The Lagrangian-space Effective Field Theory of large scale structures

By Rafael A. Porto, L. Senatore, M. Zaldarriaga. 2013

212 citations recorded by the source corpus.

We introduce a Lagrangian-space Effective Field Theory (LEFT) formalism for the study of cosmological large scale structures. Unlike the previous Eulerian-space construction, it is naturally formulated as an effective field theory of extended objects in Lagrangian space. In LEFT the resulting finite size effects are described using a multipole expansion parameterized by a set of time dependent coefficients and organized in powers of the ratio of the wavenumber of interest k over the non-linear scale kNL. The multipoles encode the effects of the short distance modes on the long-wavelength universe and absorb UV divergences when present. There are no IR divergences in LEFT. Some of the parameters that control the perturbative approach are not assumed to be small and can be automatically resummed. We present an illustrative one-loop calculation for a power law universe. We describe the dynamics both at the level of the equations of motion and through an action formalism.

Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/1e6188a3ad76043306a11a15b4060f3b088063ba

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In Astronomy and Astrophysics

  1. L. Senatore
  2. Mikhail Ivanov
  3. M. Zaldarriaga
  4. M. White
  5. Z. Vlah
  6. Guido D'Amico
  7. Pierre Zhang
  8. Shi-Fan Chen

In Atomic and Molecular Physics, and Optics

  1. L. Senatore
  2. Z. Vlah
  3. M. White
  4. Guido D'Amico
  5. Pierre Zhang
  6. Rafael A. Porto
  7. Shi-Fan Chen
  8. Alejandro Aviles

In Nuclear and High Energy Physics

  1. L. Senatore
  2. D. Baumann
  3. Guido D'Amico
  4. Pierre Zhang
  5. Rafael A. Porto
  6. M. Zaldarriaga
  7. D. Green
  8. M. White

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