论文标题

最小延伸的光速(MEVSL)

The minimally extended Varying Speed of Light (meVSL)

论文作者

Lee, Seokcheon

论文摘要

即使存在各种不同的光速(VSL)宇宙学模型,但由于它们可能违反了基本物理学中的物理法律,它们仍然是主流的。为了将VSL作为一种可行的理论,它应该继承特殊相对论的成功,包括麦克斯韦方程和热力学。因此,我们采用的是光速,$ \ tilde c $在宇宙时间内而不是当地时间,即$ \ tilde c [z] $,其中$ z $是宇宙学的红移。当一个人描述背景FLRW宇宙时,可以使用诸如温度,密度和$ \ tilde c $之类的物理量来定义恒定时间超出表面。这是因为它们随着时间的流逝而发展,宇宙的同质性要求它们必须在平等的宇宙时间相等。 $ \ tilde c $的变化伴随着所有相关物理常数的关节变化,以满足洛伦兹的不变性,热力学和比安奇身份。我们将此VSL模型称为“最小扩展的VSL(MEVSL)”。我们通过使用当前的观测值来得出MEVSL的宇宙学观察力,并获得了$ \ tilde c $变化的约束。有趣的是,除了MEVSL的光度距离之外,$ z $和所有几何距离与一般相对性相同。但是,将MEVSL的Hubble参数重新缩放为$ h =(1+z)^{ - b/4} h^{(\ rm gr)} $,可以用作解决哈勃参数测量的张力的解决方案。在此手稿中,我们提供了MEVSL对包括BBN,CMB,SZE,BAO,SNE,SNE,GWS,H,H,SL和$Δα$在内的各种宇宙学观察的主要影响。

Even though there have been the various varying speed of light (VSL) cosmology models, they remain out of the mainstream because of their possible violation of physics laws built into fundamental physics. In order to be the VSL as a viable theory, it should inherit the success of special relativity including Maxwell equations and thermodynamics at least. Thus, we adopt that the speed of light, $\tilde c$ varies for the cosmic time not for the local time, i.e., $\tilde c[z]$ where $z$ is the cosmological redshift. When one describes the background FLRW universe, one can define the constant-time hypersurface by using physical quantities such as temperature, density, and $\tilde c$. It is because they evolve in time, and the homogeneity of the Universe demands that they must equal at the equal cosmic time. The variation of $\tilde c$ accompanies the joint variations of all related physical constants in order to satisfy the Lorentz invariance, thermodynamics, and Bianchi identity. We call this VSL model as a "minimally extended VSL (meVSL)". We derive cosmological observables of meVSL and obtain the constraints on the variation of $\tilde c$ by using the current observations. Interestingly, $z$ and all geometrical distances except the luminosity distance of meVSL are the same as those of general relativity. However, the Hubble parameter of meVSL is rescaled as $H = (1+z)^{-b/4} H^{(\rm GR)}$ which might be used as a solution for the tension of the Hubble parameter measurements. In this manuscript, we provide the main effects of meVSL on various cosmological observations including BBN, CMB, SZE, BAO, SNe, GWs, H, SL, and $Δα$.

扫码加入交流群

加入微信交流群

微信交流群二维码

扫码加入学术交流群,获取更多资源