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@ARTICLE{Kummer:419492,
author = {Kummer, Janis and Brüggen, Marcus and Dolag, Klaus and
Kahlhoefer, Felix and Schmidt-Hoberg, Kai},
title = {{S}imulations of core formation for frequent dark matter
self-interactions},
reportid = {PUBDB-2019-01142, arXiv:1902.02330. DESY-19-020. TTK-19-06},
year = {2019},
abstract = {We present the first $N$-body simulations that use smoothed
particle hydrodynamics to capture the effect of dark matter
self-interactions which are too frequent to be resolved
explicitly. The relevant energy transfer equations are
derived, the appropriate thermal conductivity is determined
and the effects of different smoothing kernels are studied.
We apply our framework to simulate the formation of
isothermal cores in isolated dark matter haloes and
determine the core growth rate as a function of the
self-scattering cross section. Our approach may be combined
with explicit simulations of rare scatterings in order to
simulate accurately the effects of arbitrary dark matter
self-interactions in future cosmological simulations.},
keywords = {dark matter: halo (autogen) / conductivity: thermal
(autogen) / formation (autogen) / hydrodynamics (autogen) /
scattering (autogen) / capture (autogen)},
cin = {T},
cid = {I:(DE-H253)T-20120731},
pnm = {611 - Fundamental Particles and Forces (POF3-611) / NewAve
- New avenues towards solving the dark matter puzzle
(638528) / DFG project 13245592 - SFB 676: Teilchen, Strings
und frühes Universum: Struktur von Materie und Raum-Zeit
(13245592) / EXC 2121 - Das Quantisierte Universum
(390833306)},
pid = {G:(DE-HGF)POF3-611 / G:(EU-Grant)638528 /
G:(GEPRIS)13245592 / G:(GEPRIS)390833306},
experiment = {EXP:(DE-MLZ)NOSPEC-20140101},
typ = {PUB:(DE-HGF)25 / PUB:(DE-HGF)29},
eprint = {1902.02330},
howpublished = {arXiv:1902.02330},
archivePrefix = {arXiv},
SLACcitation = {$\%\%CITATION$ = $arXiv:1902.02330;\%\%$},
doi = {10.3204/PUBDB-2019-01142},
url = {https://bib-pubdb1.desy.de/record/419492},
}