_version_ 1866917841943396352
author Shah, Paul
Davis, Tamara M.
Vincenzi, Maria
Armstrong, Patrick
Brout, Dillon
Camilleri, Ryan
Galbany, Lluis
Garcia-Bellido, Juan
Gill, Mandeep S. S.
Lahav, Ofer
Lee, Jason
Lidman, Chris
Moeller, Anais
Sako, Masao
Sanchez, Bruno O.
Sullivan, Mark
Whiteway, Lorne
Wiseman, Phillip
Allam, S.
Aguena, M.
Bocquet, S.
Brooks, D.
Burke, D. L.
Rosell, A. Carnero
da Costa, L. N.
Pereira, M. E. S.
Desai, S.
Dodelson, S.
Doel, P.
Ferrero, I.
Flaugher, B.
Frieman, J.
Gaztanaga, E.
Gruen, D.
Gruendl, R. A.
Gutierrez, G.
Herner, K.
Hinton, S. R.
Hollowood, D. L.
Honscheid, K.
James, D. J.
Kuehn, K.
Lee, S.
Marshall, J. L.
Mena-Fernandez, J.
Miquel, R.
Myles, J.
Palmese, A.
Pieres, A.
Malagon, A. A. Plazas
Roodman, A.
Samuroff, S.
Sanchez, E.
Sevilla-Noarbe, I.
Smith, M.
Suchyta, E.
Swanson, M. E. C.
Tarle, G.
To, C.
Vikram, V.
author_facet Shah, Paul
Davis, Tamara M.
Vincenzi, Maria
Armstrong, Patrick
Brout, Dillon
Camilleri, Ryan
Galbany, Lluis
Garcia-Bellido, Juan
Gill, Mandeep S. S.
Lahav, Ofer
Lee, Jason
Lidman, Chris
Moeller, Anais
Sako, Masao
Sanchez, Bruno O.
Sullivan, Mark
Whiteway, Lorne
Wiseman, Phillip
Allam, S.
Aguena, M.
Bocquet, S.
Brooks, D.
Burke, D. L.
Rosell, A. Carnero
da Costa, L. N.
Pereira, M. E. S.
Desai, S.
Dodelson, S.
Doel, P.
Ferrero, I.
Flaugher, B.
Frieman, J.
Gaztanaga, E.
Gruen, D.
Gruendl, R. A.
Gutierrez, G.
Herner, K.
Hinton, S. R.
Hollowood, D. L.
Honscheid, K.
James, D. J.
Kuehn, K.
Lee, S.
Marshall, J. L.
Mena-Fernandez, J.
Miquel, R.
Myles, J.
Palmese, A.
Pieres, A.
Malagon, A. A. Plazas
Roodman, A.
Samuroff, S.
Sanchez, E.
Sevilla-Noarbe, I.
Smith, M.
Suchyta, E.
Swanson, M. E. C.
Tarle, G.
To, C.
Vikram, V.
contents Gravitational lensing magnification of Type Ia supernovae (SNe Ia) allows information to be obtained about the distribution of matter on small scales. In this paper, we derive limits on the fraction $α$ of the total matter density in compact objects (which comprise stars, stellar remnants, small stellar groupings and primordial black holes) of mass $M > 0.03 M_{\odot}$ over cosmological distances. Using 1,532 SNe Ia from the Dark Energy Survey Year 5 sample (DES-SN5YR) combined with a Bayesian prior for the absolute magnitude $M$, we obtain $α< 0.12$ at the 95\% confidence level after marginalisation over cosmological parameters, lensing due to large-scale structure, and intrinsic non-Gaussianity. Similar results are obtained using priors from the cosmic microwave background, baryon acoustic oscillations and galaxy weak lensing, indicating our results do not depend on the background cosmology. We argue our constraints are likely to be conservative (in the sense of the values we quote being higher than the truth), but discuss scenarios in which they could be weakened by systematics of the order of $Δα\sim 0.04$
format Preprint
id arxiv_https___arxiv_org_abs_2410_07956
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Constraints on compact objects from the Dark Energy Survey five-year supernova sample
Shah, Paul
Davis, Tamara M.
Vincenzi, Maria
Armstrong, Patrick
Brout, Dillon
Camilleri, Ryan
Galbany, Lluis
Garcia-Bellido, Juan
Gill, Mandeep S. S.
Lahav, Ofer
Lee, Jason
Lidman, Chris
Moeller, Anais
Sako, Masao
Sanchez, Bruno O.
Sullivan, Mark
Whiteway, Lorne
Wiseman, Phillip
Allam, S.
Aguena, M.
Bocquet, S.
Brooks, D.
Burke, D. L.
Rosell, A. Carnero
da Costa, L. N.
Pereira, M. E. S.
Desai, S.
Dodelson, S.
Doel, P.
Ferrero, I.
Flaugher, B.
Frieman, J.
Gaztanaga, E.
Gruen, D.
Gruendl, R. A.
Gutierrez, G.
Herner, K.
Hinton, S. R.
Hollowood, D. L.
Honscheid, K.
James, D. J.
Kuehn, K.
Lee, S.
Marshall, J. L.
Mena-Fernandez, J.
Miquel, R.
Myles, J.
Palmese, A.
Pieres, A.
Malagon, A. A. Plazas
Roodman, A.
Samuroff, S.
Sanchez, E.
Sevilla-Noarbe, I.
Smith, M.
Suchyta, E.
Swanson, M. E. C.
Tarle, G.
To, C.
Vikram, V.
Cosmology and Nongalactic Astrophysics
Gravitational lensing magnification of Type Ia supernovae (SNe Ia) allows information to be obtained about the distribution of matter on small scales. In this paper, we derive limits on the fraction $α$ of the total matter density in compact objects (which comprise stars, stellar remnants, small stellar groupings and primordial black holes) of mass $M > 0.03 M_{\odot}$ over cosmological distances. Using 1,532 SNe Ia from the Dark Energy Survey Year 5 sample (DES-SN5YR) combined with a Bayesian prior for the absolute magnitude $M$, we obtain $α< 0.12$ at the 95\% confidence level after marginalisation over cosmological parameters, lensing due to large-scale structure, and intrinsic non-Gaussianity. Similar results are obtained using priors from the cosmic microwave background, baryon acoustic oscillations and galaxy weak lensing, indicating our results do not depend on the background cosmology. We argue our constraints are likely to be conservative (in the sense of the values we quote being higher than the truth), but discuss scenarios in which they could be weakened by systematics of the order of $Δα\sim 0.04$
title Constraints on compact objects from the Dark Energy Survey five-year supernova sample
topic Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2410.07956