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希格斯玻色子真空期望值的宇宙学演化。

Cosmological evolution of the Higgs boson's vacuum expectation value.

作者信息

Calmet Xavier

机构信息

Department of Physics and Astronomy, University of Sussex, Brighton, BN1 9QH UK.

出版信息

Eur Phys J C Part Fields. 2017;77(11):729. doi: 10.1140/epjc/s10052-017-5324-5. Epub 2017 Nov 1.

Abstract

We point out that the expansion of the universe leads to a cosmological time evolution of the vacuum expectation of the Higgs boson. Within the standard model of particle physics, the cosmological time evolution of the vacuum expectation of the Higgs leads to a cosmological time evolution of the masses of the fermions and of the electroweak gauge bosons, while the scale of Quantum Chromodynamics (QCD) remains constant. Precise measurements of the cosmological time evolution of , where and are, respectively, the electron and proton mass (which is essentially determined by the QCD scale), therefore provide a test of the standard models of particle physics and of cosmology. This ratio can be measured using modern atomic clocks.

摘要

我们指出,宇宙的膨胀导致希格斯玻色子真空期望值的宇宙学时间演化。在粒子物理学的标准模型中,希格斯真空期望值的宇宙学时间演化导致费米子和电弱规范玻色子质量的宇宙学时间演化,而量子色动力学(QCD)的尺度保持不变。因此,对(\frac{m_e}{m_p})宇宙学时间演化的精确测量(其中(m_e)和(m_p)分别是电子和质子质量,质子质量本质上由QCD尺度决定)提供了对粒子物理学和宇宙学标准模型的检验。这个比率可以用现代原子钟来测量。

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本文引用的文献

2
Further evidence for cosmological evolution of the fine structure constant.
Phys Rev Lett. 2001 Aug 27;87(9):091301. doi: 10.1103/PhysRevLett.87.091301. Epub 2001 Aug 9.

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