Abstract
We report the cosmological effects that a species of Ultra Light Bosonic Dark Matter imprints in the Acoustic Peaks of the CMB and some of its thermic features. We show that the effect of the Bose‐Einstein statistics is small albeit perceptible and is equivalent to an increase of non‐relativistic matter. It is noted the mass‐to‐temperature ratio necessary for being still a Dark Matter candidate. It is also needed a non‐zero optical depth of Reionization.
Full Text
Paper version not known (
Free)
Published Version
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call