Dark gauge bosons: LHC signatures of non-abelian kinetic mixing

被引:17
|
作者
Arguelles, Carlos A. [1 ,2 ,3 ]
He, Xiao-Gang [4 ,5 ,6 ]
Oyanesyan, Grigory [7 ]
Peng, Tao [1 ]
Ramsey-Musolf, Michael J. [7 ,8 ]
机构
[1] Univ Wisconsin, Dept Phys, 1150 Univ Ave, Madison, WI 53706 USA
[2] Wisconsin IceCube Particle Astrophys Ctr, Madison, WI 53703 USA
[3] MIT, 77 Massachusetts Ave, Cambridge, MA 02139 USA
[4] Shanghai Jiao Tong Univ, Dept Phys & Astron, INPAC, Shanghai 200240, Peoples R China
[5] Natl Taiwan Univ, Dept Phys, Taipei 10617, Taiwan
[6] Natl Ctr Theoret Sci, Div Phys, Hsinchu 30013, Taiwan
[7] Univ Massachusetts Amherst, Amherst Ctr Fundamental Interact, Dept Phys, Amherst, MA 01003 USA
[8] CALTECH, Kellogg Radiat Lab, Pasadena, CA 91125 USA
基金
美国国家科学基金会;
关键词
D O I
10.1016/j.physletb.2017.04.037
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We consider non-abelian kinetic mixing between the Standard Model SU(2)(L) and a dark sector U(1)' gauge group associated with the presence of a scalar SU(2)(L) triplet. The magnitude of the resulting dark photon coupling is an element of is determined by the ratio of the triplet vacuum expectation value, constrained to by less than or similar to 4 GeV by electroweak precision tests, to the scale Lambda of the effective theory. The corresponding effective operator Wilson coefficient can be O(1) while accommodating null results for dark photon searches, allowing for a distinctive LHC dark photon phenomenology. After outlining the possible LHC signatures, we illustrate by recasting current ATLAS dark photon results into the non-abelian mixing context. (C) 2017 The Authors. Published by Elsevier B.V.
引用
收藏
页码:101 / 107
页数:7
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