Backreaction in acoustic black holes.

Backreaction in acoustic black holes.
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DOI:
10.1103/physrevlett.94.161302
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发表时间:
2004-05
影响因子:
8.6
通讯作者:
R. Balbinot;S. Fagnocchi;A. Fabbri;G. P. Procopio
R. Balbinot;S. Fagnocchi;A. Fabbri;G. P. Procopio
中科院分区:
物理与天体物理1区
文献类型:
--
作者:
R. Balbinot;S. Fagnocchi;A. Fabbri;G. P. Procopio

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给出了声黑洞中线性化量子涨落的反反应方程。视界附近的解,在一个降维范围内得到,表明声黑洞不同于史瓦西黑洞,当它们辐射声子时温度会降低。它们与近乎极端的Reissner-Nordström黑洞有着惊人的相似之处。
The backreaction equations for the linearized quantum fluctuations in an acoustic black hole are given. The solution near the horizon, obtained within a dimensional reduction, indicates that acoustic black holes, unlike Schwarzschild ones, get cooler as they radiate phonons. They show remarkable analogies with near-extremal Reissner-Nordström black holes.