1998
DOI: 10.1103/physrevc.58.356
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Preequilibrium evolution of quark-gluon plasma

Abstract: We study the production and the evolution of quark-gluon plasma expected to be formed in ultra relativistic heavy-ion collisions, within the color fluxtube model. We introduce the gluonic component in the Boltzmann equation, which we solve in the phase space which is extended to include the SU(3) color degree of freedom. The color degree of freedom is shown to play a decisive role in equilibration, and in fixing the temperature of the plasma. We further find that the soft partons that we study here contribute … Show more

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Cited by 34 publications
(34 citation statements)
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“…where the parameters T , v and µ depend on position along the path x µ (τ ) from (8). The evolution of f e describes the flow of a dissipation-free fluid, as we now demonstrate.…”
Section: Linearized Boltzmann Equationsupporting
confidence: 52%
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“…where the parameters T , v and µ depend on position along the path x µ (τ ) from (8). The evolution of f e describes the flow of a dissipation-free fluid, as we now demonstrate.…”
Section: Linearized Boltzmann Equationsupporting
confidence: 52%
“…The time component of (8), dt/dτ = E/p · u, implies that τ is the time in the fluid rest frame. Moreover, (8) defines the path x µ (τ ) of the center of momentum of a phase space cell of mean p µ relative to this frame. We now write the Boltzmann equation as…”
Section: Linearized Boltzmann Equationmentioning
confidence: 99%
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“…Below we will describe a partial reconciliation of these approaches; and 4) Little attention has been paid to particular nonAbelian features in transport equations [273]. A study [274] of Wong's equation [275] is one step in the direction of explicitly including colour algebra effects.…”
Section: Preliminariesmentioning
confidence: 99%
“…This study also plays a crucial role in determining many of the potential signatures for quark-gluon plasma detection at RHIC. The space-time evolution of the parton gas for this non-equilibrium situation can be be modeled by solving semi classical relativistic transport equations [2,3,4,5,6,7,8,9,10]. Central to solving the transport equations is what goes into the scattering kernels.…”
mentioning
confidence: 99%