SIDM physics should include contribution from host^N, not just host halo #175
Labels
dark matter
good first issue
Good for newcomers
SIDM
Issues relating to self-interacting dark matter modeling
subhalos
Currently SIDM physics (e.g. ram pressure effects) are applied only from the direct host of the satellite halo. We should include the contribution from the host-host, and host-host-host etc. also. According to simulations run by Ethan Nadler these effects can be significant.
The text was updated successfully, but these errors were encountered: