scholarly journals Overview of localised flexural waves in wedges of power-law profile and comments on their relationship with the acoustic black hole effect

2020 ◽  
Vol 468 ◽  
pp. 115100 ◽  
Author(s):  
Victor V. Krylov
Materials ◽  
2019 ◽  
Vol 12 (15) ◽  
pp. 2480 ◽  
Author(s):  
Weiguang Zheng ◽  
Shiming He ◽  
Rongjiang Tang ◽  
Shuilong He

The acoustic black hole (ABH) effect for damping flexural waves using axially functionally graded porous (FGP) structure is investigated. With proposed power-law porosity of FGP structure, ABH can be achieved and damping effect is enhanced. The physics are explained from divergent conditions of the integrated wave phase at composite ends. Numerical results show the damping effect is increased with power law index. The phenomenon is expounded by the characteristics of reflection coefficient and impedance. It indicates that increasing power law index leads to smaller wavelength along to the end, then the wave needs more oscillation cycles to travel, which leads to more energy absorption. Transient analysis for 2D FGP structure also shows the focalization and ABH effect of the flexural waves.


2006 ◽  
Vol 21 (07) ◽  
pp. 593-601
Author(s):  
JILIANG JING

We study analytically the evolution of massless Dirac fields in the background of the Schwarzschild black hole. It is shown that although the quasinormal frequencies are the same for opposite chirality with the same |k|, we can differentiate neutrinos from anti-neutrinos in evolution of the massless Dirac fields provided we know both stages for the quasinormal modes and the power-law tail behavior since the decay rate of the neutrinos is described by t-(2|k|+1) while anti-neutrinos is t-(2|k|+3).


1996 ◽  
Vol 165 ◽  
pp. 363-367
Author(s):  
W.S. Paciesas ◽  
S.N. Zhang ◽  
B.C. Rubin ◽  
B.A. Harmon ◽  
C.A. Wilson ◽  
...  

A bright transient X-ray source, GRO J1655-40 (X-ray Nova Scorpii 1994) was discovered with BATSE (the Burst and Transient Source Experiment) in late July 1994. More recently, the source also became a strong radio emitter, its rise in the radio being approximately anti-correlated with a decline in the hard X-ray intensity. High-resolution radio observations subsequent to this symposium showed evidence for superluminally expanding jets. Since the hard X-ray emission extends to at least 200 keV and we find no evidence of pulsations, we tentatively classify the source as a black-hole candidate. However, its hard X-ray spectrum is unusually steep (power-law photon index α ≃ −3) relative to most other black-hole candidates. In this regard, it resembles GRS 1915+105, the first galactic source to show superluminal radio jets.


2020 ◽  
Vol 471 ◽  
pp. 115199 ◽  
Author(s):  
J. Leng ◽  
V. Romero-García ◽  
A. Pelat ◽  
R. Picó ◽  
J.-P. Groby ◽  
...  

2019 ◽  
Vol 99 (2) ◽  
Author(s):  
M. Ghanaatian ◽  
F. Naeimipour ◽  
A. Bazrafshan ◽  
M. Eftekharian ◽  
A. Ahmadi

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