Hawking Radiation in the Laboratory
Hawking Radiation in the Laboratory
复制标题
实验室中的霍金辐射
DOI:
10.1143/ptp.107.1267
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发表时间:
2001
影响因子:
--
通讯作者:
A. Ōhashi
中科院分区:
文献类型:
--
作者:
M. Sakagami;A. Ōhashi
We propose an experimental model using the Laval nozzle of a sonic analogue of Hawking radiation. We derive the power spectrum of the outgoing wave emitted from the vicinity of the sonic horizon instead of the created particle number. Our treatment is based on classical theory, and it should make experiments easier to implement. This experimental feasibility is a great advantage of our model. Black hole evaporation, so-called Hawking radiation, is one of the most surprising predictions in theoretical physics. 1), 2) Despite the importance of Hawking radiation, its actual observation in the universe is considered to be very difficult. For this reason, it seems quite natural to seek experiments in the laboratory that can simulate this interesting phenomenon. In addition, Unruh showed that there exists a sonic analogue of black holes. We speculate that something like Hawking radiation may be observed in the evaporation of these analogous structures. 3) 4) Of course, black hole evaporation is a quantum phenomenon. Thus, in the case of the corresponding laboratory experiments, we should maintain the quantum coherence of the entire system to observe processes of particle creation and changes of vacuum caused by the existence of the horizon. With this in mind, several experiments employing superfluid 3 He have been proposed. 5) 6) However, the supersonic motion of this fluid along the walls of the apparatus would cause the collapse of superfluidity and quantum coherence, because vortices may be created near the boundaries. Additionally, even in the an experimental system 6) designed to overcome this problem, no evidence of Hawking radiation has yet been reported.