Speaker
Jessica Muir
(Perimeter Institute)
Description
Measurements of the large-scale distribution of matter in the Universe are one of our primary tools for testing the predictions of general relativity on cosmological scales. I will describe how we pursue this using data from galaxy imaging surveys, focusing on Dark Energy Survey galaxy clustering and weak lensing analyses as an example. I will highlight results from the DES Year 3 analysis that are relevant for testing gravity, some practical aspects of extending survey analyses beyond ΛCDM, as well as ongoing work to address these challenges to prepare for future surveys.
arXiv reference, if applicable: | https://arxiv.org/abs/2207.05766 |
---|---|
Contact Email | [email protected] |
Primary author
Jessica Muir
(Perimeter Institute)
External references
- 24070069
- 69bbf9fd-5a22-447d-9165-4b2d56815921