Full O(α) electroweak radiative corrections to e+e- → e+e- γ at the ILC with GRACE-Loop

被引:6
作者
Khiem, P. H. [1 ,2 ]
Kurihara, Y. [1 ]
Fujimoto, J. [1 ]
Ishikawa, T. [1 ]
Kaneko, T. [1 ]
Kato, K. [3 ]
Nakazawa, N. [3 ]
Shimizu, Y. [1 ]
Ueda, T. [4 ]
Vermaseren, J. A. M. [5 ]
Yasui, Y. [6 ]
机构
[1] KEK, Tsukuba, Ibaraki 3050801, Japan
[2] SOKENDAI Univ, Hayama, Kanagawa 2400193, Japan
[3] Kogakuin Univ, Tokyo 1638677, Japan
[4] Karlsruhe Inst Technol, D-76128 Karlsruhe, Germany
[5] Nikhef, NL-1098 XG Amsterdam, Netherlands
[6] Tokyo Management Coll, Ichikawa, Chiba 2720001, Japan
关键词
DIFFERENTIAL CROSS-SECTION; HIGGS-BOSON PRODUCTION; QED BHABHA SCATTERING; HIGH-ENERGY-PHYSICS; PHOTONIC CORRECTIONS; LINEAR COLLIDERS; EMISSION; VERSION;
D O I
10.1016/j.physletb.2014.11.048
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
By using the GRACE-Loop system, we calculate the full O(alpha) electroweak radiative corrections to the process e(+)e(-) -> e(+)e(-) gamma, which is important for future investigations at the International Linear Collider (ILC). With the GRACE-Loop system, the calculations are checked numerically by three consistency tests: ultraviolet finiteness, infrared finiteness, and gauge-parameter independence. The results show good numerical stability when quadruple precision is used. In the phenomenological results, we find that the electroweak corrections to the total cross section range from similar to-4% to similar to-21% when.7s varies from 250 GeV to 1 TeV. The corrections also significantly affect the differential cross sections, which are a function of energies and angles of the final state particles. Such corrections will play an important role in the high-precision program at the ILC. (C) 2014 The Authors. Published by Elsevier B.V.
引用
收藏
页码:192 / 198
页数:7
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