QCD-Thermodynamics using 5-dim Gravity

E. Megias; H.J. Pirner; K. Veschgini

QCD-Thermodynamics using 5-dim Gravity

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arxiv 1009.2953 v2 pith:TPY6KFPC submitted 2010-09-15 hep-ph hep-th

E. Megias , H.J. Pirner , K. Veschgini This is my paper · ORCID

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keywords temperaturetheorychangecriticalenergyfinitefreegravity

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We calculate the critical temperature and free energy of the gluon plasma using the dilaton potential arXiv:0911.0627[hep-ph] in the gravity theory of AdS/QCD. The finite temperature observables are calculated in two ways: first, from the Page-Hawking computation of the free energy, and secondly using the Bekenstein-Hawking proportionality of the entropy with the area of the horizon. Renormalization is well defined, because the T=0 theory has asymptotic freedom. We further investigate the change of the critical temperature with the number of flavours induced by the change of the running coupling constant in the quenched theory. The finite temperature behaviour of the speed of sound, spatial string tension and vacuum expectation value of the Polyakov loop follow from the corresponding string theory in AdS_5.

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In a hardwall AdS/QCD model with phenomenological boundary conditions, both baryonic and quark condensates dominate the low-temperature phase diagram of dense nuclear matter.

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