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Neutron Star masses from the Field Correlator Method Equation of State

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Figure

Figure 1. G2(μB) as computed in [21] (dashed green) and in [24] (dot-dashed blue) with G2(μB = 0) = 0.012GeV4
Figure 2. Pressure as a function of the baryon chemical potentialtions, and the dashed ones are the pressure derived in the FCM model for several values of the (gluon condensate μB
Figure 3. Pressure P (upper panel) and baryon density ρB (lower panel) vs. μB. The quark phase EoS is computedfor various V1 and with G2(μB) given by the solid red line in figure 1
Figure 4. The NS mass (in units of the solar mass) vs. the central baryon density (left panel) and the correspond-ing radius (right panel), for V1 = 0.01 GeV and some values of μB independent G2.
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