Neutralino dark matter and other LHC predictions from quasi Yukawa unification
文摘
We explore the dark matter and LHC implications of class="mathmlsrc">class="formulatext stixSupport mathImg" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0550321315003387&_mathId=si1.gif&_user=111111111&_pii=S0550321315003387&_rdoc=1&_issn=05503213&md5=4a571a60ef47e5597de08c14986ff0be" title="Click to view the MathML source">t−b−蟿class="mathContainer hidden">class="mathCode">tb quasi Yukawa unification in the framework of supersymmetric models based on the gauge symmetry class="mathmlsrc">class="formulatext stixSupport mathImg" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0550321315003387&_mathId=si129.gif&_user=111111111&_pii=S0550321315003387&_rdoc=1&_issn=05503213&md5=e5b305c1d9acbb28ca78c9f9c43b4a01" title="Click to view the MathML source">G=SU(4)c×SU(2)L×SU(2)Rclass="mathContainer hidden">class="mathCode">G=SU(4)c×SU(2)L×SU(2)R. The deviation from exact Yukawa unification is quantified by a dimensionless parameter C   (class="mathmlsrc">class="formulatext stixSupport mathImg" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0550321315003387&_mathId=si3.gif&_user=111111111&_pii=S0550321315003387&_rdoc=1&_issn=05503213&md5=26c3bae57ff91407d3c9831de0c5012a" title="Click to view the MathML source">|C|鈮?.2class="mathContainer hidden">class="mathCode">|C|鈮?/mo>0.2), such that the Yukawa couplings at class="mathmlsrc">class="formulatext stixSupport mathImg" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0550321315003387&_mathId=si22.gif&_user=111111111&_pii=S0550321315003387&_rdoc=1&_issn=05503213&md5=6e0240bd386a571d8dc9dabda3ef455b" title="Click to view the MathML source">MGUTclass="mathContainer hidden">class="mathCode">MGUT are related by class="mathmlsrc">class="formulatext stixSupport mathImg" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0550321315003387&_mathId=si5.gif&_user=111111111&_pii=S0550321315003387&_rdoc=1&_issn=05503213&md5=f83ef7de758b0fb2427b275402a5cd20" title="Click to view the MathML source">yt:yb:y=|1+C|:|1−C|:|1+3C|class="mathContainer hidden">class="mathCode">yt:yb:y=|1+C|:|1C|:|1+3C|. In contrast to earlier studies which focused on universal gaugino masses, we consider non-universal gaugino masses at class="mathmlsrc">class="formulatext stixSupport mathImg" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0550321315003387&_mathId=si22.gif&_user=111111111&_pii=S0550321315003387&_rdoc=1&_issn=05503213&md5=6e0240bd386a571d8dc9dabda3ef455b" title="Click to view the MathML source">MGUTclass="mathContainer hidden">class="mathCode">MGUT that are compatible with the gauge symmetry G. Our results reveal a variety of neutralino dark matter scenarios consistent with the observations. These include stau and chargino coannihilation scenarios, the A  -resonance scenario, as well as Higgsino dark matter solutions which are more readily probed by direct detection searches. The gluino mass is found to be class="mathmlsrc">class="formulatext stixSupport mathImg" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0550321315003387&_mathId=si6.gif&_user=111111111&_pii=S0550321315003387&_rdoc=1&_issn=05503213&md5=2ce4f2d717a7f505ec2c73403c26ceac" title="Click to view the MathML source">鈮? TeVclass="mathContainer hidden">class="mathCode">鈮?/mo>4 TeV, the stop mass is class="mathmlsrc">class="formulatext stixSupport mathImg" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0550321315003387&_mathId=si7.gif&_user=111111111&_pii=S0550321315003387&_rdoc=1&_issn=05503213&md5=599cb8931bf860a2b462a8361a93ea51" title="Click to view the MathML source">鈮? TeVclass="mathContainer hidden">class="mathCode">鈮?/mo>2 TeV, while the first two family squarks and sleptons are of order 4–5 TeV and 3 TeV respectively.
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