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2007

On Einstein clusters as galactic dark matter halos

Boehmer, C. G., Harko, T.

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We consider global and gravitational lensing properties of the recently suggested Einstein clusters of WIMPs as galactic dark matter halos.

Being tangential pressure dominated, Einstein clusters are strongly anisotropic systems which can describe any galactic rotation curve by specifying the anisotropy.
Due to this property, Einstein clusters may be considered as dark matter candidates.
We analyse the stability of the Einstein clusters against both radial and non-radial pulsations, and we show that the Einstein clusters are dynamically stable.

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Böhmer C.G., Harko T., 2005b, PLB, 630, 73

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