Non-minimal Coupling of the Higgs Boson to Curvature in an Inflationary Universe

被引:11
作者
Calmet, Xavier [1 ,2 ,3 ]
Kuntz, Ibere [1 ]
Moss, Ian G. [4 ]
机构
[1] Univ Sussex, Dept Phys & Astron, Brighton BN1 9QH, E Sussex, England
[2] Johannes Gutenberg Univ Mainz, PRISMA Cluster Excellence, D-55099 Mainz, Germany
[3] Johannes Gutenberg Univ Mainz, Mainz Inst Theoret Phys, D-55099 Mainz, Germany
[4] Newcastle Univ, Sch Math & Stat, Newcastle Upon Tyne NE1 7RU, Tyne & Wear, England
基金
英国科学技术设施理事会;
关键词
Inflation; Higgs; Electroweak vacuum stability; STANDARD MODEL; GRAVITY; CONSTANT; TENSOR;
D O I
10.1007/s10701-017-0131-2
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
In the absence of new physics around GeV, the electroweak vacuum is at best metastable. This represents a major challenge for high scale inflationary models as, during the early rapid expansion of the universe, it seems difficult to understand how the Higgs vacuum would not decay to the true lower vacuum of the theory with catastrophic consequences if inflation took place at a scale above GeV. In this paper we show that the non-minimal coupling of the Higgs boson to curvature could solve this problem by generating a direct coupling of the Higgs boson to the inflationary potential thereby stabilizing the electroweak vacuum. For specific values of the Higgs field initial condition and of its non-minimal coupling, inflation can drive the Higgs field to the electroweak vacuum quickly during inflation.
引用
收藏
页码:110 / 120
页数:11
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