| Issue |
A&A
Volume 701, September 2025
|
|
|---|---|---|
| Article Number | A220 | |
| Number of page(s) | 8 | |
| Section | Cosmology (including clusters of galaxies) | |
| DOI | https://doi.org/10.1051/0004-6361/202553824 | |
| Published online | 17 September 2025 | |
Determining H0 from a distance sum rule that combines gamma-ray bursts with observational Hubble data and strong gravitational lensing
1
Università di Camerino, Divisione di Fisica, Via Madonna delle Carceri 9, 62032 Camerino, Italy
2
SUNY Polytechnic Institute, 13502 Utica, New York, USA
3
INAF – Osservatorio Astronomico di Brera, Milano, Italy
4
INFN, Sezione di Perugia, Perugia, 06123
Italy
5
Al-Farabi Kazakh National University, Al-Farabi Av. 71, 050040 Almaty, Kazakhstan
6
ICRANet, Piazza della Repubblica 10, Pescara, 65122
Italy
⋆ Corresponding authors: orlando.luongo@unicam.it; marco.muccino@unicam.it
Received:
20
January
2025
Accepted:
5
May
2025
Context. Model-independent bounds on the Hubble constant H0 are important for gaining insight into cosmological tensions.
Aims. We work out a model-independent analysis based on the sum rule, which is applied to late- and early-time data catalogs to determine H0.
Methods. Through the model-independent Bézier interpolation of the observational Hubble data and assuming a flat universe, we reconstructed the dimensionless distances of the sum rule and applied them to strong lensing data to derive constraints on H0. We then extended this method to the high-redshift domain, and in two separate analyses, we included gamma-ray burst (GRB) data sets from the well-established Amati and Combo correlations.
Results. In all three analyses, our findings agree at the 1σ level with the H0 determined from type Ia supernovae (SNe Ia), and at the 2σ level, our findings agree with the measurement derived from the cosmic microwave background (CMB) radiation.
Conclusions. Our method evidences that the bounds on H0 are significantly affected by strong lensing data, which favor the local measurement from SNe Ia. Including GRBs causes only a negligible decrease in the value of H0. This may indicate that GRBs can be used to trace the expansion history, and in conjunction with CMB measurements, GRBs may reconcile the Hubble tension and accommodate the flat ΛCDM paradigm purported by CMB data.
Key words: cosmological parameters / cosmology: miscellaneous / cosmology: observations / cosmology: theory / dark energy / large-scale structure of Universe
© The Authors 2025
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
This article is published in open access under the Subscribe to Open model. Subscribe to A&A to support open access publication.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.