Fluid QCD approach for quark-gluon plasma in stellar structure

Details Fluid QCD approach for quark-gluon plasma in stellar structure Fluid QCD approach for quark-gluon plasma in stellar structure

2011-09-28

arxiv.org/abs/1109.6066v1

Physics

High Energy Physics

High Energy Physics - Phenomenology

7 pages, Proceeding of the Conference in Honour of Murray Gell-Mann's 80th Birthday : Quantum Mechanics, Elementary Particles,

Scientific paper

10.1142/9789814335614_0040

The quark-gluon plasma in stellar structure is investigated using the fluid-like QCD approach. The classical energy momentum tensor relevant for high energy and hot plasma having the nature of fluid bulk of gluon sea is calculated within the model. The transition of gluon field from point particle field inside stable hadrons to relativistic fluid field in hot plasma and vice versa is briefly discussed. The results are applied to construct the equation of state using the Tolman--Oppenheimer--Volkoff equation to describe the hot plasma dominated stellar structure.

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