X-ray pulsed light curves of highly compact neutron stars as probes of scalar-tensor theories of gravity

TL;DR

This paper investigates how X-ray pulsed light curves from neutron stars can be used to test scalar-tensor theories of gravity, revealing significant deviations from general relativity in high-compactness regimes.

Contribution

It introduces a detailed model of neutron star X-ray light curves within scalar-tensor theories, highlighting their potential to constrain deviations from general relativity.

Findings

Flux differences up to 80% compared to GR

Neutron star radius deviations up to 10% in STT

High-compactness regimes enhance sensitivity to scalar charges

Abstract

The strong gravitational potential of neutron stars (NSs) makes them ideal astrophysical objects for testing extreme gravity phenomena. We explore the potential of NS X-ray pulsed lightcurve observations to probe deviations from general relativity (GR) within the scalar-tensor theory (STT) of gravity framework. We compute the flux from a single, circular, finite-size hot spot, accounting for light bending, Shapiro time delay, and Doppler effect. We focus on the high-compactness regime, i.e., close to the critical GR value GM/(Rc^2) = 0.284, over which multiple images of the spot appear and impact crucially the lightcurve. Our investigation is motivated by the increased sensitivity of the pulse to the scalar charge of the spacetime in such high compactness regimes, making these systems exceptionally suitable for scrutinizing deviations from GR, notably phenomena such as spontaneous scalarization, as predicted by STT. We find significant differences in NS observables, e.g., the flux of a single spot can differ up to 80% with respect to GR. Additionally, reasonable choices for the STT parameters that satisfy astrophysical constraints lead to changes in the NS radius relative to GR of up to approximately 10%. Consequently, scalar parameters might be better constrained when uncertainties in NS radii decrease, where this could occur with the advent of next-generation gravitational wave detectors, such as the Einstein Telescope and LISA, as well as future electromagnetic missions like eXTP and ATHENA. Thus, our findings suggest that accurate X-ray data of the NS surface emission, jointly with refined theoretical models, could constrain STTs.