Numerical challenges for energy conservation in N -body simulations of collapsing self-interacting dark matter halos
Context. Dark matter (DM) halos can be subject to gravothermal collapse if the DM is not collisionless, but engaged in strong self-interactions instead. When the scattering is able to efficiently transfer heat from the centre to the outskirts, the central region of the halo collapses and reaches den...
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| Published in | Astronomy and astrophysics (Berlin) Vol. 689; p. A300 |
|---|---|
| Main Authors | , , |
| Format | Journal Article |
| Language | English |
| Published |
Germany
EDP Sciences
20.09.2024
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| Online Access | Get full text |
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