科诺普赖亚-日登科旋转非克尔黑洞的磁再连接与能量提取

Fen Long, Shangyun Wang, Songbai Chen, Jiliang Jing
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摘要

最近,磁重联作为一种新的能量提取机制引起了广泛关注,它依赖于麦积层内磁场线的快速重联。我们研究了在具有额外形变参数的科诺普利亚-日登科向非克尔黑洞时空中通过磁再连接提取能量的特性。我们的研究结果表明,正变形参数扩大了能量提取的可能区域,提高了磁重联与布兰福-兹纳杰克过程的最大功率、最大效率和能量提取的最大比率。这意味着,在科诺普利亚-日登科旋转非克尔黑洞时空中,通过磁重联提取的能量比克尔黑洞情况下更多。变形参数的这些影响可能会为未来的黑洞天文观测和引力理论验证提供有价值的线索。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Magnetic Reconnection and Energy Extraction from a Konoplya-Zhidenko rotating non-Kerr black hole
Recently, magnetic reconnection has attracted considerable attention as a novel energy extraction mechanism, relying on the rapid reconnection of magnetic field lines within the ergosphere. We have investigated the properties of the energy extraction via magnetic reconnection in a Konoplya-Zhidenko rotating non-Kerr black hole spacetime with an extra deformation parameter. Our results show that the positive deformation parameter expands the possible region of energy extraction and improves the maximum power, maximum efficiency, and the maximum ratio of energy extraction between magnetic reconnection and the Blandford-Znajek process. This means that in the Konoplya-Zhidenko rotating non-Kerr black hole spacetime one can extract more energy via magnetic reconnection than in the Kerr black hole case. These effects of the deformation parameter may provide valuable clues for future astronomical observations of black holes and verification of gravity theories.
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