Five percent measurement of the gravitational constant in the Large Magellanic Cloud

Harry Desmond, Jeremy Sakstein, and Bhuvnesh Jain
Phys. Rev. D 103, 024028 – Published 13 January 2021

Abstract

We perform a novel test of general relativity by measuring the gravitational constant in the Large Magellanic Cloud (LMC). The LMC contains six well-studied Cepheid variable stars in detached eclipsing binaries. Radial velocity and photometric observations enable a complete orbital solution, and precise measurements of the Cepheids’ periods permit detailed stellar modelling. Both are sensitive to the strength of gravity, the former via Kepler’s third law and the latter through the gravitational free-fall time. We jointly fit the observables for stellar parameters and the gravitational constant. Performing a full Markov Chain Monte Carlo analysis of the parameter space including all relevant nuisance parameters, we constrain the gravitational constant in the Large Magellanic Cloud relative to the Solar System to be GLMC/GSS=0.930.04+0.05. We discuss the implications of this 5% measurement of Newton’s constant in another galaxy for dark energy and modified gravity theories. This result excludes one Cepheid, CEP-1812, which is an outlier and needs further study: it is either a highly unusual system to which our model does not apply, or it prefers GLMC<GSS at 2.6σ. We also obtain new bounds on critical parameters that appear in semianalytic descriptions of stellar processes. In particular, we measure the mixing length parameter to be α=0.900.26+0.36 (when assumed to be constant across our sample), and obtain constraints on the parameters describing turbulent dissipation and convective flux.

  • Figure
  • Figure
  • Figure
  • Received 9 December 2020
  • Accepted 22 December 2020

DOI:https://doi.org/10.1103/PhysRevD.103.024028

© 2021 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & Astrophysics

Authors & Affiliations

Harry Desmond1,*, Jeremy Sakstein2,†, and Bhuvnesh Jain3,‡

  • 1Astrophysics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford OX1 3RH, United Kingdom
  • 2Department of Physics & Astronomy, University of Hawai’i, 2505 Correa Road, Honolulu, Hawai’i, 96822, USA
  • 3Center for Particle Cosmology, Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USA

  • *harry.desmond@physics.ox.ac.uk
  • sakstein@hawaii.edu
  • bjain@physics.upenn.edu

Article Text (Subscription Required)

Click to Expand

References (Subscription Required)

Click to Expand
Issue

Vol. 103, Iss. 2 — 15 January 2021

Reuse & Permissions
Access Options
CHORUS

Article Available via CHORUS

Download Accepted Manuscript
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review D

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×