Sensitivity enhancement of the central transition NMR signal of quadrupolar nuclei under magic-angle spinning

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1 September 2000 Ž. Chemical Physics Letters 327 2000 85 90 www.elsevier.nlrlocatercplett Sensitivity enhancement of the central transition NMR signal of quadrupolar nuclei under magic-angle spinning Zhi Yao a, Hyung-Tae Kwak a, Dimitris Sakellariou b, Lyndon Emsley b, Philip J. Grandinetti a,) a Department of Chemistry, The Ohio State UniÕersity, 120 W. 18th AÕenue, Columbus, OH 43210-1173, USA b Laboratoire de Stereochimie et des Interactions Moleculaires, UMR 5532 ENS-LyonrCNRS, Ecole Normale Superieure de Lyon, 69364 Lyon, France Received 1 March 2000; in final form 1 June 2000 Abstract An approach for enhancing the NMR sensitivity of the central transition of spin-3r2 nuclei is presented. Through selective excitation of the satellite transitions using a fast 1808 phase alternating pulse train during magic-angle spinning a selectively excited state is prepared where the populations of all eigenstates < m: with the same sign of m are equal, resulting in an enhanced central msy1r2 1r2 transition polariation. Numerical simulations predict enhancements up to a factor of 2 and values of 1.7 and 1.9 have been obtained experimentally for 23 Na in Na C O and 87 Rb in RbClO 4, respectively. We observe no significant anisotropic lineshape distortion. The conditions for optimum enhancement are discussed. q 2000 Published by Elsevier Science B.V. 1. Introduction In 1993 Haase and Conradi wx 1 proposed a method of enhancing the polariation of the central transition of half-integer spin I quadrupolar nuclei by a factor of 2 I using selective inversion of the outer satellite transitions. This effect was demonstrated on 27 Al in a static single crystal of a-al 2O 3, where the predicted enhancement factor of 5 was obtained. Using frequency swept adiabatic passages Hasse and Conradi demonstrated that a somewhat reduced enhancement of 4.1 could also be obtained in polycrystalline ) Corresponding author. Fax: q1-614-292-1685; e-mail: grandinetti.1@osu.edu a-al O. In a subsequent paper, Haase et al. wx 2 3 2 presented a more detailed theoretical picture to describe such polariation enhancements in static samw3,4x have examined ples. Kentgens and coworkers the advantages of employing double frequency Ži.e., amplitude modulated. adiabatic sweeps to not only enhance central transition polariation in static samples but also in samples undergoing magic-angle spinning Ž MAS., and to enhance multiple-quantum to single-quantum coherence transfer in MQ-MAS w5,6 x. In the case of polariation enhancement for the central transition of 23 Na, where the theoretical maximum enhancement factor is 3, they obtained factors of ; 2.7 and ; 1.7 in Na 2SO4 under static and MAS conditions, respectively. The reduced enhancement during MAS was explained as due to an inter- 0009-2614r00r$ - see front matter q 2000 Published by Elsevier Science B.V. Ž. PII: S0009-2614 00 00805-8

86 Z. Yao et al.rchemical Physics Letters 327 2000 85 90 ference between the frequency sweep and the transitions induced by MAS. More recently, Mahdu et al. wx 7 employed an X X pulse train with the goal of enhancing multiple-quantum to single-quantum coherence transfer in MQ-MAS and obtained enhancements similar to those obtained by Kentgens and Verhagen wx 4. An interesting difference in the two approaches is that Mahdu et al. maintain a constant cycle time in their X X pulse train, that is, the frequency is not swept as in the experiments of Kentgens and Verhawx 4. In a more recent paper, Mahdu et al. wx 8 gen explain the mechanism for this enhancement as coherence transfers induced by the adiabatic motion of the rotor w9,10 x, a mechanism similar to that of RIACT w11 x, but apparently more efficient. In light of the success of this approach for MQ- MAS we have investigated the utility of the X X pulse train in enhancing the central transition polariation in samples undergoing MAS. Such an approach has advantage over double-frequency sweeps that no special hardware is required for implementation and that the enhancements we obtain are similar than those obtained by Kentgens and Verhagen wx 4. 2. Experimental All experiments were performed on a 9.4 Tesla Chemagnetics CMX II spectrometer using a Chemagnetics 4 mm MAS probe operating at a 23 Na frequency of 105.82652 MH and a 87 Rb frequency of 130.932474 MH. The samples used for polariation enhancement experiments were polycrystalline Na C O and polycrystalline RbClO, which have 4 23 Na and 87 Rb quadrupolar coupling parameters of Cqs2.43 MH and hqs0.77, and Cqs3.3 MH and hqs 0.20, respectively. Using the saturation re- covery experiment the effective T of 6.4 s was measured for the 23 Na central transition in Na C O and 147 ms was measured for the 87 Rb central transition in RbClO 4. Experiments on Na 2C 2O4 were performed using a 10 s recycle delay and spinning speeds of 6 and 12 kh. Experiments on RbClO 4 were performed using a 1 s recycle delay and a spinning speed of 12 kh. The radiofrequency Ž rf. field strength was calibrated using the solid-state 23 Na resonance of NaCl and the 87 Rb resonance of 1 Fig. 1. Pulse sequence for RAPT from the satellites to the central transition for spin Is3r2. For optimum transfer the inverse of the cycle time of the X X unit is set to Cq r4. Experimentally, the optimum duration of the whole pulse train was found to be approximately one rotor period. RbCl. The pulse sequence for enhancing the central transition polariation is shown in Fig. 1. We call this approach rotor assisted population transfer Ž RAPT.. In practice, a 400 ns delay was inserted between each pulse in the X X pulse train of RAPT to allow time for the transmitter phase to stabilie. The X and X pulse lengths were equal, and the inverse of the total time to complete one X X interval Ž including the 400 ns delays. is defined as the RAPT modulation frequency, n m. 3. Results and discussion Comparisons of central transition spectra of 23 Na in polycrystalline Na C O and 87 Rb in polycrystalline RbClO4 with and without the RAPT preparation are shown in Fig. 2. A factor of 1.6 and 1.9 sensitivity enhancement is observed in Na C O and RbClO, respectively. Most importantly, there ap- 4 pears to be no significant lineshape distortions using RAPT, implying that all crystallite orientations experience the same enhancement. One possible mechanism for the enhancement involves the selective inversion of the satellite transitions, as depicted in Fig. 3a, by the fast amplitude modulated rf pulse, which only irradiates near the satellite transitions, and the motion of the rotor which acts to provide an adiabatic sweep. In this case, however, we would have expected significant lineshape distortions, since it is impossible, at any given time, for all crystallites to have undergone an odd number of adiabatic passages. Thus, there can-

Z. Yao et al.rchemical Physics Letters 327 2000 85 90 87 Fig. 2. A comparison of central transition spectra of Ž. a 23 Na in polycrystalline Na C O and Ž. b 87 Rb in polycrystalline RbClO4 with and without the RAPT preparation. In all cases, the spinning speed was 12 kh, and whole echo acquisition was used to eliminate lineshape distortions due to receiver deadtime. A RAPT modulation frequency and rf amplitude of nms550 kh and n 1s100 kh for Na 2C 2O4 and nms720 kh and n 1s175 kh for RbClO4 were employed. The RAPT duration in both cases was one rotor period. not be uniform inversion of the satellites for all crystallites using this scheme, and we would predict distortions in the anisotropic lineshapes, as some orientations will be enhanced by a factor of 3 and others will show no enhancement. An alternative mechanism consistent with our observations is that the enhancement is a result of an selective saturation of the satellite populations, as depicted in Fig. 3b, which occurs during the fast 1808 phase alternating pulse train with MAS. Although a true selectively saturated state, which in the language of fictitious spin half operators w12,13x corresponds to ² I 1 2 : s² I 3 4 : s0 Ž 1. x, y, x, y, in the spin-3r2 case, would lead to a factor of two enhancement, it is not necessary to achieve such a state to obtain the enhancement. Any selective deviation of ² I 1 2 : and ² I 3 4 : from equilibrium will lead to an enhancement, with the goal of RAPT being ² I 1 2 : s² I 3 4 : s0. Ž 2. Fig. 3. Ž. a Selective population inversion of the satellite transitions leads to a sensitivity enhancement of the central transition by a factor of 2 I. Ž. b Selective excitation or saturation of the satellite transitions leads to a sensitivity enhancement of the central transition by a factor of Iq1r2. Once this condition is satisfied the populations of all eigenstates < m: with the same sign of m will be equal, and an enhanced central m sy1r2 1r2 transition will be observed. The difference in maximum enhancements between the 23 Na and 87 Rb RAPT appear to arise from the stronger homonuclear dipolar couplings among 23 23 the more abundant Na nuclei Ži.e., 100% for Na 87 versus 27.85% for Rb., which generate transitions

88 Z. Yao et al.rchemical Physics Letters 327 2000 85 90 between neighboring 23 Na nuclei, thus reducing the efficiency of the selective population equaliation of levels having the same sign of m. When enhancing the polariation of the central transition by transferring polariation from the outer transitions it is also important that the outer transitions have re-equiw1,14 x. We investigated this as a possibility for the lesser librated before transferring polariation again enhancement in Na 2C 2O4 by increasing the recycle delay in the RAPT sequence from 10 to 100 s and found no change in the 23 Na polariation enhancement. To determine how sensitive the RAPT enhancement is to the setting of experimental parameters, we investigated its dependence on X X pulse train duration, the modulation frequency, and rf field strength. Shown in Fig. 4 is the experimental enhancement curve of the central transition spectra of 23 Na in Na 2C 2O4 as a function of the X X pulse train duration and the predicted curves for ² I 1 2 : r ² I 1 2 : eq, ² I 2 3 : r² I 2 3 : eq, and ² I 3 4 : r² I 3 4 : eq based on a full density matrix numerical calculation with the same conditions as the experiment. The shape of the experimental curve for ² I 2 3 : agrees qualitatively with the predicted curve, with the experimental enhancement maximum lying below the prediction. The simulated curves verify the selective saturation hypothesis presented above, with the enhancement in ² I 2 3 : increasing as the ² I 1 2 : and ² I 3 4 : expectation values approach ero. Fig. 5a shows the experimental and theoretical dependence of the RAPT enhancement for 23 Na in Na 2C 2O4 on the modulation frequency, n m. The modulation frequency was varied over a range of approximately 170 700 kh. The maximum experimental enhancement factor of 1.67 was found using a modulation frequency of 550 kh, a value not far from C r4s607.5 kh. Because of hardware conq straints, we were not able to experimentally explore modulation frequencies beyond 700 kh. Also shown in Fig. 5a, are numerical simulations which predict that the enhancement is diminished at higher modulation frequencies and drops to one for nm0cqr2, which in the case of Na C O is 1215 kh. Finally, we experimentally varied the rf field strength over a range of 10 100 kh at spinning speeds of n Rs 12 and n Rs 6 kh. These data along with theoretical predictions are shown in Fig. 5b. The enhancement decreases with decreasing rf field strength, and at very low rf field strengths there is no enhancement. Although it would be technically difficult to experimentally explore very high rf field strengths, numerical simulations shown in Fig. 5b predict that the enhancements would eventually di- 23 Fig. 4. Dependence of Na central transition signal enhancement in Na2C 2O4 on the duration of the X X pulse train in the RAPT sequence of Fig. 1 expressed in units of rotor period. The curves in grey are the simulated expectation values of the fictitious spin half operator I rys scaled by their equilibrium expectation values for the 1 2, 2 3, and 3 4 transitions. The curve in black is the experimental ² I 2 3 : r² I 2 3 : eq value measured by a selective pr2 pulse on the central transition. In both experiment and simulation a rf field strength of n 1 s101 KH was employed during the X X pulse train, with a modulation frequency of nm s427 KH, and a spinning frequency of 12 KH. With this combination there are approximately 35 X X cycles within about one rotor period. Optimum transfer appears to occur experimentally after one rotor period. The experimental time interval between the pulse train and acquire pulse was ts50 ms, and the recycle delay was 10 s. The simulations were based on a full density matrix calculation and were averaged over 3722 crystallite orientations.

Z. Yao et al.rchemical Physics Letters 327 2000 85 90 89 4. Conclusion Fig. 5. Ž. a Dependence of maximum RAPT enhancement on the modulation frequency. Filled squares show the experimental dependence for the 23 Na central transition in Na 2C 2O 4. For each point a series of experiments were performed with the total number of X X cycles varied in order to find the maximum enhancement. The modulation frequency, n m, is defined as the inverse of the total time to complete one X X interval. The n 1 field strength was held constant at 101 kh. The sample spinning frequency was 12 kh. Open squares show the predicted dependence of maximum signal enhancement on modulation frequency. Spinning speeds were varied slightly in order to maintain integral relationships between the X X cycle time and the rotor period. The Ž n,n. frequency pairs were Ž 100,11.11., Ž 200,11.11. m R Ž 301.205,10.76., Ž 403.2,10.61., Ž 500,10.42., Ž 595.2,10.26., Ž 694.4,10.21., Ž 806.5,10.21., Ž 892.9,10.15., Ž 1000,10.10., Ž 1087,10.06., Ž 1190,10.00., and Ž 1316,9.97. kh. Ž b. Dependence of signal enhancement on rf field strength with a fixed RAPT modulation frequency of nm s550 kh. Filled squares and circles correspond to experimental data collected for the 23 Na central transition in Na 2C 2O4 with n Rs12 kh and n Rs6 kh, respectively. Open squares show the predicted dependence of maximum signal enhancement on the rf field strength with nm s550 kh and n R s12 kh. All simulations were averaged over 3722 crystallite orientations. minish as one approaches the higher rf field strengths where the excitation of the central and satellite transitions are no longer selective. Using a simple X X pulse train with MAS we have shown that the sensitivity of the NMR signal for the central transition of spin-3r2 nuclei can be enhanced without significant anisotropic lineshape distortions by transferring polariation from the outer transitions via a selective excitation of the satellite transitions. The relevant parameters in optimiing the RAPT enhancement are the rf field strength and modulation frequency. The optimum modulation frequency appears to be on the order of nmscqr4 for a spin-3r2 nucleus, and may vary slightly depending on the value of h. We also found that the enhanceq ment gradually increased with increasing rf field strength, and through numerical simulations we predict that the enhancement will diminish as one approaches the higher rf field strengths where the excitation of the central and satellite transitions are no longer selective. Importantly, the enhancement factors are not critically sensitive to the X X pulse train modulation frequency or the rf amplitude, yielding a simple experimental protocol. Experimental enhancement factors of 1.7 were obtained in the case of the central transition of 23 Na in Na C O, and 1.9 in the case of 87 Rb in RbClO. Numerical simula- 4 tions predict that a maximum enhancement factor of 2 is possible. The less than optimal enhancements observed in Na C O appear to arise from homonu- clear dipolar couplings, which act to reduce the efficiency of the selective equaliation of populations among levels having the same sign of m. Extension of these ideas to higher spin quadrupolar nuclei with greater enhancements is possible, and in general, a theoretical maximum enhancement factor of Iq1r2 can be obtained with selective excitation of the all satellite transitions. Acknowledgements This work was supported in part by a grant from the National Science Foundation ŽNo. CHE- 9807498.. We thank Dr. Joseph Sachleben and Dr. Stefano Caldarelli for helpful discussions. P.J.G. also acknowledges support from the ENS Lyon for a visiting professorship during the early part of this work.

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