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Pantheon + supernovae corrected for progenitor age indicate the universe is decelerating

Abstract:
We examine the impact of progenitor age-dependent luminosity evolution of Type Ia supernovae on a cosmographic measurement of the deceleration parameter . Our recent redshift tomographic analysis showed that locally has a strong dipole anisotropy aligned approximately with the bulk flow, and only a small monopole component remains at distances exceeding a few hundred Mpc. Applying redshift-dependent corrections for progenitor age to the Pantheon + catalogue, we find that this shifts the monopole component of to positive values (i.e. deceleration) while leaving the local dipole component essentially unchanged.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1093/mnras/stag844

Authors

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Role:
Author
ORCID:
0000-0001-9541-916X
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Role:
Author
ORCID:
0000-0001-5023-5631
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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Theoretical Physics
Role:
Author
ORCID:
0000-0002-3542-858X


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Funder identifier:
https://ror.org/03ht1xw27


Publisher:
Oxford University Press
Journal:
Monthly Notices of the Royal Astronomical Society More from this journal
Volume:
549
Issue:
3
Article number:
stag844
Publication date:
2026-06-11
Acceptance date:
2026-04-30
DOI:
EISSN:
1365-2966
ISSN:
0035-8711


Language:
English
Keywords:
Source identifiers:
4223701
Deposit date:
2026-06-11
ARK identifier:
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