Effect of magnetic particles on NMR spectra of Murchison meteorite organic matter and a polymer-based model system

被引:22
作者
Levin, E. M.
Bud'ko, S. L.
Mao, J. D.
Huang, Y.
Schmidt-Rohr, K. [1 ]
机构
[1] Iowa State Univ, Ames Lab DOE, Ames, IA 50011 USA
[2] Iowa State Univ, Dept Phys & Astron, Ames, IA 50011 USA
[3] Iowa State Univ, Dept Chem, Ames, IA 50011 USA
[4] Old Dominion Univ, Dept Chem & Biochem, Norfolk, VA 23529 USA
[5] Brown Univ, Dept Geol Sci, Providence, RI 02912 USA
基金
美国国家科学基金会; 美国国家航空航天局;
关键词
solid-state nuclear magnetic resonance; paramagnetic effect; meteorite organic matter; magnetic particles; H-1; sidebands;
D O I
10.1016/j.ssnmr.2007.01.002
中图分类号
O64 [物理化学(理论化学)、化学物理学];
学科分类号
070304 ; 081704 ;
摘要
Organic matter from the Murchison meteorite shows pronounced spinning sidebands of the H-1 MAS NMR spectrum and exhibits a large bulk magnetization of 0.75 emu/g extrapolated to 94 kOe at 300K. By comparison with data of diamagnetic polystyrene and laponite clay mixed with ferrimagnetic gamma-Fe2O3 nano-particles, we show that the spinning sidebands arise from a combination of dipolar couplings of a given H-1 to magnetic particles, seen in a backscattered-electron image, and to other protons. Signal loss and significant broadening of protonated-carbon peaks in C-13 MAS NMR spectra of polystyrene with Fe2O3 nano-particles is demonstrated, and implications for C-13 NMR spectroscopy of Murchison meteorite are discussed. (C) 2007 Elsevier Inc. All rights reserved.
引用
收藏
页码:63 / 71
页数:9
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