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Title: Efficient exploration of cosmology dependence in the EFT of LSS

Abstract

We develop a method to efficiently predict how the distribution of dark matter at long distances in our universe changes as we change the fundamental parameters of our universe

Authors:
 [1];  [2];  [2]
  1. Univ. of Copenhagen, Copenhagen (Denmark)
  2. Stanford Univ., Stanford, CA (United States); SLAC National Accelerator Lab., Menlo Park, CA (United States)
Publication Date:
Research Org.:
SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States); Stanford Univ., CA (United States)
Sponsoring Org.:
USDOE Office of Science (SC), High Energy Physics (HEP)
OSTI Identifier:
1368575
Alternate Identifier(s):
OSTI ID: 1491168
Grant/Contract Number:  
AC02-76SF00515; SC0008078
Resource Type:
Accepted Manuscript
Journal Name:
Journal of Cosmology and Astroparticle Physics
Additional Journal Information:
Journal Volume: 2017; Journal Issue: 04; Journal ID: ISSN 1475-7516
Publisher:
Institute of Physics (IOP)
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; cosmological parameters from LSS; cosmological perturbation theory; power spectrum; cosmological simulations

Citation Formats

Cataneo, Matteo, Foreman, Simon, and Senatore, Leonardo. Efficient exploration of cosmology dependence in the EFT of LSS. United States: N. p., 2017. Web. doi:10.1088/1475-7516/2017/04/026.
Cataneo, Matteo, Foreman, Simon, & Senatore, Leonardo. Efficient exploration of cosmology dependence in the EFT of LSS. United States. https://doi.org/10.1088/1475-7516/2017/04/026
Cataneo, Matteo, Foreman, Simon, and Senatore, Leonardo. Tue . "Efficient exploration of cosmology dependence in the EFT of LSS". United States. https://doi.org/10.1088/1475-7516/2017/04/026. https://www.osti.gov/servlets/purl/1368575.
@article{osti_1368575,
title = {Efficient exploration of cosmology dependence in the EFT of LSS},
author = {Cataneo, Matteo and Foreman, Simon and Senatore, Leonardo},
abstractNote = {We develop a method to efficiently predict how the distribution of dark matter at long distances in our universe changes as we change the fundamental parameters of our universe},
doi = {10.1088/1475-7516/2017/04/026},
journal = {Journal of Cosmology and Astroparticle Physics},
number = 04,
volume = 2017,
place = {United States},
year = {Tue Apr 18 00:00:00 EDT 2017},
month = {Tue Apr 18 00:00:00 EDT 2017}
}

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Cited by: 30 works
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