# Recent Progress in Large-Scale Structure

- Institution: CERN
- Department: TH Theoretical Seminar
- Speaker: Roman Scoccimarro
- Year: 2014
- Language: English
- Source: [CERN](https://videos.cern.ch/record/3009626)
- Licence: [CERN](http://copyright.web.cern.ch)
- Who can watch: Teens profiles and older (sources give no ratings; placed by Invisible Network from the source's own words)

I will discuss recent progress in the understanding of how to model galaxy clustering. While recent analyses have focussed on the baryon acoustic oscillations as a probe of cosmology, galaxy redshift surveys contain a lot more information than the acoustic scale. In extracting this additional information three main issues need to be well understood: nonlinear evolution of matter fluctuations, galaxy bias and redshift-space distortions. I will present recent progress in modeling these three effects that pave the way to constraining cosmology and galaxy formation with increased precision..

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## Lectures

1. [Recent Progress in Large-Scale Structure](https://invisiblenetwork.ai/learn/cern/3009626/754bcf6a5422), 1 h 7 min (CERN's player)