Secular bar formation in galaxies with a significant amount of dark matter

@article{Valenzuela2003SecularBF,
  title={Secular bar formation in galaxies with a significant amount of dark matter},
  author={O. Valenzuela and Anatoly Klypin},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2003},
  volume={345},
  pages={406-422}
}
Using high resolution N-body simulations of stellar disks embedded in cosmologically motivated dark matter halos, we study the evolution of bars and the transfer of angular momentum between halos and bars. We find that dynamical friction results in some transfer of angular momentum to the halo, but the effect is much smaller than previously found in low resolution simulations and is incompatible with early analytical estimates. After 5 Gyrs of evolution the stellar component loses only 5% – 7… 
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