  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.
