Electroweak dark matter at future hadron colliders

被引:29
|
作者
Han, Tao [1 ,2 ,3 ]
Mukhopadhyay, Satyanarayan [1 ,4 ]
Wang, Xing [1 ]
机构
[1] Univ Pittsburgh, Dept Phys & Astron, PITT PACC, Pittsburgh, PA 15260 USA
[2] Tsinghua Univ, Dept Phys, Beijing 100086, Peoples R China
[3] Collaborat Innovat Ctr Quantum Matter, Beijing 100086, Peoples R China
[4] Indian Assoc Cultivat Sci, Dept Theoret Phys, Kolkata 700032, India
基金
美国国家科学基金会;
关键词
RELIC ABUNDANCE;
D O I
10.1103/PhysRevD.98.035026
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In a large class of scenarios, dark matter (DM) particles that belong to a multiplet of the standard model (SM) weak interactions are challenging to probe in direct detection experiments due to loop-suppressed cross sections. Direct production at colliders is thus crucial to look for such DM candidates, and under current estimates, future runs of the 14-TeV LHC are projected to probe masses of around 300 GeV for DM belonging to an SU(2) doublet (Higgsino-like), and 900 GeV for SU(2) triplet (winolike). We examine how far this mass reach can be extended at the proposed 27-TeV high-energy upgrade of the LHC (HE-LHC), and compare the results to the case for a 100-TeV hadron collider. Following a detector setup similar to that of the ATLAS tracking system for the run-2 LHC upgrade, with a new insertable b-layer (IBL), a disappearing charged track analysis at the HE-LHC can probe Higgsino-like (winolike) DM mass of up to 600 GeV (2.1 TeV) at the 95% C.L. The monojet and missing transverse momentum search, on the otherhand, has a weaker reach of 490 GeV (700 GeV) at 95% C.L. for the Higgsino-like (winolike) states. The mass range accessible in the collider searches can be complementary to the indirect detection probes using gamma rays from dwarf-spheroidal galaxies.
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页数:11
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