A new paper analyzing New Early Dark Energy (NEDE) using profile likelihood methods in collaboration with Aarhus U. group: Emil Brinch Holm, Thomas Tram, and Steen Hannestad and with Florian Niedermann at Nordita and Juan Cruz at SDU: https://arxiv.org/abs/2302.07934
In science, you have to be able to reach the same result by using different methods, and with the Hubble tension, physicists have a problem … here is a popular article about our method to solve this problem:
https://www.sdu.dk/en/nyheder/forskningsnyheder/boblende-univers
