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Endogenous Dynamic Nuclear Polarization for Natural Abundance 17 O and Lithium NMR in the Bulk of Inorganic Solids

  • Tamar Wolf
  • , Sandeep Kumar
  • , Harishchandra Singh
  • , Tanmoy Chakrabarty
  • , Fabien Aussenac
  • , Anatoly I. Frenkel
  • , Dan Thomas Major
  • , Michal Leskes
  • Weizmann Institute of Science
  • Stony Brook University
  • Bruker Corporation
  • United States Department of Energy

Research output: Contribution to journalArticlepeer-review

90 Scopus citations

Abstract

In recent years magic angle spinning-dynamic nuclear polarization (MAS-DNP) has developed as an excellent approach for boosting the sensitivity of solid-state NMR (ssNMR) spectroscopy, thereby enabling the characterization of challenging systems in biology and chemistry. Most commonly, MAS-DNP is based on the use of nitroxide biradicals as polarizing agents. In materials science, since the use of nitroxides often limits the signal enhancement to the materials' surface and subsurface layers, there is need for hyperpolarization approaches which will provide sensitivity in the bulk of micron sized particles. Recently, an alternative in the form of paramagnetic metal ions has emerged. Here we demonstrate the remarkable efficacy of Mn(II) dopants, used as endogenous polarization agents for MAS-DNP, in enabling the detection of 17 O at a natural abundance of only 0.038%. Distinct oxygen sites are identified in the bulk of micron-sized crystals, including battery anode materials Li 4 Ti 5 O 12 (LTO) and Li 2 ZnTi 3 O 8 , as well as the phosphor materials NaCaPO 4 and MgAl 2 O 4 , all doped with Mn(II) ions. Density functional theory calculations are used to assign the resonances to specific oxygen environments in these phases. Depending on the Mn(II) dopant concentration, we obtain significant signal enhancement factors, 142 and 24, for 6 Li and 7 Li nuclei in LTO, respectively. We furthermore follow the changes in the 6,7 Li LTO resonances and determine their enhancement factors as a function of Mn(II) concentration. The results presented show that MAS-DNP from paramagnetic metal ion dopants provides an efficient approach for probing informative nuclei such as 17 O, despite their low gyromagnetic ratio and negligible abundance, without isotope enrichment.

Original languageEnglish
Pages (from-to)451-462
Number of pages12
JournalJournal of the American Chemical Society
Volume141
Issue number1
DOIs
StatePublished - 9 Jan 2019

Bibliographical note

Publisher Copyright:
© 2018 American Chemical Society.

Funding

We thank Dr. Raanan Carmieli for help with the CW-EPR experiments. We are grateful to Dr. Ilia Kaminker for helpful suggestions and comments on the experiments, Prof. Shimon Vega for careful reading of the manuscript, and Shai Barlev for assistance with combinatorial calculations. We thank Prof. Daniella Goldfarb and Dr. Akiva Feintuch for acquiring the W band EPR spectra and Dr. Sabine Akabayov for help with fitting protocols of the relaxation data. This research was funded by the Planning & Budgeting Committee of the Council of High Education and the Prime Minister office of Israel, in the framework of the INREP project (M.L., D.T.M.), and the Israel Science Foundation (Grant No. 085170, M.L.) as well as support from a research grant from the Comisaroff Family Trust and Monroe and Marjorie Burk Fund for Alternative Energy Studies and the Merle S. Cahn Foundation (M.L.). H.S. and A.I.F. acknowledge support by NSF Grant No. DMR-1701747. This research used 8-ID (ISS) beamline of the National Synchrotron Light Source, a U.S. Department of Energy (DOE) Office of Science User Facility operated for the DOE Office of Science by Brookhaven National Laboratory under Contract No. DE-AC02-98CH10886. We also acknowledge the support of the BL2-2 beamline of the SSRL through the Synchrotron Catalysis Consortium (U.S. Department of Energy, Office of Basic Energy Sciences, Grant No. DE-SC0012335). Additionally, we thank Klaus Attenkofer and Janis Timoshenko for their help with EXAFS measurements at the NSLS-II and SSRL, respectively. The work was made possible in part by the historic generosity of the Harold Perlman family.

FundersFunder number
Comisaroff Family Trust
Council of High Education
DOE Office of Science
Merle S. Cahn Foundation
Office of Basic Energy Sciences
Prime Minister office of Israel
Synchrotron Catalysis Consortium
National Science Foundation
U.S. Department of Energy
Office of Science
Brookhaven National Laboratory
Israel Science Foundation085170

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