PreprintarXiv licencearXiv
Classical tests of New General Relativity
Abstract
In New General Relativity (NGR), the static spherically symmetric vacuum solution is characterized by two parameters, unlike General Relativity (GR), where the Schwarzschild solution has only one parameter. In this work, using the five classical tests of relativistic gravity (perihelion precession, light bending, Shapiro time delay and de Sitter geodetic precession effect, as well as gravitational redshift), a more stringent constraint on the value of the second parameter was derived compared to the original work [1].
Related
- GWTC-5.0: Tests of General Relativity
- Tests of general relativity in pseudo-Newtonian approach
- Tests of general relativity using analytic derivatives of parametrized post-Einsteinian gravitational waveforms within the Fisher-matrix framework
- The Impact of Spin Priors on Parameterized Tests of General Relativity
- Biases in Ringdown Tests of General Relativity from Gravitational-Wave Microlensing
BibTeX
@misc{vandeev2026classical,
title = {{Classical tests of New General Relativity}},
author = {V. P. Vandeev and V. A. Parkhomenko and A. N. Semenova and M. A. Matveev},
howpublished = {arXiv},
year = {2026},
month = sep,
doi = {10.48550/arxiv.2605.05500},
eprint = {2605.05500},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2605.05500},
}
RIS
TY - UNPB
TI - Classical tests of New General Relativity
AU - V. P. Vandeev
AU - V. A. Parkhomenko
AU - A. N. Semenova
AU - M. A. Matveev
PY - 2026
DA - 2026/09/05
PB - arXiv
DO - 10.48550/arxiv.2605.05500
UR - https://arxiv.org/abs/2605.05500
AB - In New General Relativity (NGR), the static spherically symmetric vacuum solution is characterized by two parameters, unlike General Relativity (GR), where the Schwarzschild solution has only one parameter. In this work, using the five classical tests of relativistic gravity (perihelion precession, light bending, Shapiro time delay and de Sitter geodetic precession effect, as well as gravitational redshift), a more stringent constraint on the value of the second parameter was derived compared to the original work [1].
ER -