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pro vyhledávání: '"Wang, Zhenru"'
Autor:
Wang, Zhenrui
The performance of a manufacturing system relies on its four types of elements: operators, machines, computer system and material handling system. To ensure the performance of these elements, operational data containing various aspects of information
Externí odkaz:
http://hdl.handle.net/10150/301673
Publikováno v:
In Renewable Energy October 2024 233
Publikováno v:
In Measurement 28 February 2024 226
Autor:
Reisinger, Christoph, Wang, Zhenru
In this article, we analyse the accuracy and computational complexity of estimators for expected functionals of the solution to multi-dimensional parabolic stochastic partial differential equations (SPDE) of Zakai-type. Here, we use the Milstein sche
Externí odkaz:
http://arxiv.org/abs/1904.08334
Akademický článek
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Autor:
Reisinger, Christoph, Wang, Zhenru
In this article, we propose an implicit finite difference scheme for a two-dimensional parabolic stochastic partial differential equation (SPDE) of Zakai type. The scheme is based on a Milstein approximation to the stochastic integral and an alternat
Externí odkaz:
http://arxiv.org/abs/1802.07682
Autor:
Wang, Zhenru, Reisinger, Christoph
In this article, we propose a space-time Multi-Index Monte Carlo (MIMC) estimator for a one-dimensional parabolic stochastic partial differential equation (SPDE) of Zakai type. We compare the complexity with the Multilevel Monte Carlo (MLMC) method o
Externí odkaz:
http://arxiv.org/abs/1612.02811
Autor:
Reisinger, Christoph, Wang, Zhenru
Publikováno v:
Journal of Computational Mathematics, 2018 Mar 01. 36(2), 202-236.
Externí odkaz:
https://www.jstor.org/stable/45151487
Publikováno v:
Publ.Astron.Soc.Jap. 58 (2006) 153-158
We have calculated the evolution of low-mass X-ray binaries that leads to the formation of the binary radio pulsars like PSR J1713+0747. We show that the mass transfer is most likely to be nonconservative, due to unstable disk accretion, to account f
Externí odkaz:
http://arxiv.org/abs/astro-ph/0512558
Autor:
Sun, Ming, Wang, Zhenru
Based on the data from the \asca observation of SNRs Kes79 and W49B, we present here the analysis of their X-ray spectra and morphologies. The Kes79 spectrum can be well fitted by a single NEI component, and the narrow-band images of that source show
Externí odkaz:
http://arxiv.org/abs/astro-ph/9911322