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Semantic Scholar Open Access 2024 5 sitasi

Euclid preparation. LXXI. Simulations and nonlinearities beyond LambdaCDM. 3. Constraints on f(R) models from the photometric primary probes

Euclid Collaboration K. Koyama S. Pamuk S. Casas B. Bose P. Carrilho +495 lainnya
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Abstrak

We study the constraint on f(R) gravity that can be obtained by photometric primary probes of the Euclid mission. Our focus is the dependence of the constraint on the theoretical modelling of the nonlinear matter power spectrum. In the Hu--Sawicki f(R) gravity model, we consider four different predictions for the ratio between the power spectrum in f(R) and that in Λ cold dark matter (ΛCDM): a fitting formula, the halo model reaction approach and two emulators based on dark matter only N -body simulations and . These predictions are added to the implementation to predict the angular power spectra for weak lensing (WL), photometric galaxy clustering, and their cross-correlation. By running Markov chain Monte Carlo, we compare constraints on parameters and investigate the bias of the recovered f(R) parameter if the data are created by a different model. For the pessimistic setting of WL, one-dimensional bias for the f(R) parameter, logfr, is found to be $0.5 σ$ when is used to create the synthetic data with logfr =-5.301 and fitted by . The impact of baryonic physics on WL is studied by using a baryonification emulator . For the optimistic setting, the f(R) parameter and two main baryonic parameters are well constrained despite the degeneracies among these parameters. However, the difference in the nonlinear dark matter prediction can be compensated for the adjustment of baryonic parameters, and the one-dimensional marginalised constraint on logfr is biased. This bias can be avoided in the pessimistic setting at the expense of weaker constraints. For the pessimistic setting, using the synthetic data for WL, we obtain the prior-independent upper limit of logfr < -5.6. Finally, we implement a method to include theoretical errors to avoid the bias due to inaccuracies in the nonlinear matter power spectrum prediction.

Topik & Kata Kunci

Physics

Penulis (500)

E

Euclid Collaboration K. Koyama

S

S. Pamuk

S

S. Casas

B

B. Bose

P

P. Carrilho

I

I. S'aez-Casares

L

L. Atayde

M

M. Cataneo

B

B. Fiorini

C

C. Giocoli

A

A. Brun

F

F. Pace

A

A. Pourtsidou

Y

Y. Rasera

Z

Z. Sakr

H

H. Winther

E

E. Altamura

J

J. Adamek

M

M. Baldi

M

M.-A. Breton

G

G. R'acz

F

F. Vernizzi

A

A. Amara

S

S. Andreon

N

N. Auricchio

C

C. Baccigalupi

S

S. Bardelli

F

F. Bernardeau

C

C. Bodendorf

D

D. Bonino

E

E. Branchini

M

M. Brescia

J

J. Brinchmann

A

A. Caillat

S

S. Camera

V

V. Capobianco

C

C. Carbone

J

J. Carretero

M

M. Castellano

G

G. Castignani

S

S. Cavuoti

A

A. Cimatti

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C. Colodro-Conde

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G. Congedo

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C. Conselice

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L. Conversi

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Y. Copin

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F. Courbin

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H. Courtois

A

A. Silva

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H. Degaudenzi

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G. Lucia

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M. Douspis

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F. Dubath

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X. Dupac

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S. Dusini

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S. Farrens

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S. Ferriol

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A

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G. Maggio

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M. Magliocchetti

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J. Mart'in-Fleitas

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C. Martins

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L. Maurin

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R. B. Metcalf

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M. Miluzio

P

P. Monaco

A

A. Montoro

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A. Mora

C

C. Moretti

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P. Reimberg

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I. Risso

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M. Sahl'en

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A

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M. Sereno

A

A. Silvestri

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J. Stadel

K

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C

C. Tao

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G. Testera

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R. Teyssier

S

S. Toft

S

S. Tosi

A

A. Troja

M

M. Tucci

J

J. Valiviita

D

D. Vergani

G

G. Verza

P

P. V. I. O. Cosmology

G

Gravitation

U

U. Portsmouth

P

PO1 3FX

U

Uk

I

I. F. Physics

C

Cosmology

R

Rwth Aachen University

5

52056 Aachen

G

Germany

I

Institute for Astronomy

U

U. Edinburgh

R

R. Observatory

B

B. Hill

E

Edinburgh EH9 3HJ

L

Laboratoire Univers et Th'eorie

O

Observatoire de Paris

U

Universit'e Psl

U

Universit'e de Paris Cit'e

C

Cnrs

9

92190 Meudon

F

France

I

I. D. A. E. C. D. Espacco

F

F. Ciencias

U

Universidade Tecnica de Lisboa

C

C. Grande

1

1049-001 Lisboa

P

Portugal

D

Departament de F'isica

C

C8 Edif'icio

P

P. Lisboa

R

R. Bochum

F

F. O. Physics

A

Astronomy

A

A. Institute

G

German Centre for Cosmological Lensing

4

44801 Bochum

U

U. Bonn

A

Argelander Institut fur Astronomie

7

71 AufdemHugel

5

53121 Bonn

I

I. Bologna

V

V. G. 933

4

40129 Bologna

I

Italy

I

Istituto Nazionale Fisica Nucleare

S

Sezione Infn di Bologna

4

46 ViaIrnerio

4

40129 Bologna

D

D. Fisica

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U. Torino

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1. ViaP.Giuria

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10125 Torino

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I. Torino

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I. Torino

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20 viaOsservatorio

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1. P. Torinese

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H. C. F. T. Physics

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S. O. Physics

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T. D. O. Edinburgh

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Edinburgh EH9 3FD

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Institut universitaire de France

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1. R. Descartes

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05 75231PARISCEDEX

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I. Physik

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U. Heidelberg

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16 Philosophenweg

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69117 Heidelberg

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Institut de Recherche en Astrophysique et Plan'etologie

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U. Toulouse

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Ups

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Cnes

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14 Avenue Edouard Belin

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31400 Toulouse

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Universit'e St Joseph

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F. O. Sciences

B

Beirut

L

Lebanon

I

I. Astrophysics

U

U. Oslo

P

P. O. B. 1. Blindern

0

0315 Oslo

N

Norway.

J

J. B. C. F. Astrophysics

D

D. Physics

U

U. Manchester

O

Oxford Road

M

M13 9PL

D

D. O. Astrophysics

U

U. Zurich

W

Winterthurerstrasse 190

8

8093 Zurich

S

Switzerland.

D

D. Astronomia

U

U. Bologna

V

V. G. 932

I

I. Bologna

6

62 vialeBertiPichat

4

40129 Bologna

I

Institute of Space Sciences

C

Campus Uab

C

Carrer de Can Magrans

S

Sn

0

08193 Barcelona

S

Spain.

I

Institut de Ci'encies de l'Espai

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sn Cerdanyola del Vall'es

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Jet propulsion Laboratory

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C. I. O. Technology.

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4800 Oak Grove Drive

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Pasadena

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Ca

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91109

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Usa

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Institut de Physique Th'eorique

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Cea

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Universit'e Paris-Saclay 91191 Gif-sur-Yvette Cedex

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S. O. Mathematics

P

Physics

U

U. Surrey

G

Guildford

S

Surrey

G

GU2 7XH

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Inaf Brera

2

28 ViaBrera

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20133 Milano

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Ifpu

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Institute for Fundamental Physics of the Universe

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2. viaBeirut

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34127 Trieste

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Inaf Trieste

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11 ViaG.B.Tiepolo

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34127 Trieste

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Infn

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Sezione di Trieste

2

2. ViaValerio

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TS 34127Trieste

S

Sissa

I

International School for Advanced Studies

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Via Bonomea 265

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TS 34136Trieste

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I. Paris

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Umr 7095

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Sorbonne Universit'e

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98 bis boulevard Arago

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7. Paris

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M. F. P. Physics

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1. Giessenbachstr.

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85748 Garching

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U. Genova

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16146

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Genova

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U. Federico

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80126

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Napoli

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80131 Napoli

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I. Naples

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U. Porto

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Caup

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Rua das Estrelas

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P. Porto

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F. Porto

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Rua do Campo Alegre

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4169-007 Porto

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A. Universit'e

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Lam

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Marseille

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20133 Milano

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Port d'Informaci'o Cient'ifica

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08193 Bellaterra

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00078 Monte Porzio Catone

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D. Bologna

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Instituto de Astrof'isica de Canarias

C

C. V. L. sn

3

38204

S

San Crist'obal de La Laguna

T

Tenerife

E

European Space AgencyESRIN

1

1. LargoGalileoGalilei

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00044 Frascati

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Roma

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Esacesa

C

Camino Bajo de Castillo

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Sn

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Urb. Villafranca del Castillo

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28692 Villanueva de la Canada

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Madrid

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CNRSIN2p3

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I. Lyon

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Umr 5822

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Villeurbanne

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F-69100

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I. O. Physics

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Laboratory of Astrophysics

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E. P. F. Lausanne

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Observatoire de Sauverny

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1290 Versoix

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Institut de Ci'encies del Cosmos

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U. Barcelona

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08193 Barcelona

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I. C. D. R. I. E. Avanccats

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08193 Barcelona

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1. UCBLyon

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Iuf

4

4. R. E. Fermi

6

69622 Villeurbanne

Format Sitasi

APA MLA BibTeX
Koyama, E.C.K., Pamuk, S., Casas, S., Bose, B., Carrilho, P., S'aez-Casares, I. et al. (2024). Euclid preparation. LXXI. Simulations and nonlinearities beyond LambdaCDM. 3. Constraints on f(R) models from the photometric primary probes. https://doi.org/10.1051/0004-6361/202452184

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Informasi Jurnal
Tahun Terbit
2024
Bahasa
en
Total Sitasi
5×
Sumber Database
Semantic Scholar
DOI
10.1051/0004-6361/202452184
Akses
Open Access ✓