How to detect the Quark-Gluon Plasma with Telescopes
نویسنده
چکیده
The appearance of the QCD phase transition (QPT) at low temperatures and high densities will change the properties of neutron stars (NS). Whether this change will be visible with telescopes and gravitational wave antennas depends strongly on the equation of state (eos) of hadronic and quark matter and on the construction of the phase transition (PT).
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تاریخ انتشار 2004