On the scalar-tetradic theories of gravitation - Cosmology and gravitational radiation

Mathematics – Logic

Scientific paper

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Cosmology, Gravitation Theory, Gravitational Waves, Tetrad Theory, Angular Momentum, Flux Density, Gravitational Constant, Hubble Constant, Relativity, Scalars

Scientific paper

Cosmological tetrads were constructed in order to derive the basic equations of Moller's (1978) scalar-tetradic theory of gravitation (theories A and B). It is shown that when the arbitrary dimensionless constants of theory A (W and lambda-asterisk) become too large, the losses of energy and gravitational momentum in a gravitationally bound system are the same as in general relativity. Solutions are obtained for the minimum energy density of a cosmological model based on theory A. It is demonstrated that since any nongravitationally bound system with energy density of at least 10 to the -20th and no more than 10 to the -31st g per cu cm would be consistent with experimental values for the Hubble constant and deceleration parameter q(0), no new intergalactic sources of energy are necessary for agreement with available observations.

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