Long-lived biνo at the LHC

被引:4
|
作者
Gehrlein, Julia [1 ]
Ipek, Seyda [2 ]
机构
[1] Brookhaven Natl Lab, Phys Dept, High Energy Theory Grp, Upton, NY 11973 USA
[2] Univ Calif Irvine, Dept Phys & Astron, 4129 Frederick Reines Hall, Irvine, CA 92617 USA
关键词
Beyond Standard Model; Neutrino Physics; Supersymmetric Standard Model; NEUTRINO MASS; PARTICLES; MECHANISM; MODEL;
D O I
10.1007/JHEP05(2021)020
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We examine the detection prospects for a long-lived bi nu o, a pseudo-Dirac bino which is responsible for neutrino masses, at the LHC and at dedicated long-lived particle detectors. The bi nu o arises in U(1)(R)-symmetric supersymmetric models where the neutrino masses are generated through higher dimensional operators in an inverse seesaw mechanism. At the LHC the bi nu o is produced through squark decays and it subsequently decays to quarks, charged leptons and missing energy via its mixing with the Standard Model neutrinos. We consider long-lived bi nu os which escape the ATLAS or CMS detectors as missing energy and decay to charged leptons inside the proposed long-lived particle detectors FASER, CODEX-b, and MATHUSLA. We find the currently allowed region in the squark-bi nu o mass parameter space by recasting most recent LHC searches for jets+ . We also determine the reach of MATHUSLA, CODEX-b and FASER. We find that a large region of parameter space involving squark masses, bi nu o mass and the messenger scale can be probed with MATHUSLA, ranging from bi nu o masses of 10 GeV-2 TeV and messenger scales 10(2-11) TeV for a range of squark masses.
引用
收藏
页数:16
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