Dirac oscillator in the near-horizon region of BTZ black hole

A. Guvendi, Faizuddin Ahmed
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Abstract

In this paper, we explore the evolution of a Dirac oscillator (DO) field within the near-horizon region of the Banados, Teitelboim, and Zanelli (BTZ) black hole (BH) by seeking exact solutions to the corresponding DO equation. We obtain the relativistic frequency expression and analyze impact of various parameters implicated in it. Our findings reveal that the damped mode of this fermionic oscillator field relies on the BH mass, spin of the fermionic field, and frequency of the oscillator field. Lastly, we focus into the quantum system for a zero oscillator frequency as a specific case and thoroughly analyze the obtained results.
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BTZ 黑洞近视界区的狄拉克振荡器
在本文中,我们通过寻求相应的狄拉克振荡器(DO)方程的精确解,探讨了狄拉克振荡器场在巴纳多斯、泰特布姆和扎内利(BTZ)黑洞(BH)近视界区域内的演化。我们得到了相对论频率表达式,并分析了其中涉及的各种参数的影响。我们的研究结果表明,这种费米子振荡场的阻尼模式取决于黑洞质量、费米子场的自旋和振荡场的频率。最后,我们以振荡器频率为零的量子系统为例,深入分析了所得结果。
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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