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pro vyhledávání: '"Ma Cunliang"'
Future GW observatories, such as the Einstein Telescope (ET), are expected to detect gravitational wave signals, some of which are likely to overlap with each other. This overlap may lead to misidentification as a single GW event, potentially biasing
Externí odkaz:
http://arxiv.org/abs/2407.13239
In the future, the third generation (3G) gravitational wave (GW) detectors, exemplified by the Einstein Telescope (ET), will be operational. The detection rate of GW from binary neutron star (BNS) is expected to reach approximately $10^4$ per year. T
Externí odkaz:
http://arxiv.org/abs/2406.15813
Publikováno v:
Physical Review D, 2024, 109(4): 043009
The existing matched filtering method for gravitational wave (GW) search relies on a template bank. The computational efficiency of this method scales with the size of the templates within the bank. Higher-order modes and eccentricity will play an im
Externí odkaz:
http://arxiv.org/abs/2309.02030
With the rapid development of deep learning technology, more and more researchers apply it to gravitational wave (GW) data analysis. Previous studies focused on a single deep learning model. In this paper we design an ensemble algorithm combining a s
Externí odkaz:
http://arxiv.org/abs/2204.12058
In recent years, much work have studied the use of convolutional neural networks for gravitational-wave detection. However little work pay attention to whether the transient noise can trigger the CNN model or not. In this paper, we study the response
Externí odkaz:
http://arxiv.org/abs/2103.03557
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Autor:
Ma, Cunliang, Lin, Wenbin
The conventional semi-empirical formula for collapse distance [Phys. Rev. 179, 862 (1969), Prog. Quant. Electr. 4, 35 (1975)] has been widely used in many applications. However, it is not applicable when the dispersion length is smaller than or has s
Externí odkaz:
http://arxiv.org/abs/1507.06382
Autor:
Ma, Cunliang, Lin, Wenbin
A parallel 2D+1 split-step Fourier method with Crank-Nicholson scheme running on multi-core shared memory architectures is developed to study the propagation of ultra-short high-intensity laser pulses in air. The parallel method achieves a near linea
Externí odkaz:
http://arxiv.org/abs/1507.05988
Publikováno v:
In Optics Communications 1 March 2020 458