Slow rotation in the bimetric theory of gravitation.

Details Slow rotation in the bimetric theory of gravitation. Slow rotation in the bimetric theory of gravitation.

Mar 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979gregr..10..343f&link_type=abstract

General Relativity and Gravitation, Volume 10, Issue 4, pp.343-349

Physics

7

Gravitation:Neutron Stars, Gravitation Theory

Scientific paper

The equations describing the moment of inertia and the dragging of inertial frames of slowly rotating neutron stars are derived according to Rosen's bimetric theory of gravitation. Numerical calculations of the properties of neutron stars according to the bimetric theory and general relativity were made using several equations of state. The general trend found is that in the bimetric theory neutron stars with a given mass induce a smaller dragging of inertial frames than in general relativity. The moment of inertia of low-mass stars also is smaller in the bimetric theory. For high-mass stars, however, the moment of inertia is found to be larger in the bimetric theory.

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