A Predicted Relation between the Temperature and Density Profile of Cluster Hot Gas

Details A Predicted Relation between the Temperature and Density Profile of Cluster Hot Gas A Predicted Relation between the Temperature and Density Profile of Cluster Hot Gas

2008-07-08

arxiv.org/abs/0807.1218v1

Astrophys.Space Sci.317:149-152,2008

Astronomy and Astrophysics

Astrophysics

Accepted for publication in Astrophysics & Space Science

Scientific paper

10.1007/s10509-008-9868-6

Based on the assumptions that a fraction of cluster dark matter is composed
of degenerate neutrinos and they are in hydrostatic equilibrium with other
matter, we predict a relation between the density profile and temperature of
the cluster hot gas. The predicted relation agrees with observational data of
103 clusters.

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