001     419492
005     20230310120349.0
024 7 _ |a Kummer:2019yrb
|2 INSPIRETeX
024 7 _ |a inspire:1718815
|2 inspire
024 7 _ |a arXiv:1902.02330
|2 arXiv
024 7 _ |a 10.3204/PUBDB-2019-01142
|2 datacite_doi
037 _ _ |a PUBDB-2019-01142
041 _ _ |a English
088 1 _ |a arXiv:1902.02330; DESY-19-020; TTK-19-06
088 _ _ |a arXiv:1902.02330
|2 arXiv
088 _ _ |a DESY-19-020
|2 DESY
088 _ _ |a TTK-19-06
|2 Other
100 1 _ |a Kummer, Janis
|0 P:(DE-H253)PIP1019753
|b 0
|e Corresponding author
245 _ _ |a Simulations of core formation for frequent dark matter self-interactions
260 _ _ |c 2019
336 7 _ |a Preprint
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336 7 _ |a WORKING_PAPER
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336 7 _ |a Electronic Article
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336 7 _ |a Report
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336 7 _ |a ARTICLE
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336 7 _ |a Output Types/Working Paper
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520 _ _ |a 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.
536 _ _ |a 611 - Fundamental Particles and Forces (POF3-611)
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|x 0
|f POF III
536 _ _ |a NewAve - New avenues towards solving the dark matter puzzle (638528)
|0 G:(EU-Grant)638528
|c 638528
|x 1
|f ERC-2014-STG
536 _ _ |a DFG project 13245592 - SFB 676: Teilchen, Strings und frühes Universum: Struktur von Materie und Raum-Zeit (13245592)
|0 G:(GEPRIS)13245592
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536 _ _ |a EXC 2121 - Das Quantisierte Universum (390833306)
|0 G:(GEPRIS)390833306
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|f DFG EXC 2121
588 _ _ |a Dataset connected to INSPIRE
650 _ 7 |a dark matter: halo
|2 autogen
650 _ 7 |a conductivity: thermal
|2 autogen
650 _ 7 |a formation
|2 autogen
650 _ 7 |a hydrodynamics
|2 autogen
650 _ 7 |a scattering
|2 autogen
650 _ 7 |a capture
|2 autogen
693 _ _ |0 EXP:(DE-MLZ)NOSPEC-20140101
|5 EXP:(DE-MLZ)NOSPEC-20140101
|e No specific instrument
|x 0
700 1 _ |a Brüggen, Marcus
|b 1
700 1 _ |a Dolag, Klaus
|b 2
700 1 _ |a Kahlhoefer, Felix
|b 3
700 1 _ |a Schmidt-Hoberg, Kai
|0 P:(DE-H253)PIP1022003
|b 4
856 4 _ |u https://bib-pubdb1.desy.de/record/419492/files/1902.02330.pdf
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910 1 _ |a Externes Institut
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910 1 _ |a Deutsches Elektronen-Synchrotron
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913 1 _ |a DE-HGF
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|0 G:(DE-HGF)POF3-611
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914 1 _ |y 2019
915 _ _ |a OpenAccess
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915 _ _ |a Published
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980 _ _ |a preprint
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980 _ _ |a report
980 _ _ |a I:(DE-H253)T-20120731
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980 1 _ |a FullTexts


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