In-depth analysis of bar formation mechanisms of disk galaxies in halos of different concentrations
Using N-body simulations, this study reveals that bar formation mechanisms in disk galaxies vary significantly with halo concentration: highly concentrated halos favor swing-amplified multi-arm modes followed by particle trapping with minimal angular momentum transfer, lowly concentrated halos are dominated by linearly unstable modes triggering strong corotation resonance and rapid slowdown, while intermediate concentrations exhibit a combination of all these processes.