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Bounds on the dragging rate and on the rotational mass-energy in slowly and differentially rotating relativistic stars

Abstract

For relativistic stars rotating slowly and differentially with a positive angular velocity, some properties in relation to the positiveness of the rate of rotational dragging and of the angular momentum density are derived. Also, a new proof for the bounds on the rotational mass-energy is given.Comment: 23 pages, latex. Submitted to J. Math. Phy

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    Last time updated on 03/12/2019