We compute the non-Gaussian contribution to the covariance of the matter power spectrum at one-loop order in standard perturbation theory (SPT), using the framework of the effective field theory (EFT) of large scale structure (LSS). The complete one-loop contributions are evaluated for the first time, including the leading EFT corrections that involve seven independent operators, of which four appear in the power spectrum and bispectrum. We compare the non-Gaussian part of the one-loop covariance computed with both SPT and EFT of LSS to two separate simulations. In one simulation, we find that the one-loop prediction from SPT reproduces the simulation well to k_i + k_j ∼ 0.25 h/Mpc, while in the other simulation we find a substantial improv...
AbstractIn order to infer the impact of the small-scale physics to the large-scale properties of the...
Accurate power spectrum (or correlation function) covariance matrices are a crucial requirement for ...
The main aim of this thesis is to investigate new methods beyond standard perturbation theory (SPT) ...
We compute the non-Gaussian contribution to the covariance of the matter power spectrum at one-loop ...
We compute the connected four point correlation function (the trispectrum in Fourier space) of cosmo...
The consistency relations in large scale structure relate the lower-order correlation functions with...
Gravitational clustering is an intrinsically non-linear process that generates significant non-Gauss...
We study the power spectrum of dark matter density fluctuations in the framework of the Effective Fi...
After the successful full-shape analyses of BOSS data using the Effective Field Theory of Large-Scal...
In the search for understanding the initial conditions of the universe, it is crucial describe with ...
We study the power spectrum of dark matter density fluctuations in the framework of the Effective Fi...
Large scale structure surveys promise to be the next leading probe of cosmological information. It i...
Using a diagrammatic approach to Eulerian perturbation theory, we analytically calculate the varianc...
We generalize previously derived analytic results for the one-loop power spectrum (PS) in scale-free...
The Large Scale Structure (LSS) of the Universe, that being the large scale distribution of dark and...
AbstractIn order to infer the impact of the small-scale physics to the large-scale properties of the...
Accurate power spectrum (or correlation function) covariance matrices are a crucial requirement for ...
The main aim of this thesis is to investigate new methods beyond standard perturbation theory (SPT) ...
We compute the non-Gaussian contribution to the covariance of the matter power spectrum at one-loop ...
We compute the connected four point correlation function (the trispectrum in Fourier space) of cosmo...
The consistency relations in large scale structure relate the lower-order correlation functions with...
Gravitational clustering is an intrinsically non-linear process that generates significant non-Gauss...
We study the power spectrum of dark matter density fluctuations in the framework of the Effective Fi...
After the successful full-shape analyses of BOSS data using the Effective Field Theory of Large-Scal...
In the search for understanding the initial conditions of the universe, it is crucial describe with ...
We study the power spectrum of dark matter density fluctuations in the framework of the Effective Fi...
Large scale structure surveys promise to be the next leading probe of cosmological information. It i...
Using a diagrammatic approach to Eulerian perturbation theory, we analytically calculate the varianc...
We generalize previously derived analytic results for the one-loop power spectrum (PS) in scale-free...
The Large Scale Structure (LSS) of the Universe, that being the large scale distribution of dark and...
AbstractIn order to infer the impact of the small-scale physics to the large-scale properties of the...
Accurate power spectrum (or correlation function) covariance matrices are a crucial requirement for ...
The main aim of this thesis is to investigate new methods beyond standard perturbation theory (SPT) ...