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- W146475139 abstract "It is shown that the repulsive shadow potential, introduced recently in theories of gravitation by Chiang, Dykla and Hwang, can stabilize, from a dynamical point of view, supermassive stars of mass M approximately less than or equal to 10/sup 8/ M/sub mass/. The value of the strength of this repulsive interaction necessary to ensure dynamical stability on the main sequence is found to be compatible with data concerning supermassive stars. For stars of mass higher than 10/sup 8/ M/sub mass/, a well developed space-time geometric theory of gravitation with shadow effect is necessary to come to a decision regarding their dynamical stability." @default.
- W146475139 created "2016-06-24" @default.
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- W146475139 date "1977-01-01" @default.
- W146475139 modified "2023-09-27" @default.
- W146475139 title "Possible dynamical stabilization of relativistic supermassive stars by a shadow gravitational potential" @default.
- W146475139 hasPublicationYear "1977" @default.
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