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Electrical Tree Simulation Based on the Self-Organization Criticality
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作者 H. M. Hu Y. Yang +1 位作者 w. lu G. P. Zhao 《Energy and Power Engineering》 2013年第4期1273-1276,共4页
So far much effort has been made to understand the development of electrical treeing. For the simulation based study of electrical treeing, the most common method is to apply DBM stochastic model to simulate the growi... So far much effort has been made to understand the development of electrical treeing. For the simulation based study of electrical treeing, the most common method is to apply DBM stochastic model to simulate the growing of electrical treeing patterns. Previous simulation results showed that this stochastic model is capable of simulating the real electrical treeing patterns in a point-to-plane electrode system. However, this model only allows the tree channels to propagate on equipotential lines proportional to local electrical field. Therefore, it is necessary to develop a novel stochastic model to simulate the electrical patterns in order to get a good agreement with experimental results. 展开更多
关键词 FRACTAL Electrical TREE SIMULATION SELF-ORGANIZATION CRITICALITY
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2-6 First Direct Measurement of 12C(12C, n)23Mg at Stellar Energies
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作者 Tang Xiaodong B. Bucher +28 位作者 X. Fang A. Heger S. Almaraz-Calderon A. Alongi A.D. Ayangeakaa M. Beard A. Best J. Browne C. Cahillane M. Couder R.J. deBoer A. Kontos L. Lamm Y.J. Li A. Long w. lu S. Lyons M. Notani D. Patel N. Paul M. Pignatari A. Roberts D. Robertson K. Smith E. Stech R. Talwar w.P. Tan M. wiescher S.E. woosley 《IMP & HIRFL Annual Report》 2015年第1期56-58,共3页
The first stars in the early Universe were formed about 400 million years after the big bang. Verification of the existence of these stars is important for our understanding of the evolution of the Universe[1]. It has... The first stars in the early Universe were formed about 400 million years after the big bang. Verification of the existence of these stars is important for our understanding of the evolution of the Universe[1]. It has been predicted that for Population-III stellar production yields, the abundances of odd-Z elements are remarkably deficient compared to their adjacent even-Z elements[2]. Astronomers are searching for long-lived, low mass stars with the unique nucleosynthetic pattern matching the predicted yields[3]. 展开更多
关键词 FIRST DIRECT MEASUREMENT
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