The IR-resummed Effective Field Theory of Large Scale Structures
Abstract
We develop a way to describe analytically the effect of large displacements of galaxies that occur in our universe, and that were affecting our capability to predict the distribution of galaxies in our universe.
- Authors:
-
- Stanford Univ., Stanford, CA (United States); SLAC National Accelerator Lab., Menlo Park, CA (United States)
- Institute for Advanced Study, Princeton, NJ (United States)
- Publication Date:
- Research Org.:
- Stanford Univ., CA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP)
- OSTI Identifier:
- 1491164
- Grant/Contract Number:
- SC0008078
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Journal of Cosmology and Astroparticle Physics
- Additional Journal Information:
- Journal Volume: 2015; Journal Issue: 02; Journal ID: ISSN 1475-7516
- Publisher:
- Institute of Physics (IOP)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; power spectrum; cosmological perturbation theory; baryon acoustic oscillations
Citation Formats
Senatore, Leonardo, and Zaldarriaga, Matias. The IR-resummed Effective Field Theory of Large Scale Structures. United States: N. p., 2015.
Web. doi:10.1088/1475-7516/2015/02/013.
Senatore, Leonardo, & Zaldarriaga, Matias. The IR-resummed Effective Field Theory of Large Scale Structures. United States. https://doi.org/10.1088/1475-7516/2015/02/013
Senatore, Leonardo, and Zaldarriaga, Matias. Tue .
"The IR-resummed Effective Field Theory of Large Scale Structures". United States. https://doi.org/10.1088/1475-7516/2015/02/013. https://www.osti.gov/servlets/purl/1491164.
@article{osti_1491164,
title = {The IR-resummed Effective Field Theory of Large Scale Structures},
author = {Senatore, Leonardo and Zaldarriaga, Matias},
abstractNote = {We develop a way to describe analytically the effect of large displacements of galaxies that occur in our universe, and that were affecting our capability to predict the distribution of galaxies in our universe.},
doi = {10.1088/1475-7516/2015/02/013},
journal = {Journal of Cosmology and Astroparticle Physics},
number = 02,
volume = 2015,
place = {United States},
year = {Tue Feb 10 00:00:00 EST 2015},
month = {Tue Feb 10 00:00:00 EST 2015}
}
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Cited by: 139 works
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Figures / Tables:
Figure 1: Parameters measuring the amplitude of non-linear correction on a mode of wavenumber k. They quantify the motions created by modes longer (ϵ$_{\delta<}$) and shorter (ϵ$_{\delta>}$) than k and the tides from larger scales (ϵ$_{\delta<}$).
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The One-Loop Matter Bispectrum in the Effective Field Theory of Large Scale Structures
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The matter power spectrum in redshift space using effective field theory
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Dark Energy and Modified Gravity in the Effective Field Theory of Large-Scale Structure
text, January 2017
- Cusin, Giulia; Lewandowski, Matthew; Vernizzi, Filippo
- arXiv
Infrared Resummation for Biased Tracers in Redshift Space
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- Ivanov, Mikhail M.; Sibiryakov, Sergey
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Figures/Tables have been extracted from DOE-funded journal article accepted manuscripts.