [98], single quark and quark anti-quark potentials [99][100][101][102][103][104][105][106][107], fermion damping rate [108][109][110], photon damping rate [111], gluon damping rate [112,113], jet energy loss [114][115][116][117][118][119][120][121][122][123][124][125], plasma instabilities [126][127][128][129][130][131][132], thermal axion production [133], and lepton asymmetry during leptogenesis [134,135] have also been calculated using HTLpt. We note, however, that most of the papers above have only worked at what we would call leading order in HTLpt.…”
Section: Jhep05(2014)027mentioning
confidence: 99%
“…There has been various attempts to study them both in the isotropic and anisotropic hot QCD medium [17][18][19][20]. The distributions functions for partons, used to study different aspects of QGP are discussed in [21][22][23][24][25]. In most of the studies, the momentum distributions that are crucial to obtain the whole plasma spectrum have been modeled by considering the QGP as free ultra-relativistic gas of quarks and gluons.…”
Section: Introductionmentioning
confidence: 99%