论文标题
对撞机的真实三胞胎标量暗物质的探针
Collider Probes of Real Triplet Scalar Dark Matter
论文作者
论文摘要
我们研究了大型强子对撞机(LHC)和未来100 TEV $ pp $ collider可能的标准模型标量扇区实际三胞胎扩展的发现前景。我们专注于中性三重态标量稳定并有助于暗物质遗物密度的情况。当以$ pp $碰撞为生时,带电的三重态标量会腐烂到中性组件,以及软亲旋或软的Lepton对,在检测器中产生了消失的充电轨道。我们重铸了当前的13TEV LHC搜索消失的轨道,并发现LHC目前不包括比248(275)GEV轻的三重态标量,以批量分配为172(160)MEV,$ \ MATHCAL {l} = \ rm36 \ rm36 \,$ fb $^,$ fb $^{-1} $。覆盖范围可以扩展到497(520)GEV,收集$ 3000 \,$ fb $^{ - 1} $。我们将13个TEV分析推送到了潜在的100 TEV $ PP $对撞机上,并发现可以使用$ \ Mathcal {l} = 30 $ ab $^{ - 1} $发现A $ \ sim3 $ TEV TEEV TRIPLET标量,这取决于控制效果的程度。我们还研究了模型中的暗物质候选者,以及来自暗物质直接检测的当前和前瞻性约束。我们发现,目前的Xenon1t可以将一个或SIM3 $ TEV的真正三重三重暗物质排除在一个或更大的订单的门户网站耦合中,而未来的Xenon20T几乎涵盖了整个深色物质可行的参数空间,除了消失了小的小门户耦合。
We study discovery prospects for a real triplet extension of the Standard Model scalar sector at the Large Hadron Collider (LHC) and a possible future 100 TeV $pp$ collider. We focus on the scenario in which the neutral triplet scalar is stable and contributes to the dark matter relic density. When produced in $pp$ collisions, the charged triplet scalar decays to the neutral component plus a soft pion or soft lepton pair, yielding a disappearing charged track in the detector. We recast current 13TeV LHC searches for disappearing tracks, and find that the LHC presently excludes a real triplet scalar lighter than 248 (275) GeV, for a mass splitting of 172 (160) MeV with $\mathcal{L}=\rm36\,$fb$^{-1}$. The reach can extend to 497 (520) GeV with the collection of $3000\,$fb$^{-1}$. We extrapolate the 13 TeV analysis to a prospective 100 TeV $pp$ collider, and find that a $\sim3$ TeV triplet scalar could be discoverable with $\mathcal{L}=30$ ab$^{-1}$, depending on the degree to which pile up effects are under control. We also investigate the dark matter candidate in our model and corresponding present and prospective constraints from dark matter direct detection. We find that currently XENON1T can exclude a real triplet dark matter lighter than $\sim3$ TeV for a Higgs portal coupling of order one or larger, and the future XENON20T will cover almost the entire dark matter viable parameter space except for vanishingly small portal coupling.