Superdense stars containing strange quark matter Yu.L.Vartanyan, A. R. Harutyunyan Yerevan State University.

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Superdense stars containing strange quark matter Yu.L.Vartanyan, A. R. Harutyunyan Yerevan State University

Strange quark matter In pioneer work of V.A.Ambartsumian and G.S. Sahakian [1] it has been shown that degenerated nuclear plasma may contain, besides neutrons, protons and electrons, also strange baryons – hyperons. In [2] G.S. Sahakian and Yu.L.Vartanian for the first time have shown that taking into account the interaction between baryons makes possible the existence of hyperons in the central regions of stable neutron stars. A new interest towards strange nuclear plasma has arisen when Witten [3] supposed, that quark-electron plasma with a strangeness -1 per baryon may be absolutely stable state of cold superdense matter. V.A.Ambartsumian, G.S. Sahakian, Sov.Astron.Zh., 37, 193,1960. G.S.Sahakian, Yu.L.Vartanian, Nuovo Cimento, 30, 82, 1963; Sov.Astron.Zh., 41, 193, E.Witten, Phys.Rev. D30, 272, 1984.

Strange Stars Yu.L.Vartanyan, A.R.Arutyunyan, A.K.Grigoryan, Astrofizika, 37, 499,1994 (Astrophysics, 37, 271, 1994); Yu.L.Vartanyan, A.R.Arutyunyan, A.K.Grigoryan, Astronomy Letters, 21, 122, 1995.

EoS for Strange Stars n (fm -3 ) E (MeV)

Radius-central density (SS)

Mass-radius relationship (SS)

Total energy density-distance from star center: 1. M=0.5Msun, 2. M=1.44Msun, 3. M=1.86Msun r (km)

EoS for Neutron Stars with a Strange Quark Core

Neutron Stars with a Strange Quark Core Yu.L.Vartanian, A.R.Harutyunian, G.B.Alaverdyan, in the Plenary Lectures and Contributed Papers, GR 15, Pune, India, December 16-21, 1997, p.159; G.B.Alaverdyan, A.R.Harutyunyan, Yu.L.Vartanyan, Spacetime and Substance, 2, 3(8), 129, 2000; G.B.Alaverdyan, A.R.Harutyunyan, Yu.L.Vartanyan, Astrophysics, 44, 265, 2001; G.B.Alaverdyan, A.R.Arutyunyan, Yu.L.Vartanyan, Astronomy Letters, 28, 24, 2002; A.R.Harutyunyan, Astrophysics, 45, 248, 2002; G.B.Alaverdyan, A.R.Harutyunyan, Yu.L.Vartanyan, Astrofizika, 46, 445, 2003.

First-order phase transition

EoS for NS with a quark core