论文标题
基于一般阳米尔斯对称性的重型电荷的暗能量的模型
A Model for Dark Energy Based on Baryonic Charges with General Yang-Mills Symmetry
论文作者
论文摘要
惯性框架中的阳米尔斯对称性和杨米尔斯重力提出了一种可能从质子和中子的巴里子电荷来理解暗能量现象的可能性。通用规格变换涉及矢量规函数和汉密尔顿的特征相函数，而不是标量表函数和通常的相函数。一个具有四阶仪表方程，导致在两个点重指电荷之间产生静态线性电势。该模型与引力力一起预测，在早期宇宙中，当重力占主导地位时，不仅以降低的速度发生扩展，因此由于$ 1/r^2 $依赖性，减速的变化速率也降低了。在当前的宇宙中，当重态力占主导地位时，宇宙加速度应大致恒定，并具有最大值$ a_ {max} \ of 10^{ - 13} m/s^2 $，如惯性框架所测量。我们希望将来可以测试延迟宇宙加速的这些特性。
General Yang-Mills symmetry and Yang-Mills gravity in inertial frames presents a possible avenue for understanding dark energy phenomenon in terms of the extremely small baryon charges of protons and neutrons. General gauge transformations involve vector gauge functions and Hamilton's characteristic phase functions rather than scalar gauge functions and usual phase functions. One has fourth-order gauge field equations, which lead to a static linear potential between two point baryonic charges. Together with gravitational force, the model predicts that in the early universe, when the gravitational force was dominant, not only was the expansion occurring at a decreasing rate, the rate of change of the deceleration was decreasing due to a $1/r^2$ dependence. In the present universe, when the baryonic force is dominant, the cosmic acceleration should be approximately constant and has a maximum value $a_{max}\approx 10^{-13} m/s^2$, as measured in an inertial frame. We hope that these properties of the late-time cosmic acceleration can be tested in the future.
