English

The EFT Likelihood for Large-Scale Structure

Cosmology and Nongalactic Astrophysics 2020-05-06 v2 High Energy Physics - Theory

Abstract

We derive, using functional methods and the bias expansion, the conditional likelihood for observing a specific tracer field given an underlying matter field. This likelihood is necessary for Bayesian-inference methods. If we neglect all stochastic terms apart from the ones appearing in the auto two-point function of tracers, we recover the result of Schmidt et al., 2018. We then rigorously derive the corrections to this result, such as those coming from a non-Gaussian stochasticity (which include the stochastic corrections to the tracer bispectrum) and higher-derivative terms. We discuss how these corrections can affect current applications of Bayesian inference. We comment on possible extensions to our result, with a particular eye towards primordial non-Gaussianity. This work puts on solid theoretical grounds the EFT-based approach to Bayesian forward modeling.

Keywords

Cite

@article{arxiv.1909.04022,
  title  = {The EFT Likelihood for Large-Scale Structure},
  author = {Giovanni Cabass and Fabian Schmidt},
  journal= {arXiv preprint arXiv:1909.04022},
  year   = {2020}
}

Comments

53 pages (36+17), 4 tables. v2: matches JCAP version. Added section to compare with Schmidt et al., 2018; added plot to show relative importance of different contributions to log-likelihood