English

Non-particle dark matter from Hubble parameter

General Physics 2021-01-25 v2

Abstract

The measurements of the Hubble parameter using the cosmic microwave background radiation appear to be inconsistent with the measurements of this parameter using Cepheid variable stars. This inconsistency may be a result of using the Λ\LambdaCDM cosmology, which assumes pressureless dark matter, in extrapolating the data from the recombination time to the present time. We show that both measurements are consistent if dark matter satisfies an equation of state in which the pressure pp and the energy density ϵ\epsilon are related by p=wϵp=w\epsilon with a negative value of ww. The data give w0.01w\approx -0.01. The negative value of ww indicates that dark matter would not be formed by particles, which is consistent with the lack of experimental evidence for them.

Keywords

Cite

@article{arxiv.1906.03947,
  title  = {Non-particle dark matter from Hubble parameter},
  author = {Nikodem J. Popławski},
  journal= {arXiv preprint arXiv:1906.03947},
  year   = {2021}
}

Comments

3 pages; published version

R2 v1 2026-06-23T09:48:45.520Z