Consistency Relations in Effective Field Theory
arXiv:1705.07866 · doi:10.1088/1475-7516/2017/06/042
Abstract
The consistency relations in large scale structure relate the lower-order correlation functions with their higher-order counterparts. They are direct outcome of the underlying symmetries of a dynamical system and can be tested using data from future surveys such as Euclid. Using techniques from standard perturbation theory (SPT), previous studies of consistency relation have concentrated on continuity-momentum (Euler)-Poisson system of an ideal fluid. We investigate the consistency relations in effective field theory (EFT) which adjusts the SPT predictions to account for the departure from the ideal fluid description on small scales. We provide detailed results for the 3D density contrast as well as the {\em scaled} divergence of velocity . Assuming a CDM background cosmology, we find the correction to SPT results becomes important at and that the suppression from EFT to SPT results that scales as square of the wave number , can reach of the total at at . We have also investigated whether effective field theory corrections to models of primordial non-Gaussianity can alter the squeezed limit behaviour, finding the results to be rather insensitive to these counterterms. In addition, we present the EFT corrections to the squeezed limit of the bispectrum in redshift space which may be of interest for tests of theories of modified gravity.
23 pages + bibliography, 6 figures. Minor changes to match version accepted for publication by JCAP
References in corpus (19)
- The Effective Field Theory of Cosmological Large Scale Structures
- Resumming Cosmological Perturbations via the Lagrangian Picture: One-loop Results in Real Space and in Redshift Space
- Nonlinear Evolution of Baryon Acoustic Oscillations
- The IR-resummed Effective Field Theory of Large Scale Structures
- A critical look at cosmological perturbation theory techniques
- A Closure Theory for Non-linear Evolution of Cosmological Power Spectra
- The Bispectrum in the Effective Field Theory of Large Scale Structure
- Dark matter clustering: a simple renormalization group approach
- Position-dependent power spectrum of the large-scale structure: a novel method to measure the squeezed-limit bispectrum
- Third-Order Density Perturbation and One-Loop Power Spectrum in Dark-Energy-Dominated Universe
- Baryonic Acoustic Oscillations via the Renormalization Group
- Third-order Perturbation Theory With Non-linear Pressure
- Renormalized Newtonian Cosmic Evolution with Primordial Non-Gaussianity
- Principal Shapes and Squeezed Limits in the Effective Field Theory of Large Scale Structure
- Non-local bias in the halo bispectrum with primordial non-Gaussianity
- Three-Point Correlations in f(R) Models of Gravity
- The Integrated Bispectrum and Beyond
- The Integrated Bispectrum in Modified Gravity Theories
- Exact Third-Order Density Perturbation and One-Loop Power Spectrum in General Dark Energy Models