Effect of quantum radiation pressure on the bubble dynamics in sonoluminescence

1998 ◽  
Vol 103 (5) ◽  
pp. 3078-3078
Author(s):  
Weizhong Chen ◽  
Rongjue Wei
2002 ◽  
Vol 66 (10) ◽  
Author(s):  
L. A. S. Machado ◽  
P. A. Maia Neto ◽  
C. Farina

2014 ◽  
Vol 1027 ◽  
pp. 44-47 ◽  
Author(s):  
Xi Jing Zhu ◽  
Ce Guo ◽  
Jian Qing Wang

The pressure field induced by cavitaion bubble is responsible for the grinding mechanism and the cutting chatter of power ultrasonic honing. Based on the cavitation bubble dynamics model in the grinding area of power ultrasonic honing, the radiation pressure field of cavitation bubble was established. Experimental results show that the bubble is distributed in the grinding area like honeycomb and the size is about 10μm. Numerical simulation of dynamics and pressure field of cavitation bubble was performed. Numerical results show the dynamic behavior of cavitation bubble presents grow, expend and collapse under an acoustic cycle. However the expansion amplitude of bubble can be decreased and the collapse time can be extended and even collapse after several acoustic cycles with increasing ambient bubble radius. The bubble radiation pressure during collapsing bubble increases with increasing ultrasonic amplitude and ultrasonic frequency. And the pressure value of collapsing bubble is about 10Mpa which is more an order of magnitude than atmospheric pressure.


2011 ◽  
Vol 12 (9-10) ◽  
pp. 826-836 ◽  
Author(s):  
Pierre Verlot ◽  
Alexandros Tavernarakis ◽  
Chiara Molinelli ◽  
Aurélien Kuhn ◽  
Thomas Antoni ◽  
...  

2019 ◽  
Vol 14 (1) ◽  
pp. 19-23 ◽  
Author(s):  
Min Jet Yap ◽  
Jonathan Cripe ◽  
Georgia L. Mansell ◽  
Terry G. McRae ◽  
Robert L. Ward ◽  
...  

1999 ◽  
Vol 24 (4) ◽  
pp. 259 ◽  
Author(s):  
Ben C. Buchler ◽  
Malcolm B. Gray ◽  
Daniel A. Shaddock ◽  
Timothy C. Ralph ◽  
David E. McClelland

2013 ◽  
Vol 88 (3) ◽  
Author(s):  
W. Zach Korth ◽  
Haixing Miao ◽  
Thomas Corbitt ◽  
Garrett D. Cole ◽  
Yanbei Chen ◽  
...  

2020 ◽  
Vol 74 (11) ◽  
Author(s):  
Sibilla Di Pace ◽  
Luca Naticchioni ◽  
Martina De Laurentis ◽  
Flavio Travasso

Abstract In this work we study the thermal noise of two monolithically suspended mirrors in a tabletop high-finesse optical cavity. We show that, given suitable seismic filters, such a cavity can be designed to be sensitive to quantum radiation pressure fluctuations in the audio band of gravitational wave interferometric detectors below 1 kHz. Indeed, the thermal noise of the suspensions and of the coatings constitutes the main limit to the observation of quantum radiation pressure fluctuations. This limit can be overcome with an adequate choice of mirror suspension and coating parameters. Finally, we propose to combine two optical cavities, like those modeled in this work, to obtain a tabletop quantum radiation pressure-limited interferometer. Graphical abstract


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