Hints of dark matter-neutrino interactions in Lyman- data
arXiv:2110.04024 · doi:10.1103/PhysRevD.105.103504
Abstract
In this work we investigate the possibility that dark matter and (massive) neutrinos can interact via a simple, constant cross section. Building on previous numerical efforts, we constrain this model with CMB, BAO and, in particular, Lyman- data. We find that the latter hint to a significant departure from CDM, with a preference for an interaction strength about 3 away from zero. We trace the origin of this preference back to the additional tilt that the interacting scenario can imprint on the Lyman- flux power spectrum, solving a well-known tension in the determination of this quantity between early-time and Lyman- probes. Future work including complementary Lyman- data as well as dedicated numerical simulations will be crucial in order to test these results.
arXiv comment7+4 pages with 5 figures and 2 tables. Published version
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