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neutron stars - Universität Heidelberg

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Phase Transitions in Quantum Chromodynamics QCD<br />

T<br />

Tc<br />

early universe<br />

RHIC, LHC<br />

Hadrons<br />

nuclei<br />

m / 3<br />

N<br />

Quark−Gluon<br />

FAIR<br />

Color<br />

Superconductivity<br />

<strong>neutron</strong> <strong>stars</strong><br />

µ<br />

c<br />

Plasma<br />

Early universe at zero density and high temperature<br />

<strong>neutron</strong> star matter at small temperature and high density<br />

first order phase transition at high density (not deconfinement)!<br />

probed by heavy-ion collisions at GSI, Darmstadt (FAIR!)<br />

µ<br />

– p.22

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