Abstract

We examine the supersymmetry (SUSY) reach of the CERN LHC operating at s=10\sqrt{s}=10 and 14 TeV within the framework of the minimal supergravity model. We improve upon previous reach projections by incorporating updated background calculations including a variety of 2n2\to n Standard Model (SM) processes. We show that SUSY discovery is possible even before the detectors are understood well enough to utilize either ETmissE_T^{\rm miss} or electrons in the signal. We evaluate the early SUSY reach of the LHC at s=10\sqrt{s}=10 TeV by examining multi-muon plus 4\ge4 jets and also dijet events with {\it no} missing ETE_T cuts and show that the greatest reach in terms of m1/2m_{1/2} occurs in the dijet channel. The reach in multi-muons is slightly smaller in m1/2m_{1/2}, but extends to higher values of m0m_0. We find that an observable multi-muon signal will first appear in the opposite-sign dimuon channel, but as the integrated luminosity increases the relatively background-free but rate-limited same-sign dimuon, and ultimately the trimuon channel yield the highest reach. We show characteristic distributions in these channels that serve to distinguish the signal from the SM background, and also help to corroborate its SUSY origin. We then evaluate the LHC reach in various no-lepton and multi-lepton plus jets channels {\it including} missing ETE_T cuts for s=10\sqrt{s}=10 and 14 TeV, and plot the reach for integrated luminosities ranging up to 3000 fb1^{-1} at the SLHC. For s=10\sqrt{s}=10 TeV, the LHC reach extends to mgluino=1.9,2.3,2.8m_{gluino}=1.9, 2.3, 2.8 and 2.9 TeV for msquarkmgluinom_{squark}\sim m_{gluino} and integrated luminosities of 10, 100, 1000 and 3000 fb1^{-1}, respectively. For s=14\sqrt{s}=14 TeV, the LHC reach for the same integrated luminosities is to m_{gluino}=2.4,\3.1, 3.7 and 4.0 TeV.Comment: 34 pages, 25 figures. Revised projections for the SUSY reach for ab^-1 integrated luminosities, with minor corrections of references and text. 2 figures added. To appear in JHE

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    Last time updated on 11/12/2019