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001     208590
005     20211110130753.0
024 7 _ |a arXiv:1504.00504
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024 7 _ |a inspire:1357597
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037 _ _ |a PUBDB-2015-01796
088 1 _ |a DESY-15-045; FTPI-MINN-15/15; IPMU15-0037; arXiv:1504.00504
088 _ _ |a DESY-15-045
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088 _ _ |a IPMU15-0037
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088 _ _ |a arXiv:1504.00504
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100 1 _ |a Nagata, Natsumi
|b 0
245 _ _ |a Probing Bino-Gluino Coannihilation at LHC
260 _ _ |c 2015
336 7 _ |a preprint
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336 7 _ |a Electronic Article
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336 7 _ |a Preprint
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336 7 _ |a ARTICLE
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336 7 _ |a Internal Report
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500 _ _ |a OA
520 _ _ |a It has been widely known that bino-like dark matter in the supersymmetric (SUSY) theories in general suffers from over-production. The situation can be drastically improved if gluinos have a mass slightly heavier than the bino dark matter as they reduce the dark matter abundance through coannihilation. In this work, we consider such a bino-gluino coannihilation scenario in high-scale SUSY models, which can be actually realized when the squark-mass scale is less than 100-1000 TeV. We study the prospects for exploring this bino-gluino coannihilation scenario at the LHC. We show that the searches for long-lived colored particles with displaced vertices offer a strong tool to test this scenario in collider experiments.
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700 1 _ |a Otono, Hidetoshi
|b 1
700 1 _ |a Shirai, Satoshi
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910 1 _ |a Deutsches Elektronen-Synchrotron
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914 1 _ |y 2015
915 _ _ |a OpenAccess
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915 _ _ |a Published
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