# Probing Massive Scalar Fields from a Pulsar in a Stellar Triple System

## TL;DR

This paper develops a formalism to test massive scalar fields using pulsar timing in a triple system, setting new constraints on alternative gravity theories beyond general relativity.

## Contribution

It introduces a generic framework for analyzing fifth forces from massive scalar fields in pulsar systems, and applies it to derive the strongest bounds from PSR J0337+1715 data.

## Key findings

- Strongest bounds on massive scalar fields from pulsar timing
- Constraints on theories with axions and dark matter mediators
- Triple system J0337 is a powerful test for alternative gravity models

## Abstract

Pulsar timing observations precisely test general relativity. Recently, the hierarchical triple system PSR J0337+1715 has placed new constraints on the existence of a fifth force from violation in the strong equivalence principle. Many alternative gravity theories exist with massive (pseudo-)scalar fields to explain a variety of phenomena from the accelerating expansion of the universe at large scales to the QCD strong CP problem at small scales. We here develop a generic formalism for the fifth force effect in theories involving massive scalar fields arising from e.g. string theory. With PSR J0337 measurements, we find the strongest bound on the simplest theory with a massive scalar field beyond general relativity and derive new constraints in other theories with axions, dark matter mediators, and higher-curvature corrections. These results show that the triple system J0337 provides a stringent test for massive scalar fields.