scholarly journals Dark energy and modified gravity in the Effective Field Theory of Large-Scale Structure

2018 ◽  
Vol 2018 (04) ◽  
pp. 005-005 ◽  
Author(s):  
Giulia Cusin ◽  
Matthew Lewandowski ◽  
Filippo Vernizzi
2018 ◽  
Vol 2018 (04) ◽  
pp. 063-063 ◽  
Author(s):  
Benjamin Bose ◽  
Kazuya Koyama ◽  
Matthew Lewandowski ◽  
Filippo Vernizzi ◽  
Hans A. Winther

Universe ◽  
2019 ◽  
Vol 5 (6) ◽  
pp. 138 ◽  
Author(s):  
Louis Perenon ◽  
Hermano Velten

We summarize the effective field theory of dark energy construction to explore observable predictions of linear Horndeski theories. We review the diagnostic of these theories on the correlation of the large-scale structure phenomenological functions: the effective Newton constant, the light deflection parameter, and the growth function of matter perturbations. We take this opportunity to discuss the evolution of the bounds the propagation speed of gravitational waves has undergone and use the most restrictive one to update the diagnostic.


Author(s):  
Tobias Baldauf

The lectures featured in this chapter review the observables relevant to the large-scale structure (LSS) of our Universe. The chapter introduces an effective field theory (EFT) that allows us to analytically describe the growth of fluctuations into the non-linear era, with uncertainties better controlled than in classical linear perturbation theory. Topics covered in the chapter include random fields in three-dimensional space, Fourier space conventions, the shape of the matter power spectrum, Gaussian random fields, estimators and cosmic variance, dynamics in the Newtonian regime, a perturbative solution of the fluid equations, the EFT approach, the Lagrangian perturbation theory, biased tracers, and redshift space distortions.


2016 ◽  
Vol 2016 (06) ◽  
pp. 052-052 ◽  
Author(s):  
Daniele Bertolini ◽  
Katelin Schutz ◽  
Mikhail P. Solon ◽  
Kathryn M. Zurek

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