https://doi.org/10.1140/epjc/s10052-023-11987-w
Regular Article - Theoretical Physics
Soft scattering evaporation of dark matter subhalos by inner galactic gases
1
Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, 100049, Beijing, China
2
School of Physical Sciences, University of Chinese Academy of Sciences, 100049, Beijing, China
3
Department of Physics, Beijing Normal University, 100875, Beijing, China
4
Center for High-Energy Physics, Peking University, 100871, Beijing, China
Received:
10
May
2023
Accepted:
29
August
2023
Published online:
11
September
2023
The large gap between a galactic dark matter subhalo’s velocity and its own gravitational binding velocity creates the situation that small subhalos can be evaporated before dark matter thermalize with baryons due to the low binding velocity. In case dark matter acquires an electromagnetic dipole moment, the survival of low-mass subhalos requires stringent limits on the photon-mediated soft scattering. The current stringent direct detection limits indicate for a small dipole moment, which lets DM decouple early and allows small subhalos to form. We calculate the DM kinetic decoupling temperature in the Early Universe and evaluate the smallest protohalo mass. In the late Universe, low-mass subhalos can be evaporated via soft collision by ionized gas and accelerated cosmic rays. We calculate the subhalos evaporation rate and show that subhalos lighter than 
in the gaseous inner galactic region are subject to evaporation via dark matter’s effective electric and magnetic dipole moments below current direct detection limits, which potentially affects the low-mass subhalos distribution in the galactic center.
© The Author(s) 2023
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