Exact solution and Classical tests of New General Relativity
General Relativity and Quantum Cosmology
2026-05-08 v1
Abstract
In this work, we present an exact static spherically symmetric vacuum solution of the New General Relativity (NGR) field equations. Unlike the Schwarzschild solution in General Relativity (GR), this solution is characterized by two parameters. Subsequently, using the four classical tests of relativistic gravity (perihelion precession, light bending, Shapiro time delay and gravitational redshift), a more stringent constraint on the value of the second parameter was derived compared to the original work [1].
Keywords
Cite
@article{arxiv.2605.05500,
title = {Exact solution and Classical tests of New General Relativity},
author = {V. P. Vandeev and V. A. Parkhomenko and A. N. Semenova},
journal= {arXiv preprint arXiv:2605.05500},
year = {2026}
}