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001 | 296474 | ||
005 | 20211110133752.0 | ||
024 | 7 | _ | |a arXiv:1009.1942 |2 arXiv |
024 | 7 | _ | |a 10.3204/DESY-PROC-2010-01/10 |2 datacite_doi |
024 | 7 | _ | |a inspire:867660 |2 inspire |
037 | _ | _ | |a PUBDB-2016-01476 |
041 | _ | _ | |a English |
088 | 1 | _ | |a arXiv:1009.1942 |
088 | _ | _ | |a arXiv:1009.1942 |2 arXiv |
100 | 1 | _ | |a Gelmini, Graciela B. |0 P:(DE-HGF)0 |b 0 |e Corresponding author |
111 | 2 | _ | |a Physics at the LHC 2010 |g PLHC2010 |c Hamburg |d 2010-06-07 - 2010-06-12 |w Germany |
245 | _ | _ | |a Theory of Dark Matter |
260 | _ | _ | |a Hamburg |c 2010 |b Verlag Deutsches Elektronen-Synchrotron |
300 | _ | _ | |a 261-266 |
336 | 7 | _ | |a Conference Paper |0 33 |2 EndNote |
336 | 7 | _ | |a conferenceObject |2 DRIVER |
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336 | 7 | _ | |a INPROCEEDINGS |2 BibTeX |
520 | _ | _ | |a The search for dark matter is a very wide and active field of research. Many potential hints of dark matter have appeared recently which led to a burst of theoretical activity and model building. I necessarily concentrate here only in some aspects of it. I review here some recent hints and some of the ways in which they could be explained. |
536 | _ | _ | |a 899 - ohne Topic (POF3-899) |0 G:(DE-HGF)POF3-899 |c POF3-899 |f POF III |x 0 |
588 | _ | _ | |a Dataset connected to INSPIRE |
650 | _ | 7 | |a dark matter |2 INSPIRE |
650 | _ | 7 | |a CERN LHC Coll |2 INSPIRE |
650 | _ | 7 | |a burst |2 INSPIRE |
693 | _ | _ | |a HERA |e Facility (machine) HERA |1 EXP:(DE-588)4159571-3 |0 EXP:(DE-H253)HERA(machine)-20150101 |5 EXP:(DE-H253)HERA(machine)-20150101 |x 0 |
773 | _ | _ | |a 10.3204/DESY-PROC-2010-01/10 |
787 | 0 | _ | |a Diehl, Markus et.al. |d Hamburg : Verlag Deutsches Elektronen-Synchrotron, 2010 |i IsPartOf |0 PUBDB-2016-01404 |r DESY-PROC-2010-01 |t Physics at the LHC2010. Proceedings, 5th Conference, PLHC2010, Hamburg, Germany, June 7-12, 2010 |
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