Slowly rotating Bose Einstein condensate galactic dark matter halos, and their rotation curves
Abstract If dark matter is composed of massive bosons, a Bose–Einstein condensation process must have occurred during the cosmological evolution. Therefore galactic dark matter may be in a form of a condensate, characterized by a strong self-interaction. We consider the effects of rotation on the Bo...
Main Authors: | Xiaoyue Zhang, Man Ho Chan, Tiberiu Harko, Shi-Dong Liang, Chun Sing Leung |
---|---|
Format: | Article |
Language: | English |
Published: |
SpringerOpen
2018-04-01
|
Series: | European Physical Journal C: Particles and Fields |
Online Access: | http://link.springer.com/article/10.1140/epjc/s10052-018-5835-8 |
Similar Items
-
Testing Bose–Einstein condensate dark matter models with the SPARC galactic rotation curves data
by: Maria Crăciun, et al.
Published: (2020-08-01) -
Jeans instability and turbulent gravitational collapse of Bose–Einstein condensate dark matter halos
by: Tiberiu Harko
Published: (2019-09-01) -
Bose–Einstein Condensate dark matter models in the presence of baryonic matter and random confining potentials
by: Tiberiu Harko, et al.
Published: (2022-05-01) -
Vortex structures in rotating Bose-Einstein condensates
by: Matveenko, S, et al.
Published: (2009) -
Rapidly rotating Bose-Einstein condensates in anharmonic confinement
by: Lu Li-Hua, et al.
Published: (2006-09-01)