| Name: | Arpit Kottur |
| Affiliation: | Fergusson College (Autonomous), Pune |
| Conference ID: | ASI2025_408 |
| Title: | A Streamlined Model for Simulating Galactic Rotation Curves with Observational Validation |
| Authors: | Arpit Kottur A 1, Meet Mehta B 1, Raka Dabhade C 1 |
| Authors Affiliation: | 1. Arpit Kottur (Fergusson College (Autonomous), Pune-411004)
2. Meet Mehta (Fergusson College (Autonomous), Pune-411004)
3. Raka Dabhade (Fergusson College (Autonomous), Pune-411004) |
| Mode of Presentation: | Poster |
| Abstract Category: | Galaxies and Cosmology |
| Abstract: | In this work we present a streamlined yet robust simulation framework for generating galactic rotation curves, optimized for computational efficiency while retaining fidelity to observed data. The model integrates contributions from a galaxy’s bulge, disk, and dark matter halo, represented by Hernquist, exponential, and NFW profiles, respectively, to replicate realistic galactic rotation dynamics. Validated against observed rotation curves from galaxies such as the Milky Way and Andromeda, the simulation captures primary rotation curve characteristics and provides a close approximation of mass distribution within these galaxies. While minor discrepancies are present, primarily due to simplified profile assumptions, the model effectively balances accuracy with simplicity, offering a practical tool for galactic dynamics research. This accessible framework serves as a foundation for further studies in galaxy structure and evolution and is adaptable for educational applications. |
