Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994apj...424..846r&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 424, no. 2, p. 846-851
Astronomy and Astrophysics
Astrophysics
44
Crusts, Equations Of State, Moments Of Inertia, Neutron Stars, Relativity, Approximation, Baryons, Size (Dimensions), Stellar Interiors, Stellar Mass, Stellar Models
Scientific paper
An approximation for the moment of inertia of a neutron star in terms of only its mass and radius is presented, and insight into it is obtained by examining the behavior of the relativistic structural equations. The approximation is accurate to approximately 10% for a variety of nuclear equations of state, for all except very low mass stars. It is combined with information about the neutron-star crust to obtain a simple expression (again in terms only of mass and radius) for the fractional moment of inertia of the crust.
Pethick Christopher J.
Ravenhall D. G.
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