论文标题

另一个关于哈勃张力与海森堡不确定性原则的联系

Another look on the connections of Hubble tension with the Heisenberg Uncertainty Principle

论文作者

Trivedi, Oem

论文摘要

哈勃紧张局势是当今宇宙学面临的最激动人心的问题之一。在过去的几年中,已经提出了许多可能的解决方案,其中很多使用了许多新的和异国情调的物理思想来解决这个问题。但是最近显示的是,H0张力可能不需要新的物理学,而只需要对测量值进行更准确的讨论,有趣的是,海森伯格的不确定性原理对这种启示至关重要。因此,如果人们通过不确定性观察到超出不确定性的光子质量,那么原则上就可以调和张力。我们通过考虑了康普顿波长的修改,在这项工作中更详细地研究了这一点,这在关于不确定性与H0张力之间互连的初步讨论中至关重要。我们主要讨论两种类型的修改,一种基于普遍的不确定性原理(GUP),另一种基于更高维物理学的考虑。我们首先表明,最小的长度和最大动量基于GUP的修改都不能在所需的尺度上提供光子质量值,因此在这种情况下,我们无法从这种意义上解决张力。然后,我们表明,即使在结合了较高的尺寸效果后,也可以使光子质量在所需的尺度上,也无法以与(3+1)时空情况相同的意义来调和哈勃张力。通过这种方式,我们表明某些新的物理学考虑不能像使用原始的Heisenberg不确定性原理在(3+1)时空相同的意义上解决H0张力。

The Hubble tension is one of the most exciting problems that Cosmology faces today. A lot of possible solutions for it have already been proposed in the last few years, with a lot of them using a lot of new and exotic physics ideas to deal with the problem. But it was shown recently that the H0 tension might not require new physics but only a more accurate discussion of measurements and interestingly it was the Heisenberg uncertainty principle which was pivotal for that revelation. Accordingly, if one observed the photon mass beyond the indeterminacy through uncertainty then one could in principle reconcile the tension. We examine this in a greater detail in this work by taking into account modifications of the Compton wavelength, which was pivotal in the initial discussion on the interconnection between uncertainty and the H0 tension. We mainly discuss two types of modifications, one based on generalized uncertainty principles (GUP) and the other on higher dimensional physics considerations. We firstly show that both minimal length and maximal momentum GUP based modifications do not provide photon mass values on the required scales and hence we cannot address the tension in this sense at all in this case. We then show that one can get the photon mass to be on the required scales even after incorporating higher dimensional effects, one cannot reconcile the Hubble Tension in the same sense as in the (3+1) space-time case. In this way, we show that certain new physics considerations cannot address the H0 tension in the same sense as one can using the original Heisenberg uncertainty principle in a (3+1) space-time.

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