1. On the Einstein tensor field equation and the Newman-Penrose spinor field equations
- Author
-
Ewald J. H. Wessels
- Subjects
Physics ,General Relativity and Quantum Cosmology ,Einstein tensor ,symbols.namesake ,Exact solutions in general relativity ,Gravitational field ,Observer (quantum physics) ,Spinor field ,Einstein field equations ,symbols ,Schwarzschild metric ,Mathematical physics ,Reference frame - Abstract
Since the publication of the Newman-Penrose (“NP”) equations in 1962 they have been regarded as simply a different version of the Einstein field equations (“EFEs”). This paper reports the fact that symmetry methods can be employed to reduce the complexity of the NP equations, reformulated in terms of the elements of the metric tensor rather than the spin coefficients, and to derive the exact solution in the reference frame of an observer who is in radial free fall through the external vacuum gravitational field of an isolated, non-rotating, spherically symmetric gravitating body. While the domain of the solution is confined to the axis along which the observer falls, it can be directly compared to the Schwarzschild solution and is shown to differ from that solution.Since the publication of the Newman-Penrose (“NP”) equations in 1962 they have been regarded as simply a different version of the Einstein field equations (“EFEs”). This paper reports the fact that symmetry methods can be employed to reduce the complexity of the NP equations, reformulated in terms of the elements of the metric tensor rather than the spin coefficients, and to derive the exact solution in the reference frame of an observer who is in radial free fall through the external vacuum gravitational field of an isolated, non-rotating, spherically symmetric gravitating body. While the domain of the solution is confined to the axis along which the observer falls, it can be directly compared to the Schwarzschild solution and is shown to differ from that solution.
- Published
- 2019
- Full Text
- View/download PDF