Natural anomaly mediation from the landscape with implications for LHC SUSY searches

被引:3
|
作者
Baer, Howard [1 ]
Barger, Vernon [2 ]
Bolich, Jessica [1 ]
Dutta, Juhi [1 ]
Sengupta, Dibyashree [3 ]
机构
[1] Univ Oklahoma, Dept Phys & Astron, Norman, OK 73019 USA
[2] Univ Wisconsin, Dept Phys, Madison, WI 53706 USA
[3] INFN, Lab Nazl Frascati, Via E Fermi 54, I-00044 Frascati, RM, Italy
关键词
SOFT SUPERSYMMETRY-BREAKING; MISSING TRANSVERSE-MOMENTUM; PP COLLISIONS; ROOT-S=13 TEV; FINAL-STATES; HIGGS MASS; HIGH-SCALE; GAUGE; MODEL;
D O I
10.1103/PhysRevD.109.035011
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Supersymmetric models with the anomaly-mediated supersymmetry (SUSY) breaking (AMSB) form for soft SUSY breaking terms arise in two different settings: (1) extra-dimensional models where SUSY breaking occurs in a sequestered sector, and (2) 4 - d models with dynamical SUSY breaking in a hidden sector where scalars gain masses of order the gravitino mass m3=2, but gaugino masses and trilinear soft terms are assumed to be of the AMSB form. Both models run into serious conflicts with (1) LHC sparticle and Higgs mass constraints, (2) constraints from winolike weakly interacting massive particle dark matter searches, and (3) bounds from naturalness. These conflicts may be avoided by introducing minor changes to the underlying phenomenological models consisting of nonuniversal bulk scalar Higgs masses and A terms, providing a setting for natural anomaly mediation (nAMSB). In nAMSB, the wino is still expected to be the lightest of the gauginos, but the Higgsinos are expected to be the lightest electroweakinos (EWinos) in accord with naturalness. We examine what sorts of spectra are expected to emerge when nAMSB arises from a string landscape setting: While model 2 can only be natural for a Higgs mass mh less than or similar to 123 GeV, model 1 can accommodate naturalness along with mh 125 GeV while still respecting LHC bounds on sparticle masses. We explore the LHC phenomenology of nAMSB models where we find that for Higgsino pair production, typically larger dilepton mass gaps arise from the soft dilepton-plus-jets signature than in models with gaugino mass unification. For wino-pair production, the higher m3=2 portion of nAMSB parameter space is excluded by recent LHC bounds from gaugino pair production searches. We characterize the dominant LHC signatures arising from the remaining lower m3=2 90-200 TeV range of parameter space, which should be fully testable at high-luminosity LHC via EWino pair production searches.
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页数:19
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