Zobrazeno 1 - 10
of 17
pro vyhledávání: '"Zhen-Peng Chen"'
Autor:
Long Chen, Zhen-Peng Chen, Jin-Jie Zhou, Jiahao Kang, Chang Ming Chiu, Charles Kim, Luo Haojun, Jie-Hui Qin, Ze Yuan, Wei Peng, Kun Zhang, Jian-Peng Li, Jiha Kim, Zihong Bill Liu, Bong-Geum Lee, Yu Xiaojun
Publikováno v:
SID Symposium Digest of Technical Papers. 51:1040-1043
Publikováno v:
SID Symposium Digest of Technical Papers. 51:1818-1821
Autor:
M. Hankins, Ross T. Smith, V. Z. Golkhou, Yuhan Yao, Eric C. Bellm, Jesper Sollerman, Richard Dekany, James D. Neill, Reed Riddle, Frank J. Masci, Michael Porter, R. Lunnan, B. Rusholme, Stephen Kaye, Anna Y. Q. Ho, Mickael Rigault, Virginia Cunningham, Ofer Yaron, Daniel J. Reiley, Kaushik De, Dmitry A. Duev, Christoffer Fremling, David L. Shupe, A. L. Miller, Melissa L. Graham, Shrinivas R. Kulkarni, Daniel A. Perley, Zhen-Peng Chen, Leonardo Tartaglia, Steve Schulze, Eran O. Ofek, Mansi Kasliwal, Kirsty Taggart, Claes Fransson, Przemek Mróz, Jacob E. Jencson, Maayane T. Soumagnac, Tao Chen, Avishay Gal-Yam, Lin Yan, Russ R. Laher, Igor Andreoni
Publikováno v:
Astrophys.J.Lett.
Astrophys.J.Lett., 2020, 902 (1), pp.L8. ⟨10.3847/2041-8213/abb8c5⟩
The Astrophysical journal letters
The Astrophysical journal letters, Bristol : IOP Publishing, 2020, 902 (1), pp.L8. ⟨10.3847/2041-8213/abb8c5⟩
The Astrophysical Journal
Astrophys.J.Lett., 2020, 902 (1), pp.L8. ⟨10.3847/2041-8213/abb8c5⟩
The Astrophysical journal letters
The Astrophysical journal letters, Bristol : IOP Publishing, 2020, 902 (1), pp.L8. ⟨10.3847/2041-8213/abb8c5⟩
The Astrophysical Journal
Helium is expected to be present in the ejecta of some hydrogen-poor superluminous supernovae (SLSN-I). However, so far only one event, PTF10hgi has been identified with He features in its photospheric spectra (Quimby et al. 2018). We present the dis
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9ce839ce5b6959f771ac48b4da75d35a
https://hal.science/hal-02899270
https://hal.science/hal-02899270
Publikováno v:
Computers & Fluids. 176:170-181
The weakly compressible material point method (WCMPM) suffers from volumetric-locking and numerical oscillation in modeling fluid flow and fluid-structure interaction problems. In this paper, a v-pformulation of the material point method (vp-MPM) is
Publikováno v:
Acta Mechanica Solida Sinica. 31:1-18
In a bird strike, the bird undergoes large deformation like flows; while most part of the structure is in small deformation, the region near the impact point may experience large deformations, even fail. This paper develops a coupled shell-material p
Publikováno v:
Computer Methods in Applied Mechanics and Engineering. 321:124-144
The explicit material point method (MPM) works successfully in modeling high frequency problems, but it is very computationally expensive in simulating low frequency with small time steps or quasi-static problems. Thus, several groups have developed
Publikováno v:
Computer Methods in Applied Mechanics and Engineering. 293:1-19
For extreme deformation problems, material point method (MPM) takes competitive advantages compared with finite element method (FEM) which often encounters mesh distortion. However, for small deformation problems, FEM is still more efficient and accu
Autor:
Zhen-Peng Chen, Zhen-Min Liu, Yan-Zhong Wang, Fu-Ting Wang, Xue-Jun He, Bao-Qiang Feng, Guo-Ying Su
Publikováno v:
DEStech Transactions on Computer Science and Engineering.
In this paper, the research object is taxi robots, firstly, establish three-dimensional physical model of robots and add material properties in Pro/E, and import ADAMS software to set up dynamics model; Then set up the drive system functions in MATLB
Autor:
Ye-Ying Sun, Jian-Kai Yu, Kan Wang, Yu-Gang Ma, Zhen-Peng Chen, Zhen-Dong An, G.T. Fan, Bo-Song Huang, Hang-Hua Xu, Yong-Jiang Li
Publikováno v:
Physical Review C. 92
Publikováno v:
The Astrophysical Journal. 817:L5
A new astrophysical reaction rate for C-12(alpha, gamma)O-16 has been evaluated on the basis of a global R-matrix fitting to the available experimental data. The reaction rates of C-12(alpha, gamma)O-16 for stellar temperatures between 0.04