On Shapiro time delay in massive scalar-tensor theories
arXiv:2111.13900 · doi:10.1088/1475-7516/2022/01/029
Abstract
The problem of determining the post-Newtonian parameter in massive scalar-tensor theories is considered. We demonstrate equivalent correspondence between the post-Newtonian parameter and the parameter appearing in the equation of null geodysic in massive scalar-tensor theories. We show that massive scalar-tensor theories can be distinguished from general relativity based on the predictions of Shapiro time delay. All calculations are presented using hybrid metric-Palatini f(R)-gravity as an example. The expression for Shapiro time delay in hybrid f(R)-gravity is obtained for the first time.
10 pages, submitted to JCAP
References in corpus (7)
- The Confrontation between General Relativity and Experiment
- Extended Theories of Gravity and their Cosmological and Astrophysical Applications
- Class of viable modified gravities describing inflation and the onset of accelerated expansion
- Modified f(R) gravity unifying R^m inflation with \LambdaCDM epoch
- Limit to General Relativity in f(R) theories of gravity
- The matter power spectrum in f(R) gravity
- Is exponential gravity a viable description for the whole cosmological history?