000208590 001__ 208590 000208590 005__ 20211110130753.0 000208590 0247_ $$2arXiv$$aarXiv:1504.00504 000208590 0247_ $$2altmetric$$aaltmetric:3866739 000208590 0247_ $$2inspire$$ainspire:1357597 000208590 037__ $$aPUBDB-2015-01796 000208590 0881_ $$aDESY-15-045; FTPI-MINN-15/15; IPMU15-0037; arXiv:1504.00504 000208590 088__ $$2DESY$$aDESY-15-045 000208590 088__ $$2Other$$aFTPI-MINN-15/15 000208590 088__ $$2Other$$aIPMU15-0037 000208590 088__ $$2arXiv$$aarXiv:1504.00504 000208590 1001_ $$aNagata, Natsumi$$b0 000208590 245__ $$aProbing Bino-Gluino Coannihilation at LHC 000208590 260__ $$c2015 000208590 3367_ $$2DRIVER$$apreprint 000208590 3367_ $$028$$2EndNote$$aElectronic Article 000208590 3367_ $$0PUB:(DE-HGF)25$$2PUB:(DE-HGF)$$aPreprint$$bpreprint$$mpreprint$$s1428399518_14846 000208590 3367_ $$2BibTeX$$aARTICLE 000208590 3367_ $$0PUB:(DE-HGF)15$$2PUB:(DE-HGF)$$aInternal Report$$mintrep 000208590 500__ $$aOA 000208590 520__ $$aIt has been widely known that bino-like dark matter in the supersymmetric (SUSY) theories in general suffers from over-production. The situation can be drastically improved if gluinos have a mass slightly heavier than the bino dark matter as they reduce the dark matter abundance through coannihilation. In this work, we consider such a bino-gluino coannihilation scenario in high-scale SUSY models, which can be actually realized when the squark-mass scale is less than 100-1000 TeV. We study the prospects for exploring this bino-gluino coannihilation scenario at the LHC. We show that the searches for long-lived colored particles with displaced vertices offer a strong tool to test this scenario in collider experiments. 000208590 536__ $$0G:(DE-HGF)POF3-611$$a611 - Fundamental Particles and Forces (POF3-611)$$cPOF3-611$$fPOF III$$x0 000208590 588__ $$aDataset connected to arXivarXiv 000208590 693__ $$0EXP:(DE-MLZ)NOSPEC-20140101$$5EXP:(DE-MLZ)NOSPEC-20140101$$eNo specific instrument$$x0 000208590 7001_ $$aOtono, Hidetoshi$$b1 000208590 7001_ $$0P:(DE-H253)PIP1023373$$aShirai, Satoshi$$b2$$eCorresponding Author$$udesy 000208590 8564_ $$yOpenAccess 000208590 8564_ $$uhttps://bib-pubdb1.desy.de/record/208590/files/1504.00504v1.pdf$$yOpenAccess 000208590 8564_ $$uhttps://bib-pubdb1.desy.de/record/208590/files/1504.00504v1.gif?subformat=icon$$xicon$$yOpenAccess 000208590 8564_ $$uhttps://bib-pubdb1.desy.de/record/208590/files/1504.00504v1.jpg?subformat=icon-1440$$xicon-1440$$yOpenAccess 000208590 8564_ $$uhttps://bib-pubdb1.desy.de/record/208590/files/1504.00504v1.jpg?subformat=icon-180$$xicon-180$$yOpenAccess 000208590 8564_ $$uhttps://bib-pubdb1.desy.de/record/208590/files/1504.00504v1.jpg?subformat=icon-640$$xicon-640$$yOpenAccess 000208590 8564_ $$uhttps://bib-pubdb1.desy.de/record/208590/files/1504.00504v1.jpg?subformat=icon-700$$xicon-700$$yOpenAccess 000208590 8564_ $$uhttps://bib-pubdb1.desy.de/record/208590/files/1504.00504v1.pdf?subformat=pdfa$$xpdfa$$yOpenAccess 000208590 909CO $$ooai:bib-pubdb1.desy.de:208590$$pdnbdelivery$$pdriver$$pVDB$$popen_access$$popenaire 000208590 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1023373$$aDeutsches Elektronen-Synchrotron$$b2$$kDESY 000208590 9130_ $$0G:(DE-HGF)POF2-514$$1G:(DE-HGF)POF2-510$$2G:(DE-HGF)POF2-500$$aDE-HGF$$bStruktur der Materie$$lElementarteilchenphysik$$vTheoretical Particle Physics$$x0 000208590 9131_ $$0G:(DE-HGF)POF3-611$$1G:(DE-HGF)POF3-610$$2G:(DE-HGF)POF3-600$$3G:(DE-HGF)POF3$$4G:(DE-HGF)POF$$aDE-HGF$$bForschungsbereich Materie$$lMaterie und Universum$$vFundamental Particles and Forces$$x0 000208590 9141_ $$y2015 000208590 915__ $$0StatID:(DE-HGF)0510$$2StatID$$aOpenAccess 000208590 915__ $$0StatID:(DE-HGF)0580$$2StatID$$aPublished 000208590 9201_ $$0I:(DE-H253)T-20120731$$kT$$lTheorie-Gruppe$$x0 000208590 980__ $$apreprint 000208590 980__ $$aVDB 000208590 980__ $$aUNRESTRICTED 000208590 980__ $$aFullTexts 000208590 980__ $$aintrep 000208590 980__ $$aI:(DE-H253)T-20120731 000208590 9801_ $$aFullTexts