Zobrazeno 1 - 10
of 4 266
pro vyhledávání: '"Wu, A. Q."'
Autor:
Liu, W., Li, S., Guo, N. -J., Zeng, X. -D., Xie, L. -K., Liu, J. -Y., Ma, Y. -H., Wu, Y. -Q., Wang, Y. -T., Wang, Z. -A., Ren, J. -M., Ao, C., Xu, J. -S., Tang, J. -S., Gali, A., Li, C. -F., Guo, G. -C.
Spin defects in atomically thin two-dimensional (2D) materials such as hexagonal boron nitride (hBN) attract significant attention for their potential quantum applications. The layered host materials not only facilitate seamless integration with opto
Externí odkaz:
http://arxiv.org/abs/2410.18892
Autor:
Tang, T. F., Xu, X. Q., Li, K., Wu, M. Q., Zhang, X. X., Gao, X., Li, G. Q., Xia, T. Y., Wang, D. Z.
Small edge-localized-mode (ELM), similar to the quasi-continuous exhaust (QCE), has been achieved by increasing the density at the separatrix. Starting from the Type-I ELM experimental data in EAST, we have performed a numerical separatrix density sc
Externí odkaz:
http://arxiv.org/abs/2204.07912
Molecular dynamics simulations were performed for five monatomic metallic liquids and the atomic structural characteristics and dynamical properties were systematically investigated and compared for understanding the underlying structural basis of li
Externí odkaz:
http://arxiv.org/abs/2204.01944
Publikováno v:
In Neurocomputing 28 December 2024 610
Publikováno v:
In Information Fusion March 2025 115
Autor:
Wang, Zhi, Xue, Wenyuan, Li, Kuangyu, Tang, Zhenhao, Liu, Yang, Zhang, Fan, Cao, Shengxian, Peng, Xianyong, Wu, Edmond Q., Zhou, Huaichun
Publikováno v:
In Applied Thermal Engineering 15 January 2025 259
Publikováno v:
In Information Fusion September 2024 109
Publikováno v:
Physical Review MATERIALS 5, 065801 (2021)
Perovskite SrTiO3 (STO) is an attractive photocatalyst for solar water splitting, but suffers from a limited photoresponse in the ultraviolet spectral range due to its wide band gap. By means of hybrid density functional theory calculations, we syste
Externí odkaz:
http://arxiv.org/abs/2105.14165
Employing the the stellar evolution code (Modules for Experiments in Stellar Astrophysics), we calculate yields of heavy elements from massive stars via stellar wind and core-collapse supernovae (CCSN) ejecta to interstellar medium (ISM). In our mode
Externí odkaz:
http://arxiv.org/abs/2102.01352
Publikováno v:
In The Innovation November 2024