Revisiting perfect fluid dark matter: Observational constraints from our galaxy
Alexander A. Potapov, Guzel M. Garipova, Kamal K. Nandi
TL;DR
This paper reevaluates the properties of a perfect fluid dark matter halo model for our galaxy using observational data to test its validity and constraints.
Contribution
It provides new observational constraints on the perfect fluid dark matter model based on galactic data.
Findings
Constraints on dark matter density profiles
Compatibility with galactic rotation curves
Limits on model parameters
Abstract
We revisit certain features of an assumed spherically symmetric perfect fluid dark matter halo in the light of the observed data of our galaxy
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