English

Mixed Cold-Hot Dark Matter Model with several Massive Neutrino Types

Astrophysics 2009-09-25 v2 General Relativity and Quantum Cosmology High Energy Physics - Phenomenology

Abstract

Mixed cold-hot dark matter cosmological models (CHDM) with Ωtot=1\Omega_{tot}=1, approximately flat initial spectrum of adiabatic perturbations and 1, 2 or 3 types of massive neutrinos are compared and tested using recent observational data. The models with 2 or 3 neutrino types of equal mass permit as the best fit larger values of both the Hubble constant (H060H_0\le 60 for 2 types, H065H_0\le 65 for 3 types) and the total Ων\Omega_{\nu} (up to 0.3 for 3 types) than the model with 1 massive type. Also, they have less problems with abundances of early compact objects including LyαLy-\alpha clouds.

Keywords

Cite

@article{arxiv.astro-ph/9502019,
  title  = {Mixed Cold-Hot Dark Matter Model with several Massive Neutrino Types},
  author = {Dmitri Pogosyan and Alexei Starobinsky},
  journal= {arXiv preprint arXiv:astro-ph/9502019},
  year   = {2009}
}

Comments

5 pages, LaTeX file, 1 figure. Postscript version of paper is at ftp://ftp.cita.utoronto.ca/ftp/cita/dmitry/mdm_nv_text.ps, and figure is at ftp://ftp.cita.utoronto.ca/ftp/cita/dmitry/mdm_nv_fig.ps