Strong Gravitational Lensing by Bardeen Black Hole in Cloud of Strings

Bijendra Kumar Vishvakarma, Shubham Kala, Sanjay Siwach
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Abstract

We investigate the gravitational lensing by Bardeen black hole in cloud of strings (CoS) in strong field limit. The effect of CoS parameter $b$ has been outlined in comparison with Bardeen black hole lens. The impact parameter increases as we increase the CoS parameter consequently more photons approach towards lens. We also obtain magnification of relativistic images and determine relativistic Einstein rings by using the parameters of two astrophysical black hole lenses $SgrA^{*}$ and $M87^{*}$. We constrain CoS parameter of black hole using EHT observations for these black holes. We also consider the time delay of signals in the presence of CoS parameter. It is significantly measurable for supermassive black hole $M87^{*}$ than $SgrA^{*}$. This analysis would constrain the Bardeen black hole in CoS as one of the candidates of primordial gravitational lens.
弦云中的巴丁黑洞产生的强引力透镜效应
我们研究了强场极限下弦云(CoS)中巴丁黑洞的引力透镜现象。与巴丁黑洞透镜相比,我们概述了CoS参数$b$的影响。随着 CoS 参数的增大,影响参数也随之增大,从而有更多的光子接近透镜。我们还利用两个天体物理黑洞透镜 $SgrA^{*}$ 和 $M87^{*}$ 的参数,获得了相对论图像的放大率,并确定了相对论爱因斯坦环。我们利用对这些黑洞的 EHT 观测来约束黑洞的 CoS 参数。我们还考虑了CoS参数存在时信号的时间延迟。与SgrA^{*}$相比,超大质量黑洞M87^{*}$的CoS参数明显可以测量。这一分析将限制CoS中的巴丁黑洞成为原初引力透镜的候选者之一。
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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