001     470101
005     20240227162433.0
024 7 _ |a vanMarle:2022vvv
|2 INSPIRETeX
024 7 _ |a inspire:2040871
|2 inspire
024 7 _ |a arXiv:2203.00353
|2 arXiv
024 7 _ |a 10.3204/PUBDB-2021-04070
|2 datacite_doi
037 _ _ |a PUBDB-2021-04070
041 _ _ |a English
088 _ _ |a DESY-21-171
|2 DESY
088 _ _ |a arXiv:2203.00353
|2 arXiv
100 1 _ |a Marle, Allard Jan van
|0 P:(DE-HGF)0
|b 0
245 _ _ |a Diffusive shock acceleration at oblique high Mach number shocks
260 _ _ |c 2021
336 7 _ |a Preprint
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|m preprint
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|s 1647438291_28781
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336 7 _ |a WORKING_PAPER
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336 7 _ |a Electronic Article
|0 28
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336 7 _ |a preprint
|2 DRIVER
336 7 _ |a ARTICLE
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336 7 _ |a Output Types/Working Paper
|2 DataCite
500 _ _ |a Accepted for publication in ApJ
520 _ _ |a The current paradigm of cosmic ray (CR) origin states that the most part of galactic CRs is produced by supernova remnants. The interaction of supernova ejecta with the interstellar medium after supernova's explosions results in shocks responsible for CR acceleration via diffusive shock acceleration (DSA). We use particle-in-cell (PIC) simulations and a combined PIC-magnetohydrodynamic (PIC-MHD) technique to investigate whether DSA can occur in oblique high Mach number shocks. Using the PIC method, we follow the formation of the shock and determine the fraction of the particles that gets involved in DSA. Then, with this result, we use PIC-MHD simulations to model the large-scale structure of the plasma and the magnetic field surrounding the shock and find out whether or not the reflected particles can generate the upstream turbulence and trigger DSA. We find that the feasibility of this process in oblique shocks depends strongly on the Alfvenic Mach number, and the DSA process is more likely triggered at high Mach number shocks.
536 _ _ |a 611 - Fundamental Particles and Forces (POF4-611)
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588 _ _ |a Dataset connected to INSPIRE
693 _ _ |0 EXP:(DE-MLZ)NOSPEC-20140101
|5 EXP:(DE-MLZ)NOSPEC-20140101
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700 1 _ |a Bohdan, Artem
|0 P:(DE-H253)PIP1083006
|b 1
|e Corresponding author
700 1 _ |a Morris, Paul
|0 P:(DE-H253)PIP1091338
|b 2
700 1 _ |a Pohl, Martin
|0 P:(DE-H253)PIP1010085
|b 3
700 1 _ |a Marcowith, Alexandre
|0 P:(DE-HGF)0
|b 4
856 4 _ |u https://bib-pubdb1.desy.de/record/470101/files/HTML-Approval_of_scientific_publication.html
856 4 _ |u https://bib-pubdb1.desy.de/record/470101/files/High_Mach_shock_obliquity_studies_.pdf
856 4 _ |u https://bib-pubdb1.desy.de/record/470101/files/PDF-Approval_of_scientific_publication.pdf
856 4 _ |y OpenAccess
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910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 1
|6 P:(DE-H253)PIP1083006
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 2
|6 P:(DE-H253)PIP1091338
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 3
|6 P:(DE-H253)PIP1010085
913 1 _ |a DE-HGF
|b Forschungsbereich Materie
|l Matter and the Universe
|1 G:(DE-HGF)POF4-610
|0 G:(DE-HGF)POF4-611
|3 G:(DE-HGF)POF4
|2 G:(DE-HGF)POF4-600
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|v Fundamental Particles and Forces
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914 1 _ |y 2021
915 _ _ |a OpenAccess
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915 _ _ |a Published
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920 1 _ |0 I:(DE-H253)Z_THAT-20210408
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|l Theoretische Astroteilchenphysik
|x 0
980 _ _ |a preprint
980 _ _ |a VDB
980 _ _ |a UNRESTRICTED
980 _ _ |a I:(DE-H253)Z_THAT-20210408
980 1 _ |a FullTexts


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