Fig. 1.
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Comparison of the NS mass-radius relation of four different equations of state (EoS s) with the LIGO/Virgo constraints from NS-NS merger GW170817 (90% credible limits shown by green and blue boxes: Abbott et al. 2018a). We employ the MPA1 EoS, which reaches ∼2.5 M⊙ (our adopted maximum NS mass) and agrees with the LIGO/Virgo constraints. Other relations are WFF1 (Wiringa et al. 1988), APR4 (Akmal et al. 1998), and DD2 (Alvarez-Castillo et al. 2016).
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