Gluon matter plasma in the compact star core within a fluid QCD model

DOI10.1134/S020228931201015XzbMath1252.85007arXiv1112.4719WikidataQ125358125 ScholiaQ125358125MaRDI QIDQ1761352

L. T. Handoko, T. P. Djun, A. O. Latief, Chrisna Setyo Nugroho

Publication date: 15 November 2012

Published in: Gravitation \& Cosmology (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1112.4719

Mathematics Subject Classification ID

Strong interaction, including quantum chromodynamics (81V05) Magnetohydrodynamics and electrohydrodynamics (76W05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

Related Items (1)

Viscosities of gluon dominated QGP model within relativistic non-Abelian hydrodynamics

Cites Work

• Unnamed Item
• MAGNETOFLUID UNIFICATION IN YANG–MILLS LAGRANGIAN
• Cosmological Yang–Mills hydrodynamics
• Effect of Inhomogeneity on Cosmological Models
• Analogy between the Navier–Stokes equations and Maxwell’s equations: Application to turbulence
• On Massive Neutron Cores

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