On Shapiro time delay in massive scalar-tensor theories
P. I. Dyadina, S. P. Labazova

TL;DR
This paper investigates how massive scalar-tensor theories affect the Shapiro time delay, providing new expressions and demonstrating potential observational differences from general relativity.
Contribution
It establishes a correspondence between the post-Newtonian parameter and null geodesics in massive scalar-tensor theories, and derives the first expression for Shapiro delay in hybrid f(R)-gravity.
Findings
Massive scalar-tensor theories predict distinguishable Shapiro delays from general relativity.
Derived the first formula for Shapiro time delay in hybrid f(R)-gravity.
Showed the equivalence between post-Newtonian parameter γ and null geodesic parameters.
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.
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