Measuring anisotropic stress with relativistic effects
Daniel Sobral-Blanco, Camille Bonvin

TL;DR
This paper introduces a new method to directly measure anisotropic stress in the universe by using relativistic effects in galaxy counts, bypassing assumptions about dark matter and enabling tests of gravity theories.
Contribution
The paper proposes a novel observational technique that directly measures anisotropic stress using relativistic effects, independent of dark matter assumptions.
Findings
Method enables direct measurement of anisotropic stress.
Relativistic effects in galaxy counts are key to the measurement.
Provides a new test for theories of gravity.
Abstract
One of the main goal of large-scale structure surveys is to test the consistency of General Relativity at cosmological scales. In the CDM model of cosmology, the relations between the fields describing the geometry and the content of our Universe are uniquely determined. In particular, the two gravitational potentials -- that describe the spatial and temporal fluctuations in the geometry -- are equal. Whereas large classes of dark energy models preserve this equality, theories of modified gravity generally create a difference between the potentials, known as anisotropic stress. Even though measuring this anisotropic stress is one of the key goals of large-scale structure surveys, there are currently no methods able to measure it directly. Current methods all rely on measurements of galaxy peculiar velocities (through redshift-space distortions), from which the time component of…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
