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- W42688086 abstract "The parameters of differentially rotating white dwarfs are planted by means of the energy method for various fixed values of the angular momentum. In particular, the dependence of the mass M on the central density, i.e., the curves of M/sub k/ (rho/sub c/) is found. In the calculations account is taken of the effect of ..beta.. capture and general relativity. It is shown that fast rotation suppresses the effects of ..beta.. capture and general relativity and makes possible the existence of stable white dwarfs with masses up to three solar masses and central densities two orders of magnitude greater than the density of static configurations." @default.
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- W42688086 date "1975-01-01" @default.
- W42688086 modified "2023-09-27" @default.
- W42688086 title "Rapidly rotating massive white dwarfs. [Angular momentum, masses, central densities]" @default.
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