Gravitational waves and Black Hole perturbations in acoustic analogues

被引:0
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作者
Coviello, Chiara [1 ]
Chiofalo, Maria Luisa [2 ,3 ]
Grasso, Dario [3 ]
Liberati, Stefano [4 ,5 ,6 ]
Mannarelli, Massimo [7 ]
Trabucco, Silvia [7 ,8 ]
机构
[1] Kings Coll London, Dept Phys, The Strand, London WC2R 2LS, England
[2] Univ Pisa, Dipartimento Fis, Polo Fibonacci, Largo B Pontecorvo 3, I-56127 Pisa, Italy
[3] Sez Pisa, INFN, Polo Fibonacci, Largo B Pontecorvo 3, I-56127 Pisa, Italy
[4] Scuola Int Super Studi Avanzati SISSA, Phys Area,Via Bonomea 265, I-34136 Trieste, Italy
[5] Univ IFPU, Inst Fundamental Phys, Via Beirut 2, I-34014 Trieste, Italy
[6] Sez Trieste, INFN, Via Valerio 2, I-34127 Trieste, Italy
[7] INFN, Lab Nazl Gran Sasso, Via G Acitelli 22, I-67100 Assergi, AQ, Italy
[8] Gran Sasso Sci Inst, Viale Francesco Crispi 7, I-67100 Laquila, Italy
来源
AVS QUANTUM SCIENCE | 2025年 / 7卷 / 01期
关键词
D O I
10.1116/5.0241559
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Phonons in Bose-Einstein condensates propagate as massless scalar particles on top of an emergent acoustic metric. This hydrodynamics/gravity analogy can be exploited to realize acoustic black holes, featuring an event horizon that traps phonons. The authors show that by an appropriate external potential, gravitational wave-like perturbations of the acoustic metric can be produced. Such perturbations can be used to excite an acoustic black hole, which should then relax by phonon emission. (c) 2025 Author(s). All article content, except where otherwise noted, is licensed under a Creative Commons Attribution (CC BY) license (https://creativecommons.org/licenses/by/4.0/)
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页数:12
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