Calmet Xavier
Department of Physics and Astronomy, University of Sussex, Brighton, BN1 9QH UK.
Eur Phys J C Part Fields. 2017;77(11):729. doi: 10.1140/epjc/s10052-017-5324-5. Epub 2017 Nov 1.
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.
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。