On partial deconfinement, strange star and quark-hadron phase transition in the early universe
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Summary
Using the thermodynamic model at zero temperature and a density-dependent quark mass model of confinement, the possibilities of light-quark liberation and strange-quark formation near ground-state nuclear matter have been investigated. Some thermodynamic properties of strange quark matter which may be produced at the core of neutron stars have been studied. The possibility of quark-hadron phase transition in the early Universe has also been investigated using a modified version of a density-dependent confinement mechanism at finite temperature.
Keywords
PACS 05.70 Thermodynamics PACS 12.50.Ch Models of quarks and leptons PACS 97.30 Variable and peculiar stars (including novae) PACS 97.90 Other topics on starsPreview
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References
- [1]A. M. Polyakov:Phys. Lett. B,72, 477 (1978).MathSciNetADSCrossRefGoogle Scholar
- [2]L. Susskind:Phys. Rev. D,20, 2610 (1979).ADSCrossRefGoogle Scholar
- [3]J. Kogut, M. Stone, H. W. Wyld, W. R. Gibbs, J. Shigemitsu, S. H. Shenker andD. K. Sinclair:Phys. Rev. Lett.,50, 397 (1983).ADSCrossRefGoogle Scholar
- [4]
- [5]A. Chados, R. L. Jaffe, K. Johnson, C. B. Thorn andV. F. Weiskopf:Phys. Rev. D,9, 3471 (1974).MathSciNetADSCrossRefGoogle Scholar
- [6]
- [7]
- [8]K. A. Olive:Nucl. Phys. B,190, 483 (1981).ADSCrossRefGoogle Scholar
- [9]
- [10]O. Zhirov:Yad. Fiz.,30, 1098 (1979).Google Scholar
- [11]
- [12]M. Plümer: Doctoral Dissertation, Phillips Universität, Marburg (1984).Google Scholar
- [13]
- [14]J. C. Pati andA. Salam: inProceedings of the International Neutrino Conference 1976, Aachen, West Germany, edited byH. Faissner, H. Reithler andP. Zerwas (Vieweg, Braunschweig, 1977), p. 589.CrossRefGoogle Scholar
- [15]E. Written:Phys. Rev. D,30, 272 (1984).ADSCrossRefGoogle Scholar
- [16]
- [17]
- [18]
- [19]
- [20]O. G. Benvenuto, J. E. Horvath andH. Vucetich:Int. J. Mod. Phys. A,4, 257. (1989).ADSCrossRefGoogle Scholar
- [21]
- [22]
- [23]J. Kristian, C. R. Pennypacker, J. Middleditch, M. A. Hamuy, J. N. Imamura, W. E. Kunkel, R. Lucinio, D. E. Morris, R. A. Muller, S. Perlmutter, S. J. Rawlings, T. P. Sasseen, L. K. Shelton, T. Y. Steiman-Cameron andI. R. Tuohy:Nature,338, 234 (1989).ADSCrossRefGoogle Scholar
- [24]J. L. Friedman, J. R. Ipser andL. Parker:Phys. Rev. Lett.,62, 3015 (1989);N. K. Glendenning:Phys. Rev. Lett.,63, 1443 (1989).ADSCrossRefGoogle Scholar
- [25]S. Chakrabarty:Phys. Scr. (in press);Phys. Rev. D (in press).Google Scholar
- [26]St. Mrówczynski:J. Phys.,11, L235 (1985).ADSCrossRefGoogle Scholar
- [27]
- [28]
- [29]
- [30]W. Broniowski, T. D. Cohen andM. K. Banerjee:Phys. Lett. B,187, 229 (1986).ADSCrossRefGoogle Scholar
- [31]K. Huang:Statistical Mechanics (Wiley, New York, N.Y., 1963).Google Scholar
- [32]S. L. Sapiro andS. A. Teukoloky:Black Holes, White Dwarfs and Newton Stars, The Physics of Compact Objects (J. Wiley, 1983).Google Scholar
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© Società Italiana di Fisica 1991