Detecting Rotational Superradiance in Fluid Laboratories

被引:37
作者
Cardoso, Vitor [1 ,2 ,3 ]
Coutant, Antonin [4 ]
Richartz, Mauricio [5 ]
Weinfurtner, Silke [4 ]
机构
[1] Univ Lisbon, Inst Super Tecn, Dept Fis, CENTRA, Ave Rovisco Pais 1, P-1049 Lisbon, Portugal
[2] Perimeter Inst Theoret Phys, Waterloo, ON N2J 2W9, Canada
[3] CERN, Dept Theoret Phys, CH-1211 Geneva 23, Switzerland
[4] Univ Nottingham, Sch Math Sci, Nottingham NG7 2RD, England
[5] Univ Fed ABC UFABC, Ctr Matemat Comp & Cognicao, BR-09210170 Sao Paulo, Brazil
基金
英国工程与自然科学研究理事会; 巴西圣保罗研究基金会;
关键词
GRAVITY-WAVES; BLACK-HOLE; AMPLIFICATION; REFLECTION; STABILITY;
D O I
10.1103/PhysRevLett.117.271101
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Rotational superradiance was predicted theoretically decades ago, and is chiefly responsible for a number of important effects and phenomenology in black-hole physics. However, rotational superradiance has never been observed experimentally. Here, with the aim of probing superradiance in the lab, we investigate the behavior of sound and surface waves in fluids resting in a circular basin at the center of which a rotating cylinder is placed. We show that with a suitable choice for the material of the cylinder, surface and sound waves are amplified. Two types of instabilities are studied: one sets in whenever superradiant modes are confined near the rotating cylinder and the other, which does not rely on confinement, corresponds to a local excitation of the cylinder. Our findings are experimentally testable in existing fluid laboratories and, hence, offer experimental exploration and comparison of dynamical instabilities arising from rapidly rotating boundary layers in astrophysical as well as in fluid dynamical systems.
引用
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页数:6
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