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Entropy Conservation of Linear Dilaton Black Holes in Quantum Corrected Hawking Radiation

机译:量子校正的Hawking辐射中线性Dilaton黑洞的熵守恒

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摘要

It has been shown recently that information is lost in the Hawking radiation of the linear dilaton black holes in various theories when applying the tunneling formalism of Parikh and Wilczek without considering quantum gravity effects. In this paper, we recalculate the emission probability by taking into account the log-area correction to the Bekenstein-Hawking entropy and the statistical correlation between quanta emitted. The crucial role of the quantum gravity effects on the information leakage and black hole remnant is highlighted. The entropy conservation of the linear dilaton black holes is discussed in detail. We also model the remnant as an extreme linear dilaton black hole with a pointlike horizon in order to show that such a remnant cannot radiate and its temperature becomes zero. In summary, we show that the information can also leak out of the linear dilaton black holes together with preserving unitarity in quantum mechanics.
机译:最近显示,在不考虑量子引力效应的情况下应用帕里克(Parikh)和威尔切克(Wilczek)的隧道形式主义时,在各种理论中线性狄拉顿黑洞的霍金辐射中都丢失了信息。在本文中,我们通过考虑对Bekenstein-Hawking熵的对数区域校正和发射的量子之间的统计相关性,重新计算发射概率。突出了量子引力效应对信息泄漏和黑洞残留物的关键作用。详细讨论了线性膨胀黑洞的熵守恒。我们还将残留物建模为具有点状视界的极端线性Dilaton黑洞,以表明此类残留物无法辐射并且其温度变为零。总而言之,我们表明信息还可以从线性Dilaton黑洞中泄漏出来,同时还能保持量子力学中的统一性。

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