射电光子对之间伽马射线爆发时间延迟的相关性

Golden Gadzirayi Nyambuya, Simbarashe Marusenga, Godson Fortune Abbey, Prospery Christopher Simpemba, Joseph Simfukwe
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引用次数: 0

摘要

我们提出了一个试点研究的时间延迟Δt在四个GRB射电余辉发射,即不同频率的无线电波的到达时间延迟从八个GRB射电余辉发出。与大多数关于这一现象的研究不同,我们并不认为这种时间延迟是由于光子被赋予了非零质量,但这很可能是由于星际空间是一个冷稀薄的宇宙等离子体,介质的电子与光子的电子成分相互作用,从而产生微小的电流,导致色散,因此,频率(v)依赖于光的速度,这个速度缩放为v-1。上述相互作用是这样的,较低频率的光子将以较低的速度传播,从而导致不同频率的光子到达时间的观察到的时间延迟。与提出的模型合理一致,我们发现对于其中四个GRB余辉,观测到的时间延迟与频率之间存在很强的非请求相关性。如果这个模型可以被足够大的数据集证实,那么这个模型就有希望更好地理解grb中观测到的时间延迟。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Correlation in Gamma Ray Burst Time Delays between Pairs of Radio Photons
We present a pilot study of time delays Δt in four GRB Radio Afterglow emissions, i.e., delays in the arrival times of radio waves of different frequencies emanating from eight GRB Radio Afterglows. Unlike in most studies on this phenomenon, we do not assume that this time delay is due to the Photon being endowed with a non-zero mass, but that this may very well be due to the interstellar space being a cold rarefied cosmic plasma, which medium’s Electrons interact with the electric component of the Photon, thus generating tiny currents that lead to dispersion, hence, a frequency (v) dependent speed of Light where this speed scales off as v-1. The said interaction is such that, lower frequency Photons will propagate at lower speeds than higher frequency Photons thus leading to the observed time delays in the arrivals times of Photons of different frequencies. In reasonable accord with the proposed model, we find that for four of these GRB afterglows, there is a strong unsolicited correlation between the observed time delays and the frequency. If this model can be corroborated by a large enough data set, there is hope that this same model might lead to a better understanding of the observed time delays in GRBs.
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