Built on

Y. B. Zel’dovich, Gravitational instability: An approximate theory for large density perturbations
1970
Earlier work this paper cites.
T. Buchert, A class of solutions in Newtonian cosmology and the pancake theory
1989
Earlier work this paper cites.
F. Moutarde, J.-M. Alimi, F. R. Bouchet, R. Pellat, and A. Ramani, Precollapse scale invariance in gravitational instability
1991
Earlier work this paper cites.
F. R. Bouchet, S. Colombi, E. Hivon, and R. Juszkiewicz, Perturbative Lagrangian approach to gravitational instability
1995
Earlier work this paper cites.
E. Hivon, F. R. Bouchet, S. Colombi, and R. Juszkiewicz, Redshift distortions of clustering: a Lagrangian approach
1995
Earlier work this paper cites.
S. Bharadwaj, The Evolution of Correlation Functions in the Zeldovich Approximation and Its Implications for the Validity of Perturbation Theory
1996
Earlier work this paper cites.
A. N. Taylor and A. J. S. Hamilton, Non-linear cosmological power spectra in real and redshift space
1996
Earlier work this paper cites.
F. Bernardeau, S. Colombi, E. Gaztañaga, and R. Scoccimarro, Large-scale structure of the Universe and cosmological perturbation theory
2002
Earlier work this paper cites.
M. White, The Mass Function
2002
Earlier work this paper cites.
T. Matsubara, Resumming cosmological perturbations via the Lagrangian picture: One-loop results in real space and in redshift space
Original
2008
Earlier work this paper cites.
T. Matsubara, Nonlinear perturbation theory with halo bias and redshift-space distortions via the Lagrangian picture
Original
2008
Earlier work this paper cites.
N. Padmanabhan and M. White, Calibrating the baryon oscillation ruler for matter and halos
Original
2009
Earlier work this paper cites.
N. Padmanabhan, M. White, and J. D. Cohn, Reconstructing baryon oscillations: A Lagrangian theory perspective
Original
2009
Earlier work this paper cites.
Y. Noh, M. White, and N. Padmanabhan, Reconstructing baryon oscillations
Original
2009
Earlier work this paper cites.
C. Rampf and T. Buchert, Lagrangian perturbations and the matter bispectrum I: fourth-order model for non-linear clustering
Original
2012
Earlier work this paper cites.

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Then

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2014
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S. M. Carroll, S. Leichenauer, and J. Pollack, Consistent effective theory of long-wavelength cosmological perturbations
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S. Tassev, Lagrangian or Eulerian; real or Fourier? Not all approaches to large-scale structure are created equal
Original
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2015

A Lagrangian effective field theory

Vlah, Zvonimir, White, Martin, Aviles, Alejandro

Understand

We have continued the development of Lagrangian, cosmological perturbation theory for the low-order correlators of the matter density field.

We provide a new route to understanding how the effective field theory (EFT) of large-scale structure can be formulated in the Lagrandian framework and a new resummation scheme, comparing our results to earlier work and to a series of high-resolution N-body simulations in both Fourier and configuration space.
The `new' terms arising from EFT serve to tame the dependence of perturbation theory on small-scale physics and improve agreement with simulations (though with an additional free parameter).
We find that all of our models fare well on scales larger than about two to three times the non-linear scale, but fail as the non-linear scale is approached.

Built on

Y. B. Zel’dovich, Gravitational instability: An approximate theory for large density perturbations
1970
Earlier work this paper cites.
T. Buchert, A class of solutions in Newtonian cosmology and the pancake theory
1989
Earlier work this paper cites.
F. Moutarde, J.-M. Alimi, F. R. Bouchet, R. Pellat, and A. Ramani, Precollapse scale invariance in gravitational instability
1991
Earlier work this paper cites.
F. R. Bouchet, S. Colombi, E. Hivon, and R. Juszkiewicz, Perturbative Lagrangian approach to gravitational instability
1995
Earlier work this paper cites.
E. Hivon, F. R. Bouchet, S. Colombi, and R. Juszkiewicz, Redshift distortions of clustering: a Lagrangian approach
1995
Earlier work this paper cites.
S. Bharadwaj, The Evolution of Correlation Functions in the Zeldovich Approximation and Its Implications for the Validity of Perturbation Theory
1996
Earlier work this paper cites.
A. N. Taylor and A. J. S. Hamilton, Non-linear cosmological power spectra in real and redshift space
1996
Earlier work this paper cites.
F. Bernardeau, S. Colombi, E. Gaztañaga, and R. Scoccimarro, Large-scale structure of the Universe and cosmological perturbation theory
2002
Earlier work this paper cites.
M. White, The Mass Function
2002
Earlier work this paper cites.
T. Matsubara, Resumming cosmological perturbations via the Lagrangian picture: One-loop results in real space and in redshift space
Original
2008
Earlier work this paper cites.
T. Matsubara, Nonlinear perturbation theory with halo bias and redshift-space distortions via the Lagrangian picture
Original
2008
Earlier work this paper cites.
N. Padmanabhan and M. White, Calibrating the baryon oscillation ruler for matter and halos
Original
2009
Earlier work this paper cites.
N. Padmanabhan, M. White, and J. D. Cohn, Reconstructing baryon oscillations: A Lagrangian theory perspective
Original
2009
Earlier work this paper cites.
Y. Noh, M. White, and N. Padmanabhan, Reconstructing baryon oscillations
Original
2009
Earlier work this paper cites.
C. Rampf and T. Buchert, Lagrangian perturbations and the matter bispectrum I: fourth-order model for non-linear clustering
Original
2012
Earlier work this paper cites.