Gravitational Field of Non-conserving Mass Particle
Ghanshyam H. Jadhav
Abstract
Open-access reader
Ghanshyam H. Jadhav
Abstract
Open-access reader
Gravitational field equations are written in the form of Maxwell’s type field equations. Lorentz gauge on the gravitational scalar and vector potentials is discarded by introducing a gravitational scalar field. It makes the mass particles to be time-dependent. The non-conserving part of the mass causes to produce the gravitational scalar field, which further con-tributes to the gravitational and gravitomagnetic vector fields. This contribution makes possible to produce a repulsive gravitational field by a decaying mass particle beyond a critical distance.
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Gravitational field equations are written in the form of Maxwell’s type field equations. Lorentz gauge on the gravitational scalar and vector potentials is discarded by introducing a gravitational scalar field. It makes the mass particles to be time-dependent. The non-conserving part of the mass causes to produce the gravitational scalar field, which further con-tributes to the gravitational and gravitomagnetic vector fields. This contribution makes possible to produce a repulsive gravitational field by a decaying mass particle beyond a critical distance.
Key concepts: Physics, Gravitational field, Gravitation, Speed of gravity, Scalar (mathematics), Gravitational redshift, Scalar field, Classical field theory