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首页> 外文期刊>Advances in high energy physics >The Nonequilibrium Back Reaction of Hawking Radiation to a Schwarzschild Black Hole
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The Nonequilibrium Back Reaction of Hawking Radiation to a Schwarzschild Black Hole

机译：Hawking辐射到Schwarzschild黑洞的非质量反应

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We investigate the nonequilibrium back reaction on the Schwarzschild black hole from the radiation field. The back reactions are characterized by the membrane close to the black hole. When the membrane is thin, we found that larger temperature difference can lead to more significant negative surface tension, larger thermodynamic dissipation cost, and back reaction in energy and entropy as well as larger black hole area. This may be relevant to the primordial black holes in early universe. Moreover, our nonequilibrium model can resolve the inconsistency issue of the black hole back reaction under zero mass limit in the equilibrium case. In the thick membrane case, the nonequilibrium back reaction is found to be more significant than that in the thin membrane case. The nonequilibrium temperature difference can increase the energy and entropy loss as well as the thermodynamic dissipation of the black hole and the membrane back reactions. The nonequilibrium dissipation cost characterized by the entropy production rate appears to be significant compared to the entropy rate radiated by the black hole under finite temperature difference. This may shed light on the black hole information paradox due to the information loss from the entropy production rate in the nonequilibrium cases. The nonequilibrium thermodynamic fluctuations can also reflect the effects of the back reactions of the Hawking radiation on the evolution of a black hole.
机译：我们研究了辐射场的施瓦茨柴尔德黑洞上的非Quibibribrium反应。背反应的特征在于靠近黑洞的膜。当膜很薄时，我们发现较大的温差会导致更大的负面表面张力，更大的热力耗散成本，以及能量和熵的反应以及更大的黑洞区域。这可能与早期宇宙的原始黑洞有关。此外，我们的非支配模型可以在均衡壳体中的零质量限制下解析黑洞反应的不一致问题。在厚膜壳中，发现不足反应比薄膜壳体更显着。非平衡温度差可以增加能量和熵损失以及黑洞的热力耗散和膜背反应。与有限温度差异辐射的黑洞辐射的熵速率相比，具有熵产生率的非识别耗散成本似乎是显着的。这可能会在黑洞信息悖论上阐明，由于从非凝固情况下的熵产生率的信息丢失。非QuibiBribrium热动力波动还可以反映霍克辐射对黑洞演变的反应的影响。

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