Abstract
We investigate the possibility of testing Einstein's general theory of relativity (GR) and the standard cosmological model via the EG statistic using neutral hydrogen (H i) intensity mapping. We generalize the Fourier space estimator for EG to include H i as a biased tracer of matter and forecast statistical errors using H i
clustering and lensing surveys that can be performed in the near
future, in combination with ongoing and forthcoming optical galaxy and
cosmic microwave background (CMB) surveys. We find that fractional
errors <1 per cent in the EG measurement can be
achieved in a number of cases and compare the ability of various survey
combinations to differentiate between GR and specific modified gravity
models. Measuring EG with intensity mapping and the Square Kilometre Array can provide exquisite tests of gravity at cosmological scales
Original language | English |
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Pages (from-to) | 1457-1464 |
Number of pages | 8 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 461 |
Issue number | 2 |
Early online date | 14 Jun 2016 |
DOIs | |
Publication status | Published - 11 Sept 2016 |
Keywords
- astro-ph.CO
- cosmology
- theory
- large-scale structure of the universe
- gravitational lensing: weak
- cosmology: observations
- cosmology: theory