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References:
[1] Liebendörfer, M. et al: Probing the gravitational well: No supernova explosion in spherical symmetry with general relativistic Boltzmann neutrino transport. Phys. Rev. D63 (2001), 103004.
[2] Weber, F.: Pulsars as Astrophysical Laboratories for Nuclear and Particle Physics. IOP Publishing Ltd 1999.
[3] Boyanovsky, D.: Phase transitions in the early and the present Universe: from the big bang to heavy ion collisions. hep-ph/0102120 (2001). Zbl 0990.83018
[4] Youngblood, D. H.: Isoscalar Giant Resonances and Nuclear Matter Compressibility. Nucl. Phys. A687 (2001), 1c.
[5] Heiselberg, H., Hjorth-Jensen, M.: Phases of dense matter in neutron stars. Physics Reports 328 (2000), 237.
[6] Danielewicz, P., Lacey, R., Lynch, W. G.: Determination of the Equation of State of Dense Matter. Science 298 (2002), 1592.
[7] Chýla, J.: Od barevných kvarků ke kvantové chromodynamice a Nobelové ceně za fyziku v roce 2004. PMFA 50 (2005), 2.
[8] Pochodzalla, J. et al: Probing the Nuclear Liquid-Gas Phase Transition. Phys. Rev. Lett. 75 (1995), 1040.
[9] Collins, J. C., Perry, M. J.: Superdense matter: Neutrons or Asymptotically Free Quarks?. Phys. Rev. Letter 34 (1975), 1353.
[10] Shuryak, E. V.: Quantum Chromodynamics and the theory of superdense matter. Phys. Rep. 61 (1980), 71. MR 0571448
[11] Heinz, U., Jacob, M.: Evidence for a New State: an Assessment of the Results from the CERN Lead Beam Program. nucl-th/0002042 (2000).
[12] Phobos, Star, Phoenix, Brahms: Formal Report. BNL-73847-2005, http://www.bnl.gov/bnlweb/pubaf/pr/docs/Hunting-the-QGP.pdf
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