Next-to-leading-order QCD corrections to e+e− → H + γ
Sun QF(孙青峰); Sang, W.-L., 陈文; Feng F(冯锋); Jia Y(贾宇); W. Chen, F. Feng, Y. Jia and Q.-F. Sun
刊名PHYSICS LETTERS B
2017
卷号775页码:152-159
关键词Standard Model Higgs boson QCD corrections
ISSN号0370-2693
DOI10.1016/j.physletb.2017.10.044
文献子类Article
英文摘要The associated production of Higgs boson with a hard photon at lepton collider, i.e., e(+)e(-) -> H gamma, is known to bear a rather small cross section in Standard Model, and can serve as a sensitive probe for the potential new physics signals. Similar to the loop-induced Higgs decay channels H -> gamma gamma, Z gamma, the e(+)e(-) -> H gamma process also starts at one-loop order provided that the tiny electron mass is neglected. In this work, we calculate the next-to-leading-order (NLO) QCD corrections to this associated H + gamma production process, which mainly stem from the gluonic dressing to the top quark loop. The QCD corrections are found to be rather modest at lower center-of-mass energy range (root s < 300 GeV), thus of negligible impact on Higgs factory such as CEPC. Nevertheless, when the energy is boosted to the ILC energy range (root s approximate to 400 GeV), QCD corrections may enhance the leading-order cross section by 20%. In any event, the e(+)e(-) -> H gamma process has a maximal production rate sigma(max) approximate to 0.08 fb around root s= 250 GeV, thus CEPC turns out to be the best place to look for this rare Higgs production process. In the high energy limit, the effect of NLO QCD corrections become completely negligible, which can be simply attributed to the different asymptotic scaling behaviors of the LO and NLO cross sections, where the former exhibits a milder decrement alpha 1/s, but the latter undergoes a much faster decrease alpha 1/s(2). (C) 2017 The Author(s). Published by Elsevier B.V.
电子版国际标准刊号1873-2445
WOS关键词ELECTROWEAK RADIATIVE-CORRECTIONS ; HIGGS-BOSON ; FEYNMAN DIAGRAMS ; E+E-ANNIHILATION ; STANDARD MODEL ; 2-PHOTON DECAY ; PARTICLES ; COLLIDERS ; PHYSICS ; QUARKS
WOS研究方向Astronomy & Astrophysics ; Physics
语种英语
WOS记录号WOS:000417190700021
内容类型期刊论文
源URL[http://ir.ihep.ac.cn/handle/311005/284579]  
专题高能物理研究所_理论物理室
作者单位中国科学院高能物理研究所
推荐引用方式
GB/T 7714
Sun QF,Sang, W.-L., 陈文,Feng F,et al. Next-to-leading-order QCD corrections to e+e− → H + γ[J]. PHYSICS LETTERS B,2017,775:152-159.
APA 孙青峰,Sang, W.-L., 陈文,冯锋,贾宇,&W. Chen, F. Feng, Y. Jia and Q.-F. Sun.(2017).Next-to-leading-order QCD corrections to e+e− → H + γ.PHYSICS LETTERS B,775,152-159.
MLA 孙青峰,et al."Next-to-leading-order QCD corrections to e+e− → H + γ".PHYSICS LETTERS B 775(2017):152-159.
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