Radiative symmetry breaking in brane models

被引:56
作者
Antoniadis, I
Benakli, K [1 ]
Quirós, M
机构
[1] CERN, Div Theory, CH-1211 Geneva 23, Switzerland
[2] Ecole Polytech, Ctr Phys Theor, Unite EP, CNRS,UMR 7644, F-91128 Palaiseau, France
[3] Ecole Normale Super, Phys Theor Lab, Unite ENS, UMR 8549,CNRS, F-75231 Paris, France
[4] CSIC, Inst Estructura Mat, E-28006 Madrid, Spain
关键词
D O I
10.1016/S0550-3213(00)00357-6
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We propose a way to generate the electroweak symmetry breaking radiatively in non-supersymmetric type I models with string scale in the TeV region. By identifying the Higgs field with a tree-level massless open string state, we find that a negative squared mass term can be generated at one loop, It is finite, computable and typically a loop factor smaller than the string scale, that acts as an ultraviolet cutoff in the effective field theory. When the Higgs open string has both ends confined on our world brane, its mass is predicted to be around 120 GeV, i.e., that of the lightest Higgs in the minimal supersymmetric model for large tan beta and m(A) Moreover, the string scale turns out to be one to two orders of magnitude higher than the weak scale. We also discuss possible effects of higher order string threshold corrections that might increase the string scale and the Higgs mass. (C) 2000 Elsevier Science B.V. All tights reserved.
引用
收藏
页码:35 / 48
页数:14
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