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Home All issues Volume 502 / No 2 (August I 2009) A&A, 502 2 (2009) 605-610 Full HTML
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Table 1:

Equations of state of the neutron star core.
EOS Model Ref. $M_{\rm max}^{\rm stat}$ R1.4
      [$M_\odot$] [km]
FPS N, energy a 1.800 10.85
  density functional      
GN3 N, relativistic b 2.134 14.22
  mean field      
DH N, energy c 2.048 11.69
  density functional      
APR N, variational ${\rm d}$ 2.212 11.42
  theory      
BGN1H1 NH, energy e 1.630 12.90
  density functional      
BBB N, Brueckner theory f 1.920 11.13
GNH3 NH, relativistic g 1.964 14.20
  mean field      
GMGS-Km N + mixed h 1.454 13.12
  N-kaon condensed      
GMGS-Kp N + pure i 1.450 13.20
  N-kaon condensed      
N - nucleons and leptons. NH - nucleons, hyperons, and leptons. Exotic states of hadronic matter are indicated explicitly. Maximum allowable mass for non-rotating stars, $M_{\rm max}^{\rm stat}$, and the circumferential radius of non-rotating stars of $1.4~M_\odot$, R1.4, are given in last two columns, respectively. References for the EOSs: a - (); b - Glendenning (1985); c - Douchin & Haensel (2001); d - A18 Argonne NN potential with relativistic corrections and Urbana modified UIX* NNN potential model, from Akmal et al. (1998); e - Balberg & Gal (1997); f - Paris two-body NN potential and Urbana UIX three body NNN potential, from Baldo et al. (1997); g - Glendenning (1985); h, i - kaon condensate models with $U_K^{\rm lin}=-125~$MeV, Pons et al. (2000).

Source LaTeX | All tables | In the text

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