Are observations of the galaxy cluster Abell 1689 consistent with a neutrino dark matter scenario?

Abstract

Recent weak and strong lensing data of the galaxy cluster A1689 are modelled by dark fermions that are quantum degenerate within some core. The gas density, deduced from X-ray observations up to 1 Mpc and obeying a cored power law, is taken as input, while the galaxy mass density is modelled. An additional dark matter tail may arise from cold or warm dark matter, axions or non-degenerate neutrinos. The fit yields that the fermions are degenerate within a 430 kpc radius. The fermion mass is a few eV and the best case involves 3 active plus 3 sterile neutrinos of equal mass, for which we deduce $1.51\pm 0.04$ eV. The eV mass range will be tested in the KATRIN experiment.

5 pages latex, 5 figures. Accepted for MNRAS Letters

References in corpus (5)

• Dark Matter Results from 225 Live Days of XENON100 Data
• Combining Strong and Weak Gravitational Lensing in Abell 1689
• Combining Lens Distortion and Depletion to Map the Mass Distribution of A1689
• X-ray and Sunyaev-Zel'dovich scaling relations in galaxy clusters
• On Dark Peaks and Missing Mass: A Weak Lensing Mass Reconstruction of the Merging Cluster System Abell 520

Cited by in corpus (4)

• Three-dimensional Multi-probe Analysis of the Galaxy Cluster A1689
• Free Form Lensing Implications for the Collision of Dark Matter and Gas in the Frontier Fields Cluster MACSJ0416.1-2403
• The gravitational field of X-COP galaxy clusters
• Solution of the dark matter riddle within standard model physics: From black holes, galaxies and clusters to cosmology