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Peculiar velocity cosmology with type Ia supernovae
R. Graziani
1
M. Rigault
1
N. Regnault
2
Ph Gris
1
A. Möller
1
P. Antilogus
2
P. Astier
2
M. Betoule
2
S. Bongard
2
M. Briday
3
J. Cohen-Tanugi
4
Y. Copin
3
H. M. Courtois
3
D. Fouchez
5
E. Gangler
1
D. Guinet
3
A. J. Hawken
5
Y. -L. Kim
3
P. -F. Léget
2
J. Neveu
6
P. Ntelis
3
Ph. Rosnet
1
E. Nuss
4
R. Graziani 1
Author
M. Rigault 1
Author IdHAL : mickael-rigault
N. Regnault 2
Author
Ph Gris 1
Author
A. Möller 1
Author
P. Antilogus 2
Author IdHAL : pierre-antilogus ORCID : https://orcid.org/0000-0002-0389-5706
P. Astier 2
Author
M. Betoule 2
Author IdHAL : marc-betoule ORCID : https://orcid.org/0000-0003-0804-836X
S. Bongard 2
Author IdHAL : sebastien-bongard
M. Briday 3
Author
J. Cohen-Tanugi 4
Author IdHAL : johann-cohen-tanugi ORCID : https://orcid.org/0000-0001-9022-4232
Y. Copin 3
Author IdHAL : yannick-copin ResearcherId : http://www.researcherid.com/rid/B-4928-2015 ORCID : https://orcid.org/0000-0002-5317-7518
H. M. M Courtois 3
Author
D. Fouchez 5
Author IdHAL : dominique-fouchez ORCID : https://orcid.org/0000-0002-7496-3796
E. Gangler 1
Author
D. Guinet 3
Author
1
LPC - Laboratoire de Physique de Clermont (Campus Universitaire des Cézeaux, 4 Avenue Blaise Pascal, TSA 60026, CS 6002, 63178 Aubière Cedex - France)
- CNRS - Centre National de la Recherche Scientifique : UMR6533 (France)
- UCA [2017-2020] - Université Clermont Auvergne [2017-2020] : UMR6533 (49, bd François-Mitterrand / CS 60032 / 63001 Clermont-Ferrand Cedex 1 - France)
- IN2P3 - Institut National de Physique Nucléaire et de Physique des Particules du CNRS (France)
2
LPNHE (UMR_7585) - Laboratoire de Physique Nucléaire et de Hautes Énergies (Barre 12-22, 1er étage 4 Place Jussieu 75252 Paris Cedex 05 - France)
- IN2P3 - Institut National de Physique Nucléaire et de Physique des Particules du CNRS : UMR_7585 (France)
- SU - Sorbonne Université : UMR_7585 (21 rue de l’École de médecine - 75006 Paris - France)
- CNRS - Centre National de la Recherche Scientifique : UMR_7585 (France)
3
IP2I Lyon - Institut de Physique des 2 Infinis de Lyon (Campus LyonTech-la Doua
Bâtiment Paul DIRAC
4 Rue Enrico Fermi
69622 Villeurbanne Cedex - France)
- IN2P3 - Institut National de Physique Nucléaire et de Physique des Particules du CNRS (France)
- UCBL - Université Claude Bernard Lyon 1 (43, boulevard du 11 novembre 1918, 69622 Villeurbanne cedex - France)
- Université de Lyon (92 rue Pasteur - CS 30122, 69361 Lyon Cedex 07 - France)
- CNRS - Centre National de la Recherche Scientifique : UMR5822 (France)
4
LUPM - Laboratoire Univers et Particules de Montpellier (Place Eugène Bataillon - CC 72 34095 Montpellier Cédex 05 - France)
- IN2P3 - Institut National de Physique Nucléaire et de Physique des Particules du CNRS (France)
- UM - Université de Montpellier (163 rue Auguste Broussonnet - 34090 Montpellier - France)
- CNRS - Centre National de la Recherche Scientifique : UMR5299 (France)
5
CPPM - Centre de Physique des Particules de Marseille (163, avenue de Luminy - Case 902 - 13288 Marseille cedex 09 - France)
- AMU - Aix Marseille Université : UMR7346 / UMR6550 / UMR6450 / URA6450 (Aix-Marseille Université Jardins du Pharo 58 Boulevard Charles Livon 13284 Marseille cedex 7 - France)
- IN2P3 - Institut National de Physique Nucléaire et de Physique des Particules du CNRS (France)
- CNRS - Centre National de la Recherche Scientifique : UMR7346 / UMR6550 / UMR6450 / URA6450 (France)
6
IJCLab - Laboratoire de Physique des 2 Infinis Irène Joliot-Curie (Bât. 100 et 200, 15 rue Georges Clémenceau 91405 Orsay
- France)
- IN2P3 - Institut National de Physique Nucléaire et de Physique des Particules du CNRS (France)
- Université Paris-Saclay (Bâtiment Bréguet, 3 Rue Joliot Curie 2e ét, 91190 Gif-sur-Yvette - France)
- CNRS - Centre National de la Recherche Scientifique : UMR9012 (France)
Abstract : Type Ia Supernovae have yet again the opportunity to revolutionize the field of cosmology as the new generation of surveys are acquiring thousands of nearby SNeIa opening a new era in cosmology: the direct measurement of the growth of structure parametrized by $fD$. This method is based on the SNeIa peculiar velocities derived from the residual to the Hubble law as direct tracers of the full gravitational potential caused by large scale structure. With this technique, we could probe not only the properties of dark energy, but also the laws of gravity. In this paper we present the analytical framework and forecasts. We show that ZTF and LSST will be able to reach 5\% precision on $fD$ by 2027. Our analysis is not significantly sensitive to photo-typing, but known selection functions and spectroscopic redshifts are mandatory. We finally introduce an idea of a dedicated spectrograph that would get all the required information in addition to boost the efficiency to each SNeIa so that we could reach the 5\% precision within the first two years of LSST operation and the few percent level by the end of the survey.
Document type :
Preprints, Working Papers, ...
Domain :
Complete list of metadata
https://hal-cnrs.archives-ouvertes.fr/hal-03045617
Contributor : Philippe Gris Connect in order to contact the contributor
Submitted on : Tuesday, December 8, 2020 - 9:56:45 AM
Last modification on : Friday, April 15, 2022 - 3:35:12 AM
Long-term archiving on: : Tuesday, March 9, 2021 - 6:36:07 PM
Contributor : Philippe Gris Connect in order to contact the contributor
Submitted on : Tuesday, December 8, 2020 - 9:56:45 AM
Last modification on : Friday, April 15, 2022 - 3:35:12 AM
Long-term archiving on: : Tuesday, March 9, 2021 - 6:36:07 PM
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2001.09095.pdf
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Identifiers
- HAL Id : hal-03045617, version 1
- ARXIV : 2001.09095
- INSPIRE : 1777187
Collections
CNRS | LPC-CLERMONT | IN2P3 | PRES_CLERMONT | LPNHE | UNIV-PARIS | UP-SCIENCES | COSMOLOGIE | UDL | SU-SCIENCES | SORBONNE-UNIVERSITE | UNIV-AMU | CPPM | UNIV-PARIS-SACLAY | SU-TI | IP2I | IJCLAB | UNIV-LYON1 | INSTITUT-SCIENCES-LUMIERE | LUPM | UNIV-MONTPELLIER | LUPM_EMA
Citation
R. Graziani, M. Rigault, N. Regnault, Ph Gris, A. Möller, et al.. Peculiar velocity cosmology with type Ia supernovae. 2020. ⟨hal-03045617⟩
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