- 29 - Density Dependent Hadron Field Theory

نویسنده

  • C. Keil
چکیده

The appearance of the QCD phase transition (QPT) atlow temperatures and high densities will change the prop-erties of neutron stars (NS). Whether this change will bevisible with telescopes and gravitational wave antennas de-pends strongly on the equation of state (eos) of hadronicand quark matter and on the construction of the phasetransition (PT).

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تاریخ انتشار 2004