IMPLICATIONS OF THE CRUSTAL MOMENT OF INERTIA FOR NEUTRON-STAR EQUATIONS OF STATE

Authors
Citation
B. Datta et Ma. Alpar, IMPLICATIONS OF THE CRUSTAL MOMENT OF INERTIA FOR NEUTRON-STAR EQUATIONS OF STATE, Astronomy and astrophysics, 275(1), 1993, pp. 210-212
Citations number
23
Categorie Soggetti
Astronomy & Astrophysics
Journal title
ISSN journal
00046361
Volume
275
Issue
1
Year of publication
1993
Pages
210 - 212
Database
ISI
SICI code
0004-6361(1993)275:1<210:IOTCMO>2.0.ZU;2-A
Abstract
The dynamical models for neutron star glitches and postglitch behaviou r, and the information they yield on the crustal moment of inertia, ar e applied to a catalogue of neutron star models. The implications for neutron star equations of state are discussed. The postglitch timing d ata 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.