Superradiance in Dicke systems: A picture with field correlation functions

Author(s):  
Sergiy F. Lyagushyn ◽  
Alexander I. Sokolovsky
1992 ◽  
Vol 07 (33) ◽  
pp. 3059-3070 ◽  
Author(s):  
S. STIEBERGER ◽  
D. JUNGNICKEL ◽  
J. LAUER ◽  
M. SPALIŃSKI

The three-point correlation functions with twist fields are determined for bosonic ZN orbifolds. Both the choice of the modular background (compatible with the twist) and of the (higher) twisted sectors involved are fully general. We point out a necessary restriction on the set of instantons contributing to twist field correlation functions not obtained in previous calculations. Our results show that the theory is target space duality invariant.


Author(s):  
Gabriele Gradoni ◽  
Stephen C. Creagh ◽  
Gregor Tanner ◽  
Christopher Smartt ◽  
Mohd Hafiz Baharuddin ◽  
...  

1994 ◽  
Vol 50 (2) ◽  
pp. R925-R928 ◽  
Author(s):  
J. D. Cresser ◽  
S. M. Pickles

2015 ◽  
Vol 17 (9) ◽  
pp. 093027 ◽  
Author(s):  
Gabriele Gradoni ◽  
Stephen C Creagh ◽  
Gregor Tanner ◽  
Christopher Smartt ◽  
David W P Thomas

2019 ◽  
Vol 220 (3) ◽  
pp. 1521-1535
Author(s):  
Loïc Viens ◽  
Chris Van Houtte

SUMMARY Seismic interferometry is an established method for monitoring the temporal evolution of the Earth’s physical properties. We introduce a new technique to improve the precision and temporal resolution of seismic monitoring studies based on deep learning. Our method uses a convolutional denoising autoencoder, called ConvDeNoise, to denoise ambient seismic field correlation functions. The technique can be applied to traditional two-station cross-correlation functions but this study focuses on single-station cross-correlation (SC) functions. SC functions are computed by cross correlating the different components of a single seismic station and can be used to monitor the temporal evolution of the Earth’s near surface. We train and apply our algorithm to SC functions computed with a time resolution of 20 min at seismic stations in the Tokyo metropolitan area, Japan. We show that the relative seismic velocity change [dv/v(t)] computed from SC functions denoised with ConvDeNoise has less variability than that calculated from raw SC functions. Compared to other denoising methods such as the SVD-based Wiener Filter method developed by Moreau et al., the dv/v results obtained after using our algorithm have similar precision. The advantage of our technique is that once the algorithm is trained, it can be apply to denoise near-real-time SC functions. The near-real-time aspect of our denoising algorithm may be useful for operational hazard forecasting models, for example when applying seismic interferometry at an active volcano.


2010 ◽  
Vol 73 (11) ◽  
pp. 1970-1975
Author(s):  
V. D. Orlovsky ◽  
V. I. Shevchenko

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