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修正的色散关系与对EDGES异常的一种可能解释。

Modified dispersion relations and a potential explanation of the EDGES anomaly.

作者信息

Das Saurya, Fridman Mitja, Lambiase Gaetano, Stabile Antonio, Vagenas Elias C

机构信息

Theoretical Physics Group and Quantum Alberta, Department of Physics and Astronomy, University of Lethbridge, 4401 University Drive, Lethbridge, AB T1K 3M4 Canada.

Dipartimento di Fisica E.R: Caianiello, Universita di Salerno, Via Giovanni Paolo II, 132, Fisciano, 84084 Salerno, Italy.

出版信息

Eur Phys J C Part Fields. 2022;82(8):720. doi: 10.1140/epjc/s10052-022-10680-8. Epub 2022 Aug 18.

Abstract

The (EDGES) collaboration has recently reported an important result related to the absorption signal in the Cosmic Microwave Background radiation spectrum. This signal corresponds to the red-shifted 21-cm line at , whose amplitude is about twice the expected value. This represents a deviation of approximately from the predictions of the standard model of cosmology, i.e. the CDM model. This opens a window for testing new physics beyond both the standard model of particle physics and the CDM model. In this work, we explore the possibility of explaining the EDGES anomaly in terms of modified dispersion relations. The latter are typically induced in unified theories and theories of quantum gravity, such as String/M-theories and Loop Quantum Gravity. These modified dispersion relations affect the density of states per unit volume and thus the thermal spectrum of the Cosmic Microwave Background photons. The temperature of the 21-cm brightness temperature is modified accordingly giving a potential explanation of the EDGES anomaly.

摘要

(EDGES)合作团队最近报告了一项与宇宙微波背景辐射光谱中的吸收信号相关的重要成果。该信号对应于红移后的21厘米谱线,其幅度约为预期值的两倍。这表示与宇宙学标准模型(即ΛCDM模型)的预测大约有[具体偏差数值未给出]的偏差。这为检验超越粒子物理学标准模型和ΛCDM模型的新物理打开了一扇窗口。在这项工作中,我们探索了用修正色散关系来解释EDGES异常的可能性。后者通常在统一理论和量子引力理论中诱导产生,例如弦/M理论和圈量子引力。这些修正色散关系会影响单位体积的态密度,进而影响宇宙微波背景光子的热谱。21厘米亮度温度会相应改变,从而为EDGES异常提供了一种潜在解释。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ca16/9388467/f13d393d2d42/10052_2022_10680_Fig1_HTML.jpg

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