Review paper compares baryonic mass and gravitational lensing methods in galaxy clusters, highlighting implications for cosmology.
This review paper presents a comparative analysis of baryonic mass estimation methods and gravitational lensing techniques in galaxy clusters, with emphasis on dark matter distribution, hydrostatic bias, weak lensing calibration, and cosmological implications. The paper discusses observational approaches, challenges in cluster mass determination, and the role of gravitational lensing in understanding large-scale structure formation and dark matter physics.
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Aaria Joshi (2026) studied this question.
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