Table 2 Mass, radius, and total moment of inertia of glitching pulsars for three nuclear equation of state models.
PSRM (MSun)R (km)I (MSun km2)
BSk20 EOS
J0537−6910Embedded ImageEmbedded ImageEmbedded Image
B0833−45Embedded ImageEmbedded ImageEmbedded Image
B1046−58Embedded ImageEmbedded ImageEmbedded Image
B1338−62Embedded ImageEmbedded ImageEmbedded Image
B1706−44Embedded ImageEmbedded ImageEmbedded Image
B1757−24Embedded ImageEmbedded ImageEmbedded Image
B1800−21Embedded ImageEmbedded ImageEmbedded Image
B1823−13Embedded ImageEmbedded ImageEmbedded Image
1E 1841−045Embedded ImageEmbedded ImageEmbedded Image
BSk21 EOS
J0537−6910Embedded ImageEmbedded ImageEmbedded Image
B0833−45Embedded ImageEmbedded ImageEmbedded Image
B1046−58Embedded ImageEmbedded ImageEmbedded Image
B1338−62Embedded ImageEmbedded ImageEmbedded Image
B1706−44Embedded ImageEmbedded ImageEmbedded Image
B1757−24Embedded ImageEmbedded ImageEmbedded Image
B1800−21Embedded ImageEmbedded ImageEmbedded Image
B1823−13≥ 1.71≤ 12.6≥ 88.9
1E 1841−045Embedded ImageEmbedded ImageEmbedded Image
APR EOS
J0537−6910Embedded ImageEmbedded ImageEmbedded Image
B0833−45Embedded ImageEmbedded ImageEmbedded Image
B1046−58Embedded ImageEmbedded ImageEmbedded Image
B1338−62Embedded ImageEmbedded ImageEmbedded Image
B1706−44Embedded ImageEmbedded ImageEmbedded Image
B1757−24Embedded ImageEmbedded ImageEmbedded Image
B1800−21Embedded ImageEmbedded ImageEmbedded Image
B1823−13Embedded ImageEmbedded ImageEmbedded Image
1E 1841−045Embedded ImageEmbedded ImageEmbedded Image