A spherically symmetric matter collapses under its own gravity. For the Milky Way, the time scale of collapse for a spherical halo with NFW density is ∼ 26 My which is very small compared to the age of the Milky Way. The effect of a pressure, obeying a polytrope equation of state is investigated. It is shown that for p ∝ ρ9/8, the time scale would be of the order of 1 Gy. It is also argued that such a polytrope, if considered to be in equilibrium, could explain the rotation curve of the milky way.
Farhadi, E. & Shariati, A. (2023). Gravitational collapse of the galactic dark matter. Iranian Journal of Physics Research, 23(3), 101-106. https://doi.org/10.47176/ijpr.23.3.11596
MLA
Farhadi, E., & Shariati, A. "Gravitational collapse of the galactic dark matter", Iranian Journal of Physics Research, 23, 3, 2023, 101-106. doi: 10.47176/ijpr.23.3.11596
HARVARD
Farhadi E., Shariati A. (2023). 'Gravitational collapse of the galactic dark matter', Iranian Journal of Physics Research, 23(3), pp. 101-106. doi: 10.47176/ijpr.23.3.11596
CHICAGO
E. Farhadi & A. Shariati, "Gravitational collapse of the galactic dark matter," Iranian Journal of Physics Research, 23 3 (2023): 101-106, doi: 10.47176/ijpr.23.3.11596
VANCOUVER
Farhadi E., Shariati A. Gravitational collapse of the galactic dark matter. Iranian Journal of Physics Research. 2023;23(3):101-106 (In Persian). doi: 10.47176/ijpr.23.3.11596