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том 537 издание 4 страницы 3814-3825

It’s not σ8 : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample

Paul Shah 1, 2
T.D Davis 3
M Vincenzi 4
Patrick Armstrong 5
Dillon Brout 4, 6, 7
R Camilleri 3
L. Galbany 8, 9, 10, 11
M. S. S. Gill 12
D. Huterer 13
N. Jeffrey 1, 2
O. Lahav 1, 2
J. Lee 14
C. Lidman 5, 15
A Möller 16, 17
M. Sullivan 18
L. Whiteway 1, 2
P. Wiseman 18
S. Allam 19
M. Aguena 20, 21
J. Annis 19
J. Blazek 22
D. Brooks 1, 2
A. Carnero Rosell 20, 21, 23, 24, 25
J. Carretero 26, 27
C. Conselice 28, 29
L. N. da Costa 20, 21
M. E. S. Pereira 30, 31
S. Desai 32
H. T. Diehl 19
P. Doel 1, 2
S. Everett 33, 34
I. Ferrero 35, 36
B. Flaugher 19
J. Frieman 19, 37
J. García-Bellido 38, 39
E. Gaztanaga 8, 9, 10, 11, 40
G. Giannini 27, 37, 41
D. Gruen 42, 43
R. A. Gruendl 44, 45, 46
G. Gutierrez 19
S. R. Hinton 3
D. L. Hollowood 47
K. Honscheid 48, 49
D. J. James 6, 7
S ( Lee 50
J. L. Marshall 51, 52
J. Mena-Fernández 53, 54
R. Miquel 26, 27, 55
A. Palmese 56
A. Pieres 20, 21, 57, 58
A. A. Plazas Malagón 12, 59, 60
A. Porredon 61, 62, 63
S. Samuroff 22, 26, 27
E. Sanchez 61
I. Sevilla-Noarbe 61
M. Smith 64
E. Suchyta 65
M. E. C. Swanson 44, 46
G. Tarle 13
D. L. Tucker 19
N. Weaverdyck 66, 67
11
 
Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans , s/n, E-08193 Barcelona ,
20
 
Laboratório Interinstitucional de e-Astronomia—LIneA , Rua Gal. José Cristino 77, Rio de Janeiro, RJ—20921–400 ,
21
 
Laboratório Interinstitucional de e-Astronomia – LIneA , Rua Gal. José Cristino 77, Rio de Janeiro, RJ-20921-400 ,
44
 
Center for Astrophysical Surveys, National Center for Supercomputing Applications , 1205 West Clark St., Urbana, IL 61801 ,
46
 
Center for Astrophysical Surveys, National Center for Supercomputing Applications , 1205 West Clark St, Urbana, IL 61801 ,
47
 
Santa Cruz Institute for Particle Physics , Santa Cruz, CA 95064 ,
53
 
LPSC Grenoble—53, Avenue des Martyrs 38026 Grenoble ,
54
 
Laboratoire de Physique Subatomique et de Cosmologie, Avenue des Martyrs F-38026, Grenoble ,
57
 
Observatório Nacional , Rua Gal. José Cristino 77, Rio de Janeiro, RJ—20921–400 ,
58
 
Observatório Nacional , Rua Gal. José Cristino 77, Rio de Janeiro, RJ-20921-400 ,
Тип публикацииJournal Article
Дата публикации2025-02-17
scimago Q1
wos Q1
БС1
SJR1.702
CiteScore9.7
Impact factor4.8
ISSN00358711, 13652966, 13658711
Краткое описание
ABSTRACT

The weak gravitational lensing magnification of Type Ia supernovae (SNe Ia) is sensitive to the matter power spectrum on scales $k\gt 1 h$ Mpc$^{-1}$, making it unwise to interpret SNe Ia lensing in terms of power on linear scales. We compute the probability density function of SNe Ia magnification as a function of standard cosmological parameters, plus an empirical parameter $A_{\rm mod}$ which describes the suppression or enhancement of matter power on non-linear scales compared to a cold dark matter only model. While baryons are expected to enhance power on the scales relevant to SN Ia lensing, other physics such as neutrino masses or non-standard dark matter may suppress power. Using the Dark Energy Survey Year-5 sample, we find $A_{\rm mod} = 0.77^{+0.69}_{-0.40}$ (68 per cent credible interval around the median). Although the median is consistent with unity there are hints of power suppression, with $A_{\rm mod} \lt 1.09$ at 68 per cent credibility.

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Physical Review Letters
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Physical Review D
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Shah P. et al. It’s not σ8 : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample // Monthly Notices of the Royal Astronomical Society. 2025. Vol. 537. No. 4. pp. 3814-3825.
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Shah P. et al. It’s not σ8 : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample // Monthly Notices of the Royal Astronomical Society. 2025. Vol. 537. No. 4. pp. 3814-3825.
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@article{2025_Shah,
author = {Paul Shah and T.D Davis and M Vincenzi and Patrick Armstrong and Dillon Brout and R Camilleri and L. Galbany and M. S. S. Gill and D. Huterer and N. Jeffrey and O. Lahav and J. Lee and C. Lidman and A Möller and M. Sullivan and L. Whiteway and P. Wiseman and S. Allam and M. Aguena and J. Annis and J. Blazek and D. Brooks and A. Carnero Rosell and J. Carretero and C. Conselice and L. N. da Costa and M. E. S. Pereira and S. Desai and H. T. Diehl and P. Doel and S. Everett and I. Ferrero and B. Flaugher and J. Frieman and J. García-Bellido and E. Gaztanaga and G. Giannini and D. Gruen and R. A. Gruendl and G. Gutierrez and S. R. Hinton and D. L. Hollowood and K. Honscheid and D. J. James and S ( Lee and J. L. Marshall and J. Mena-Fernández and R. Miquel and A. Palmese and A. Pieres and others},
title = {It’s not σ8 : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample},
journal = {Monthly Notices of the Royal Astronomical Society},
year = {2025},
volume = {537},
publisher = {Oxford University Press},
month = {feb},
url = {https://academic.oup.com/mnras/advance-article/doi/10.1093/mnras/staf286/8019799},
number = {4},
pages = {3814--3825},
doi = {10.1093/mnras/staf286}
}
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Shah, Paul, et al. “It’s not σ8 : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample.” Monthly Notices of the Royal Astronomical Society, vol. 537, no. 4, Feb. 2025, pp. 3814-3825. https://academic.oup.com/mnras/advance-article/doi/10.1093/mnras/staf286/8019799.