001     434875
005     20211110155935.0
024 7 _ |a Habermehl:2020njb
|2 INSPIRETeX
024 7 _ |a inspire:1774758
|2 inspire
024 7 _ |a arXiv:2001.03011
|2 arXiv
024 7 _ |a 10.3204/PUBDB-2020-00400
|2 datacite_doi
037 _ _ |a PUBDB-2020-00400
041 _ _ |a English
088 _ _ |a arXiv:2001.03011
|2 arXiv
088 _ _ |a DESY-19-237
|2 DESY
100 1 _ |a Habermehl, Moritz
|0 P:(DE-H253)PIP1013042
|b 0
245 _ _ |a WIMP Dark Matter at the International Linear Collider
260 _ _ |c 2019
300 _ _ |a 30
336 7 _ |a report
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336 7 _ |a REPORT
|2 ORCID
336 7 _ |a Report
|0 10
|2 EndNote
336 7 _ |a Output Types/Report
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336 7 _ |a Report
|b report
|m report
|0 PUB:(DE-HGF)29
|s 1591952005_13154
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336 7 _ |a TECHREPORT
|2 BibTeX
500 _ _ |a * Temporary entry *30 pages, 21 figures
520 _ _ |a In this study, the sensitivity of future lepton colliders to WIMP dark matter is evaluated assuming WIMP pair production accompanied by a photon from initial state radiation, through which the process can be identified. A full detector simulation for the International Large Detector (ILD) concept at the International Linear Collider (ILC) is performed for a \com energy of 500\,GeV. Energy scales of up to $3$\,TeV can be tested for different effective operators for WIMP masses almost up to half the \com energy. The sensitivity benefits from the polarised beams, which can reduce the main SM background from neutrino pair production substantially. In addition, systematic uncertainties are shown to be significantly reduced by combining data with several different polarisation configurations. In comparison to a previous study, the reconstruction of the forward detectors has been improved and the systematic uncertainties are fully treated. The results are also extrapolated to other \com energies, luminosities and beam polarisations. This allows to provide results for the full ILC programme, i.e.\ from 250\,GeV to 1\,TeV, as well as to give approximate results for other planned lepton colliders.
536 _ _ |a 611 - Fundamental Particles and Forces (POF3-611)
|0 G:(DE-HGF)POF3-611
|c POF3-611
|f POF III
|x 0
588 _ _ |a Dataset connected to INSPIRE
650 _ 7 |a WIMP: dark matter
|2 autogen
650 _ 7 |a WIMP: pair production
|2 autogen
650 _ 7 |a WIMP: mass
|2 autogen
650 _ 7 |a neutrino: pair production
|2 autogen
650 _ 7 |a beam: polarization
|2 autogen
650 _ 7 |a radiation: initial-state interaction
|2 autogen
650 _ 7 |a ILC Coll
|2 autogen
650 _ 7 |a sensitivity
|2 autogen
650 _ 7 |a lepton
|2 autogen
650 _ 7 |a forward spectrometer
|2 autogen
650 _ 7 |a polarized beam
|2 autogen
650 _ 7 |a initial state
|2 autogen
650 _ 7 |a ILD detector
|2 autogen
650 _ 7 |a background
|2 autogen
650 _ 7 |a photon
|2 autogen
693 _ _ |a ILC
|e Facility (machine) ILC
|1 EXP:(DE-H253)ILC-20150101
|0 EXP:(DE-H253)ILC(machine)-20150101
|5 EXP:(DE-H253)ILC(machine)-20150101
|x 0
700 1 _ |a Berggren, Mikael
|0 P:(DE-H253)PIP1006429
|b 1
|u desy
700 1 _ |a List, Jenny
|0 P:(DE-H253)PIP1005630
|b 2
|e Corresponding author
|u desy
856 4 _ |y OpenAccess
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856 4 _ |y OpenAccess
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856 4 _ |y OpenAccess
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856 4 _ |y OpenAccess
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909 C O |o oai:bib-pubdb1.desy.de:434875
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910 1 _ |a External Institute
|0 I:(DE-HGF)0
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|6 P:(DE-H253)PIP1013042
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
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910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
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913 1 _ |a DE-HGF
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|l Materie und Universum
|1 G:(DE-HGF)POF3-610
|0 G:(DE-HGF)POF3-611
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|v Fundamental Particles and Forces
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915 _ _ |a OpenAccess
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920 1 _ |0 I:(DE-H253)FLC-20120731
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980 _ _ |a report
980 _ _ |a VDB
980 _ _ |a UNRESTRICTED
980 _ _ |a I:(DE-H253)FLC-20120731
980 1 _ |a FullTexts


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