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Prog. Theor. Phys. Vol. 83 No. 3 (1990) pp. 499-521

[ Full Text PDF : FREE ACCESS (1349K) ]

Static and Dynamical Properties of Neutron Stars with Combined π0c Condensation

— Consequences from the First Order Phase Transition —

Takumi Muto and Toshitaka Tatsumi*

Research Institute for Fundamental Physics, Kyoto University, Kyoto 606
*Department of Physics, Kyoto University, Kyoto 606

(Received November 6, 1989)

Abstract:

Static and dynamical properties of neutron stars, in which combined π0c condensed core is contained, are investigated on the basis of the chiral symmetry approach. The first order nature of the phase transition is emphasized in studying these properties. For static properties, significant softening of the equation of state mainly due to the π0 condensate brings about a large change of internal structure from that of the normal phase. Effects on dynamical properties, especially mini-collapse associated with the first order phase transition from the metastable (supercompressed) πc condensed core to the stable combined π0c condensed core, are investigated in some detail. Energy release and lifetime of the metastable core are estimated and their implications on astronomical phenomena, especially 5 March 1979 event, are discussed.


URL : http://ptp.ipap.jp/link?PTP/83/499/
DOI : 10.1143/PTP.83.499

[ Full Text PDF : FREE ACCESS (1349K) ] Citation:


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  4. Progress of Theoretical Physics Supplement No.120 (1995) pp. 111-133 :
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