Hoeneisen, B. (2020) Cold or Warm Dark Matter? A Study of Galaxy Stellar Mass Distributions. International Journal of Astronomy and Astrophysics, 10, 57-70.
https://doi.org/10.4236/ijaa.2020.102005

has been cited by the following article:

• TITLE: Comments on Warm Dark Matter Measurements and Limits

  AUTHORS: Bruce Hoeneisen

  KEYWORDS: Warm Dark Matter, Spiral Galaxy Rotation Curves, Stellar Mass Distributions, Lyman-α Forest

  JOURNAL NAME: International Journal of Astronomy and Astrophysics, Vol.12 No.1, March 18, 2022

  ABSTRACT: Observed spiral galaxy rotation curves allow a measurement of the warm dark matter particle velocity dispersion and mass. The measured thermal relic mass mh ≈ 100 eV is in disagreement with limits, typically in the range 1 to 4 keV. We review the measurements, update the no freeze-in and no freeze-out scenario of warm dark matter, and try to identify the cause of the discrepancies between measurements and limits.