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Plasma-Based Graphene Functionalization in Glow Discharge 被引量:1
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作者 x. fang J. Donahue +1 位作者 A. Shashurin M. Keidar 《Graphene》 2015年第1期1-6,共6页
Glow discharge was utilized to add oxygen functional groups to the graphene platelets sample produced in chemical exfoliation synthesis. It was concluded based on Raman spectra that the graphene sample treated with th... Glow discharge was utilized to add oxygen functional groups to the graphene platelets sample produced in chemical exfoliation synthesis. It was concluded based on Raman spectra that the graphene sample treated with the glow discharge preserves specific graphene features while no transformation to amorphous carbon is happening. SEM and EDS results indicated the increases of oxygen content in the graphene sample after the exposure to the glow discharge. Raman spectra also support the fact that the graphene platelets have been decorated with oxygen as the result of the glow discharge treatment. 展开更多
关键词 GRAPHENE FUNCTIONALIZATION Plasma-Based
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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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