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The stability of stars with potential-dependent masses
Authors:Vladimír Majerník  Jozef Gembarovi?
Institution:(1) Katedra fyziky Pedagogickej fakulty, Nitra, Czechoslovakia
Abstract:We calculate the effective mass of a spherical star-like object under the assumption that the mass of an object represents a function of the gravitational potential in which it occurs. We show that due to this mass-dependence on the gravitational potential, it is not possible that a star of a larger mass than that of a neutron star shrinks to a point singularity. We present the value of the upper limits to the mass of spherical mass bodies as a function of their radii in a large range of their mass densities.
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