在大型强子对撞机上寻找含有暗物质的希格斯玻色子

M. Gallinaro
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引用次数: 0

摘要

在星系尺度上存在暗物质(DM)的令人信服的直接证据来自对星系旋转曲线的观察。在粒子对撞机中,对DM的搜索涉及产生一对稳定的电中性和弱相互作用的粒子,其特征是缺少横向能量($E^{\rm T}_{\rm miss}$)反冲到SM粒子上。由此产生的签名产生一个最终状态,表示为X+$E^{\rm T}_{\rm miss}$,其中SM粒子X作为初始状态辐射发射。希格斯玻色子在大型强子对撞机上的发现为通过h+$E^{\rm T}_{\rm miss}$特征寻找超越SM的新物理过程打开了一扇新窗口,作为涉及DM粒子相互作用的直接探测。由于与夸克和胶子的小汤川耦合,希格斯玻色子的初始态辐射被抑制,但它可以在与DM粒子的新相互作用的情况下产生。讨论了与希格斯玻色子相关的DM粒子的搜索。它们基于LHC在不同最终状态下的质子-质子碰撞数据。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Searches for Higgs bosons with dark matter at the Large Hadron Collider
Convincing and direct evidence for dark matter (DM) on galactic scales comes from the observation of the rotation curves of galaxies. At particle colliders, searches for DM involve the production of a pair of stable electrically neutral and weakly interacting particles with a signature of missing transverse energy ($E^{\rm T}_{\rm miss}$) recoiling against a SM particle. The resulting signature yields a final state denoted as X+$E^{\rm T}_{\rm miss}$, where the SM particle X is emitted as initial state radiation. The Higgs boson discovery at the LHC opens a new window into the searches for new physics processes beyond the SM through the h+$E^{\rm T}_{\rm miss}$ signature, as a direct probe of the interaction involving DM particles. Due to the small Yukawa couplings to quarks and gluons, the initial state radiation of the Higgs boson is suppressed, but it can be produced in the case of a new interaction with DM particles. Searches for DM particles produced in association with the Higgs boson are discussed. They are based on proton-proton collision data at the LHC in different final states.
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