Comments on "Modeling Galaxy Halos Using Dark Matter with Pressure"

Details Comments on "Modeling Galaxy Halos Using Dark Matter with Pressure" Comments on "Modeling Galaxy Halos Using Dark Matter with Pressure"

2009-05-13

arxiv.org/abs/0905.2084v1

Phys.Rev.D79:128301,2009

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

3 pages, 2 figures

Scientific paper

10.1103/PhysRevD.79.128301

We comment on the calculational mistake in the paper "Modeling galaxy halos using dark matter with pressure" by Somnath Bharadwaj and Sayan Kar. The authors made a mistake while calculating the metric, which led to an overestimate of the deflection angle of light passing through the halos for -10 should not exist. Although the Bharadwaj-Kar solution should be corrected, it appears that the characteristics of the deflection angle under the supposed non-conventional non-ideal fluid equation of state for the dark matter halo remain sensitive to the impact parameter and may be verifiable through observations.

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