Limits on clustering and smooth quintessence from the EFTofLSS - INSPIRE

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Limits on clustering and smooth quintessence from the EFTofLSS

Guido D'Amico
(
- U. Parma (main) and
- INFN, Parma
)
,
Yaniv Donath
(
- ETH, Zurich (main) and
- Stanford U., ITP and
- KIPAC, Menlo Park and
- SLAC and
- Stanford U.
)
,
Leonardo Senatore
(
- Stanford U., ITP and
- KIPAC, Menlo Park and
- SLAC and
- Stanford U.
)
,
Pierre Zhang
(
- USTC, Hefei
)

Dec 14, 2020

41 pages

Published in:

JCAP 03 (2024) 032

Published: Mar 14, 2024

e-Print:

2012.07554 [astro-ph.CO]

DOI:

10.1088/1475-7516/2024/03/032

View in:

ADS Abstract Service

reference search44 citations

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Abstract: (IOP)

We apply the Effective Field Theory of Large-Scale Structure (EFTofLSS) to analyzecosmological models with clustering quintessence, which allows us to consistently describe theparameter region in which the quintessence equation of state w < -1. First, we extend thedescription of biased tracers in redshift space to the presence of clustering quintessence, andcompute the one-loop power spectrum. We solve the EFTofLSS equations using the exact timedependence, which is relevant to obtain unbiased constraints. Then, fitting the full shape of BOSSpre-reconstructed power spectrum measurements, the BOSS post-reconstruction BAO measurements, BAOmeasurements from 6DF/MGS and eBOSS, the Supernovae from Pantheon, and a prior from BBN, we boundthe clustering quintessence equation of state parameter w = -1.011

_{-0.048}

^{+0.053}

at 68%C.L. Further combining with Planck, we obtain w = -1.028

_{-0.030}

^{+0.037}

at 68% C.L. Wealso obtain constraints on smooth quintessence, in the physical regime w ≥ -1: combining alldatasets, we get -1 ≤ w < -0.979 at 68% C.L. These results strongly support a cosmological constant.

Note:

41 pages, 10 figures. v2: minor modifications, added references, matches JCAP published version

cosmological parameters from LSS
power spectrum
dark energy theory
galaxy clustering
nucleosynthesis: big bang
quintessence
equation of state
galaxy: power spectrum
effective field theory
cosmological constant

References(92)

Figures(12)

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John Joseph M. Carrasco
(
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Simon Foreman
(
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Leonardo Senatore
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Simon Foreman
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Matthew Lewandowski
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Leonardo Senatore
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- KIPAC, Menlo Park
)

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Thomas Konstandin
(
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Rafael A. Porto
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Henrique Rubira
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•
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•
DOI:
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