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带电有质量标量场对带电黑洞时空的量子效应

Quantum effects of charged massive scalar fields on charged black hole space-times

Cormac Breen, George Montagnon, Peter Taylor, Elizabeth Winstanley

arXiv 2608.19359首次发表:更新:

AI 中文总结

该研究计算Reissner-Nordstrom黑洞上有质量带电量子标量场的相关重整化期望值,采用不同方案处理不同量子态,通过高效数值方法探索含近极端黑洞电荷等的参数空间,揭示带电有质量标量场对带电黑洞时空的量子效应。

AI 中文摘要

我们计算了Reissner-Nordstrom黑洞上有质量带电量子标量场的标量凝聚、电荷流和应力-能量张量的重整化期望值,该标量场质量足够大,不存在经典超辐射。我们给出了Boulware、Unruh和Hartle-Hawking态的结果:Hartle-Hawking态的重整化期望值采用高效且准确的模式求和方案计算,另外两个态则采用态减法。数值方法的高效性使我们能探索大部分参数空间,包括近极端黑洞电荷和接近超辐射极限的标量场质量。

英文摘要

We compute the renormalized expectation values of the scalar condensate, charge current and stress-energy tensor for a massive charged quantum scalar field on a Reissner-Nordstrom black hole. The mass of the scalar field is sufficiently large that classical superradiance is absent. We present results for the Boulware, Unruh and Hartle-Hawking states. Renormalized expectation values in the Hartle-Hawking state are computed using an efficient and accurate mode sum prescription, and for the other two states we employ state subtraction. The efficiency of our numerical method enables us to explore a large part of the parameter space, including near-extremal black hole charges and scalar field masses close to the superradiant limit.

Comments23 pages, 15 figures

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