Advances in High Energy Physics / 2009 / Article / Tab 2

Research Article

The Density-Dependent Correlations among Observables in Nuclear Matter and Hyperon-Rich Neutron Stars

Table 2

The maximum masses, , and central energy densities, ( , of neutron stars produced by way of (a) ( )-( ) and (b) ( )-( ) are listed, respectively, with the same coupling constants. The EOS of the hyperon phase ( ) and ( ) is calculated with the ratio [26].
(a)

( )-( )


1.002.222.14
2/32.082.24
1/31.931.21

(b)

( )-( )


1.002.222.15
2/31.671.00
1/31.561.02

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