000276508 001__ 276508 000276508 005__ 20250717105437.0 000276508 0247_ $$2doi$$a10.1016/j.physletb.2015.06.044 000276508 0247_ $$2ISSN$$a0370-2693 000276508 0247_ $$2ISSN$$a1873-2445 000276508 0247_ $$2inspire$$ainspire:1357597 000276508 0247_ $$2altmetric$$aaltmetric:3866739 000276508 0247_ $$2arXiv$$aarXiv:1504.00504 000276508 0247_ $$2WOS$$aWOS:000359146200006 000276508 0247_ $$2openalex$$aopenalex:W2151850086 000276508 037__ $$aPUBDB-2015-04709 000276508 082__ $$a530 000276508 088__ $$2DESY$$aDESY-15-045 000276508 088__ $$2Other$$aFTPI-MINN-15/15 000276508 088__ $$2Other$$aIPMU15-0037 000276508 088__ $$2arXiv$$aarXiv:1504.00504 000276508 0881_ $$aDESY-15-045 000276508 1001_ $$0P:(DE-HGF)0$$aNagata, Natsumi$$b0$$eCorresponding author 000276508 245__ $$aProbing bino–gluino coannihilation at the LHC 000276508 260__ $$aAmsterdam$$bNorth-Holland Publ.$$c2015 000276508 3367_ $$2DRIVER$$aarticle 000276508 3367_ $$2DataCite$$aOutput Types/Journal article 000276508 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article$$bjournal$$mjournal$$s1600260977_32371 000276508 3367_ $$2BibTeX$$aARTICLE 000276508 3367_ $$2ORCID$$aJOURNAL_ARTICLE 000276508 3367_ $$00$$2EndNote$$aJournal Article 000276508 500__ $$aOA 000276508 520__ $$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 or large energy loss offer a strong tool to test this scenario in collider experiments. 000276508 536__ $$0G:(DE-HGF)POF3-611$$a611 - Fundamental Particles and Forces (POF3-611)$$cPOF3-611$$fPOF III$$x0 000276508 588__ $$aDataset connected to CrossRef 000276508 693__ $$0EXP:(DE-MLZ)NOSPEC-20140101$$5EXP:(DE-MLZ)NOSPEC-20140101$$eNo specific instrument$$x0 000276508 7001_ $$aOtono, Hidetoshi$$b1 000276508 7001_ $$0P:(DE-H253)PIP1023373$$aShirai, Satoshi$$b2$$eCorresponding author 000276508 773__ $$0PERI:(DE-600)1466612-1$$a10.1016/j.physletb.2015.06.044$$gVol. 748, p. 24 - 29$$p24 - 29$$tPhysics letters / B$$v748$$x0370-2693$$y2015 000276508 7870_ $$0PUBDB-2015-01796$$aNagata, Natsumi et.al.$$d2015$$iIsParent$$rDESY-15-045 ; FTPI-MINN-15/15 ; IPMU15-0037 ; arXiv:1504.00504$$tProbing Bino-Gluino Coannihilation at LHC 000276508 8564_ $$uhttps://bib-pubdb1.desy.de/record/276508/files/1-s2.0-S0370269315004669-main.pdf$$yOpenAccess 000276508 8564_ $$uhttps://bib-pubdb1.desy.de/record/276508/files/1-s2.0-S0370269315004669-main.gif?subformat=icon$$xicon$$yOpenAccess 000276508 8564_ $$uhttps://bib-pubdb1.desy.de/record/276508/files/1-s2.0-S0370269315004669-main.jpg?subformat=icon-1440$$xicon-1440$$yOpenAccess 000276508 8564_ $$uhttps://bib-pubdb1.desy.de/record/276508/files/1-s2.0-S0370269315004669-main.jpg?subformat=icon-180$$xicon-180$$yOpenAccess 000276508 8564_ $$uhttps://bib-pubdb1.desy.de/record/276508/files/1-s2.0-S0370269315004669-main.jpg?subformat=icon-640$$xicon-640$$yOpenAccess 000276508 8564_ $$uhttps://bib-pubdb1.desy.de/record/276508/files/1-s2.0-S0370269315004669-main.pdf?subformat=pdfa$$xpdfa$$yOpenAccess 000276508 909CO $$ooai:bib-pubdb1.desy.de:276508$$pdnbdelivery$$pdriver$$pVDB$$popen_access$$popenaire 000276508 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1023373$$aDeutsches Elektronen-Synchrotron$$b2$$kDESY 000276508 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 000276508 9141_ $$y2015 000276508 915__ $$0StatID:(DE-HGF)0200$$2StatID$$aDBCoverage$$bSCOPUS 000276508 915__ $$0LIC:(DE-HGF)CCBY4$$2HGFVOC$$aCreative Commons Attribution CC BY 4.0 000276508 915__ $$0StatID:(DE-HGF)0100$$2StatID$$aJCR$$bPHYS LETT B : 2014 000276508 915__ $$0StatID:(DE-HGF)1150$$2StatID$$aDBCoverage$$bCurrent Contents - Physical, Chemical and Earth Sciences 000276508 915__ $$0StatID:(DE-HGF)0500$$2StatID$$aDBCoverage$$bDOAJ 000276508 915__ $$0StatID:(DE-HGF)0110$$2StatID$$aWoS$$bScience Citation Index 000276508 915__ $$0StatID:(DE-HGF)0111$$2StatID$$aWoS$$bScience Citation Index Expanded 000276508 915__ $$0StatID:(DE-HGF)0150$$2StatID$$aDBCoverage$$bWeb of Science Core Collection 000276508 915__ $$0StatID:(DE-HGF)0510$$2StatID$$aOpenAccess 000276508 915__ $$0StatID:(DE-HGF)9905$$2StatID$$aIF >= 5$$bPHYS LETT B : 2014 000276508 915__ $$0StatID:(DE-HGF)0300$$2StatID$$aDBCoverage$$bMedline 000276508 915__ $$0StatID:(DE-HGF)0420$$2StatID$$aNationallizenz 000276508 915__ $$0StatID:(DE-HGF)0199$$2StatID$$aDBCoverage$$bThomson Reuters Master Journal List 000276508 915__ $$0StatID:(DE-HGF)0570$$2StatID$$aSCOAP3 000276508 9201_ $$0I:(DE-H253)T-20120731$$kT$$lTheorie-Gruppe$$x0 000276508 980__ $$ajournal 000276508 980__ $$aVDB 000276508 980__ $$aUNRESTRICTED 000276508 980__ $$aI:(DE-H253)T-20120731 000276508 9801_ $$aUNRESTRICTED 000276508 9801_ $$aFullTexts