scholarly journals Impact of bias and redshift-space modelling for the halo power spectrum: testing the effective field theory of large-scale structure

2020 ◽  
Vol 2020 (07) ◽  
pp. 011-011 ◽  
Author(s):  
Lucía Fonseca de la Bella ◽  
Donough Regan ◽  
David Seery ◽  
David Parkinson
2020 ◽  
Vol 102 (12) ◽  
Author(s):  
Takahiro Nishimichi ◽  
Guido D’Amico ◽  
Mikhail M. Ivanov ◽  
Leonardo Senatore ◽  
Marko Simonović ◽  
...  

2016 ◽  
Vol 93 (12) ◽  
Author(s):  
Daniele Bertolini ◽  
Katelin Schutz ◽  
Mikhail P. Solon ◽  
Jonathan R. Walsh ◽  
Kathryn M. Zurek

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

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.


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