Pulsars as a probe for the nuclear and quark matter equation of state
Pulsars as a probe for the nuclear and quark matter equation of state
Pulsars as a probe for the nuclear and quark matter equation of state
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Ph<strong>as</strong>e Diagram <strong>of</strong> Quantum Chromodynamics QCD<br />
– p.6<br />
T<br />
T c<br />
early universe<br />
RHIC, LHC<br />
Quark−Gluon<br />
Pl<strong>as</strong>ma<br />
FAIR<br />
Hadrons<br />
nuclei<br />
Color<br />
Superconductivity<br />
neutron stars<br />
m / 3<br />
Early universe at zero density <strong>and</strong> high temperature<br />
N<br />
µ<br />
c<br />
µ<br />
neutron star <strong>matter</strong> at small temperature <strong>and</strong> high density<br />
first order ph<strong>as</strong>e transition at high density (not deconfinement!)<br />
<strong>probe</strong>d by heavy-ion collisions at GSI, Darmstadt (FAIR)
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