It’s my last morning in Phoenix and since I was too busy at the weekend to post the usual update from the Open Journal of Astrophysics I will do so now, before I go to the Airport for my flight home.
Looking at the workflow I see that there is a considerable backlog of papers that have been accepted but are waiting for the authors to put the final version on arXiv. As a result there is only one paper to report for last week, being the 17th paper in Volume 7 (2024) and the 132nd altogether; it was published on March 6 2024. I expect more soon!
The title of the latest paper is “Bayesian analysis of a Unified Dark Matter model with transition: can it alleviate the H0tension?” and it is in the folder marked Cosmology and NonGalactic Astrophysics. The article presents an investigation using Bayesian techniques of a specific cosmological model, in which dark matter and dark energy are aspects of a single component, with particular emphasis on the Hubble tension.
The authors are seven in number: Emmanuel Frion (University of Helsinki, Finland, and Western University, Canada); David Camarena (University of New Mexico, USA); Leonardo Giani (University of Queensland, Australia); Tays Miranda (University of Helsinki and University of Jyväskylä, both in Finland); Daniele Bertacca (Università degli Studi di Padova, Italy); Valerio Marra (Universidade Federal do Espírito Santo, Brazil and Osservatorio Astronomico di Trieste, Italy);
and Oliver F. Piattella (Università degli Studi dell’Insubria, Como, Italy).
Here is the overlay of the paper containing the abstract:
You can click on the image of the overlay to make it larger should you wish to do so. You can also find the officially accepted version of the paper on the arXiv here.
In the Dark 