SUMMARY
The discussion centers on the peculiar rotation of galaxies, particularly Barred Galaxies, and the implications of dark matter on their dynamics. Participants clarify that stars orbiting a black hole, such as the supermassive black hole (SMBH) at the center of the Milky Way, follow elliptical orbits rather than circular ones. The conversation highlights the unexpected behavior of the outer vortex rotation in these galaxies, which does not conform to the expected power decay equation, leading to the hypothesis of dark matter as a solution. Additionally, the concept of angular momentum conservation in forced vortex dynamics is introduced, suggesting that Barred Galaxies may not be in a steady-state mode.
PREREQUISITES
- Understanding of gravitational dynamics and orbital mechanics
- Familiarity with the concept of dark matter in astrophysics
- Knowledge of vortex dynamics, specifically Rankine Vortex theory
- Basic comprehension of galaxy classification, particularly Barred Galaxies
NEXT STEPS
- Research the properties and implications of dark matter in galactic rotation
- Study the dynamics of Rankine Vortex and its applications in astrophysics
- Examine the classification and characteristics of Barred Galaxies
- Explore the role of supermassive black holes (SMBH) in galaxy evolution
USEFUL FOR
Astronomers, astrophysics students, and anyone interested in the dynamics of galaxies and the role of dark matter in cosmic structures.