Projects per year
The Vainshtein mechanism, present in many models of gravity, is very effective at screening dark matter halos such that the fifth force is negligible and general relativity is recovered within their Vainshtein radii. Vainshtein screening is independent of halo mass and environment, in contrast to e.g. chameleon screening, making it difficult to test. However, our previous studies have found that the dark matter particles in filaments, walls, and voids are not screened by the Vainshtein mechanism. We therefore investigate whether cosmic voids, identified as local density minima using a watershed technique, can be used to test models of gravity that exhibit Vainshtein screening. We measure density, velocity, and screening profiles of stacked voids in cosmological N-body simulations using both dark matter particles and dark matter halos as tracers of the density field. We find that the voids are completely unscreened, and the tangential velocity and velocity dispersion profiles of stacked voids show a clear deviation from ΛCDM at all radii. Voids have the potential to provide a powerful test of gravity on cosmological scales.
|Number of pages||11|
|Journal||Monthly Notices of the Royal Astronomical Society|
|Early online date||22 Dec 2017|
|Publication status||Published - 11 Apr 2018|
- dark energy
- large-scale structure of Universe
- methods: numercal
FingerprintDive into the research topics of 'Using voids to unscreen modified gravity'. Together they form a unique fingerprint.
- 1 Finished