Abstract
The gravitational interplay between a supermassive black hole and dark matter has set up an exotic environment at the center of a galaxy. In this paper, I present an analytic framework modeling the gravitational influence on the stars orbiting a galactic supermassive black hole. In particular, we discuss two intriguing features, stellar orbital precession and orbital shrinking, which demonstrate an extraordinary gravitational environment near a galactic supermassive black hole. Moreover, I show that these features can be analytically determined by the supermassive black hole mass. Copyright © 2024 World Scientific Publishing Company.
| Original language | English |
|---|---|
| Article number | 2441010 |
| Journal | International Journal of Modern Physics D |
| Volume | 33 |
| Issue number | 15 |
| Early online date | Sept 2024 |
| DOIs | |
| Publication status | Published - 2024 |
Keywords
- Supermassive black holes
- Dark matter
- Galactic center
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