Abstract. We study the bispectrum in the Effective Field Theory of Large Scale Struc-ture, consistently accounting for the effects of short-scale dynamics. We begin by proving that, as long as the theory is perturbative, it can be formulated to arbitrary order us-ing only operators that are local in time. We then derive all the new operators required to cancel the UV-divergences and obtain a physically meaningful prediction for the one-loop bispectrum. In addition to new, subleading stochastic noises and the viscosity term needed for the one-loop power spectrum, we find three new effective operators. The three new parameters can be constrained by comparing with N-body simulations. The best fit is precisely what is suggested by the structure...
We present a complete framework for numerical calculation of the power spectrum and bispectrum in ca...
We present a new observable, position-dependent power spectrum, to measure the large-scale structure...
The bispectrum, the three-point function of density fluctuations in Fourier space, is the lowest ord...
Given the importance of future large scale structure surveys for delivering new cosmological informa...
We provide a comparison between the matter bispectrum derived with different flavours of perturbatio...
We present measurements of the dark matter bispectrum in N-body simulations with non-Gaussian initia...
We have accurately measured the bispectrum for four scale-free models of structure formation with th...
Aims. We investigate how unified models should be built to be able to predict the matter-d...
We study the power spectrum of dark matter density fluctuations in the framework of the Effective Fi...
International audienceThe large-scale matter distribution in the late-time Universe exhibits gravity...
We apply an orthogonalization procedure on the effective field theory of large scale structure (EFT ...
We study the power spectrum of dark matter density fluctuations in the framework of the Effective Fi...
Dark matter evolution during the process of cosmological structure formation can be described in ter...
We compute the non-Gaussian contribution to the covariance of the matter power spectrum at one-loop ...
A perturbative description of Large Scale Structure is a cornerstone of our understanding of the obs...
We present a complete framework for numerical calculation of the power spectrum and bispectrum in ca...
We present a new observable, position-dependent power spectrum, to measure the large-scale structure...
The bispectrum, the three-point function of density fluctuations in Fourier space, is the lowest ord...
Given the importance of future large scale structure surveys for delivering new cosmological informa...
We provide a comparison between the matter bispectrum derived with different flavours of perturbatio...
We present measurements of the dark matter bispectrum in N-body simulations with non-Gaussian initia...
We have accurately measured the bispectrum for four scale-free models of structure formation with th...
Aims. We investigate how unified models should be built to be able to predict the matter-d...
We study the power spectrum of dark matter density fluctuations in the framework of the Effective Fi...
International audienceThe large-scale matter distribution in the late-time Universe exhibits gravity...
We apply an orthogonalization procedure on the effective field theory of large scale structure (EFT ...
We study the power spectrum of dark matter density fluctuations in the framework of the Effective Fi...
Dark matter evolution during the process of cosmological structure formation can be described in ter...
We compute the non-Gaussian contribution to the covariance of the matter power spectrum at one-loop ...
A perturbative description of Large Scale Structure is a cornerstone of our understanding of the obs...
We present a complete framework for numerical calculation of the power spectrum and bispectrum in ca...
We present a new observable, position-dependent power spectrum, to measure the large-scale structure...
The bispectrum, the three-point function of density fluctuations in Fourier space, is the lowest ord...