Static and Dynamic Components of the Redshift

Rajendra P. Gupta
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引用次数: 8

Abstract

We analyse the possibility that the observed cosmological redshift may be cumulatively due to the expansion of the universe and the tired light phenomenon. Since the source of both the redshifts is the same, they both independently relate to the same proper distance of the light source. Using this approach we have developed a hybrid model combining the Einstein de Sitter model and the tired light model that yields a slightly better fit to Supernovae Ia redshift data using one parameter than the standard ΛCDM model with two parameters. We have shown that the ratio of tired light component to the Einstein de Sitter component of redshift has evolved from 2.5 in the past, corresponding to redshift 1000, to its present value of 1.5. The hybrid model yields Hubble constant H0 =69.11(±0.53)km·s-1 ·Mpc-1 and the deceleration parameter q0 =-0.4. The component of Hubble constant responsible for expansion of the universe is 40% of H0 and for the tired light is 60% of H0. Consequently, the critical density is only 16% of its currently accepted value; a lot less dark matter is needed to make up the critical density. In addition, the best data fit yields the cosmological constant density parameter =0. The tired light effect may thus be considered equivalent to the cosmological constant in the hybrid model.
红移的静态和动态分量
我们分析了观测到的宇宙学红移可能是由于宇宙膨胀和累光现象而累积的可能性。由于两个红移的来源是相同的,它们都独立地与光源的相同固有距离有关。利用这种方法,我们开发了一个混合模型,将爱因斯坦德西特模型和累光模型结合起来,使用一个参数比使用两个参数的标准ΛCDM模型更适合超新星Ia红移数据。我们已经表明,累光分量与红移的爱因斯坦德西特分量的比值已经从过去的2.5(对应于红移1000)发展到现在的1.5。混合模型得到哈勃常数H0 =69.11(±0.53)km·s-1·Mpc-1,减速参数q0 =-0.4。哈勃常数中负责宇宙膨胀的部分是H0的40%而疲劳光的部分是H0的60%。因此,临界密度仅为当前可接受值的16%;要达到临界密度所需的暗物质要少得多。此外,最佳的数据拟合得到宇宙常数密度参数=0。因此,可以认为累光效应等同于混合模型中的宇宙学常数。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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