dark matter gravitational lensing spiral galaxies Newtonian dynamics quantum gravity galactic rotation curves

The study of dark matter has been a pivotal aspect of astrophysics to understand the mass distribution in galaxies. Our objective is to investigate the distribution of dark matter in spiral galaxies by analyzing the gravitational lensing effects observed at the galactic scale. Utilizing data from the Hubble Space Telescope and advanced computational models, we employed a combination of Newtonian dynamics and quantum gravitational frameworks to simulate galactic environments. Our findings suggest that dark matter halos exhibit a more complex structure than previously anticipated, with variations correlating to galactic rotation curves. The study revealed that these halos significantly influence the gravitational potential experienced by luminous matter. In conclusion, this research enhances our understanding of galactic dynamics and the pivotal role of dark matter, offering new insights into the mysterious components of the universe. Future work will involve extending this methodology to different galaxy morphologies to further refine our comprehension of dark matter influences.

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