Fluid QCD approach for quark-gluon plasma in stellar structure
High Energy Physics - Phenomenology
2011-09-29 v1 General Relativity and Quantum Cosmology
Nuclear Theory
Abstract
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.
Keywords
Cite
@article{arxiv.1109.6066,
title = {Fluid QCD approach for quark-gluon plasma in stellar structure},
author = {T. P. Djun and L. T. Handoko},
journal= {arXiv preprint arXiv:1109.6066},
year = {2011}
}
Comments
7 pages, Proceeding of the Conference in Honour of Murray Gell-Mann's 80th Birthday : Quantum Mechanics, Elementary Particles, Quantum Cosmology, Complexity (2011) 419-425