Hawking radiation can be interpreted as a quantum phenomenon of particles tunneling through black hole horizons. In this formulation, Kerner and Mann analyzed fermions emission via tunneling and investigated tunneling probabilities related to the Hawking temperature. This paper is devoted to the use of the Kerner and Mann technique for axially symmetric slowly rotating wormholes. We calculate tunneling probability for outgoing (as well as incoming) charged fermions and obtain their respective Hawking temperatures at horizon radii and also explore their graphical pictures.
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机译：霍金辐射可以解释为粒子穿过黑洞视界的量子现象。在此公式中，Kerner和Mann通过隧道分析了费米子的排放，并研究了与霍金温度有关的隧道概率。本文致力于将Kerner and Mann技术用于轴向对称的缓慢旋转的虫洞。我们计算输出（以及输入）带电费米子的隧穿概率，并获得其在水平半径处的霍金温度，并浏览其图形化图片。
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