Atomic dark matter, interacting dark radiation, and the Hubble tension

Abstract We present a new class of interacting dark sector models that can address the Hubble tension. Interacting dark radiation (DR) has previously been put forward as a solution to the problem, but this proposal is disfavored by the high-ℓ cosmic microwave background (CMB) data. We modify this ba...

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Bibliographic Details
Main Authors: Manuel A. Buen-Abad, Zackaria Chacko, Ina Flood, Can Kilic, Gustavo Marques-Tavares, Taewook Youn
Format: Article
Language:English
Published: SpringerOpen 2025-07-01
Series:Journal of High Energy Physics
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Online Access:https://doi.org/10.1007/JHEP07(2025)084
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