Implications of the Crustal Moment of Inertia for Neutron Star Equations of State

Details Implications of the Crustal Moment of Inertia for Neutron Star Equations of State Implications of the Crustal Moment of Inertia for Neutron Star Equations of State

Aug 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...275..210d&link_type=abstract

Astronomy and Astrophysics, Vol.275, NO. 1/AUG(I), P. 210, 1993

Astronomy and Astrophysics

Astrophysics

12

Neutron Star: Equation Of State, Neutron Star: Glitches

Scientific paper

The dynamical models for neutron star glitches and postglitch behaviour, and the information they yield on the crustal moment of inertia, are applied to a catalogue of neutron star models. The implications for neutron star equations of state are discussed. The postglitch timing data from the Vela pulsar are interpreted to rule out one of the softer equations of state for neutron matter with an admixture of hyperons, if the neutron star mass is 1.4 solar mass.

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