| Literature DB >> 26029349 |
Roman V Shchepin, Milton L Truong, Thomas Theis, Aaron M Coffey, Fan Shi, Kevin W Waddell, Warren S Warren, Boyd M Goodson, Eduard Y Chekmenev.
Abstract
We report NMR Signal Amplification by Reversible Exchange (SABRE) hyperpolarization of the rare isotopes in "neat" liquids, each composed only of an otherwise pure target compound with isotopic natural abundance (n.a.) and millimolar concentrations of dissolved catalyst. Pyridine (Py) or Py derivatives are studied at 0.4% isotopic natural abundance ¹⁵N, deuterated, ¹⁵N enriched, and in various combinations using the SABRE-SHEATH variant (microTesla magnetic fields to permit direct ¹⁵N polarization from parahydrogen via reversible binding and exchange with an Ir catalyst). We find that the dilute n.a. ¹⁵N spin bath in Py still channels spin order from parahydrogen to dilute ¹⁵N spins, without polarization losses due to the presence of ¹⁴N or ²H. We demonstrate P(15N) ≈ 1% (a gain of 2900 fold relative to thermal polarization at 9.4 T) at high substrate concentrations. This fundamental finding has a significant practical benefit for screening potentially hyperpolarizable contrast agents without labeling. The capability of screening at n.a. level of ¹⁵N is demonstrated on examples of mono- and dimethyl-substituted Py (picolines and lutidines previously identified as promising pH sensors), showing that the presence of a methyl group in the ortho position significantly decreases SABRE hyperpolarization.Entities:
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Year: 2015 PMID: 26029349 PMCID: PMC4442667 DOI: 10.1021/acs.jpclett.5b00782
Source DB: PubMed Journal: J Phys Chem Lett ISSN: 1948-7185 Impact factor: 6.475
Figure 1(A) Schematic of the 15N SABRE-SHEATH hyperpolarization process conducted in a pressurized (1–7 atm) 5 mm NMR tube with para-H2 bubbling.[20] (B) Schematic of the SABRE exchange process, wherein parahydrogen and a substrate, for example, pyridine, exchange on activated Ir-hydride complexes.[15]
Figure 2SABRE of “neat” natural abundance 15N (0.36%) pyridine (Py). (A) 15N SABRE-SHEATH hyperpolarized spectrum (red) and the corresponding thermally polarized reference spectrum (blue) after 192 signal averages. (B) 1H SABRE spectrum of hyperpolarized (red) sample in milliTesla magnetic field (∼6 mT) and the corresponding NMR spectrum using thermally polarized sample (blue). (C) Effect of the para-H2 flow rate (measured in standard cubic centimeters per minute or sccm) on 15N signal enhancement at ∼90 mM catalyst concentration under five para-H2 pressure values. (D) Effect of [Py] to [catalyst] ratio on 15N signal enhancement using 120 sccm flow rate under ∼7 atm of para-H2 pressure. (E) 15N SABRE-SHEATH dependence (modeled as exponential decay) as a function of the sample exposure to the microTesla magnetic field after stopping para-H2 bubbling time. (F) 15N T1 decay at 9.4 T. The experiments in panels E and F are conducted using ∼90 mM catalyst concentration (∼140:1 [Py] to [catalyst] ratio) at 120 sccm flow rate and ∼7 atm para-H2 pressure.
Summary of Experimental Results with Natural Abundance (n.a.) Pyridine (Py), Py-d5, 15N-Py, and Their Mixturesa
| [15N] (mM) | 15N ε @ 9.4T | 15N effective | 15N | 1H ε @9.4T | [catalyst] (mM) | ||
|---|---|---|---|---|---|---|---|
| 1) Py (n.a.) | ∼45 | ∼−2900 | 5.5(0.5) | 60.8(0.6) | ∼25000 | ∼−4.2 | ∼90 |
| 2) Py- | ∼45 | ∼−850 | 2.2(0.1) | 74.3(2.9) | ∼125 | ∼−60 | ∼90 |
| 3) 15N-Py | ∼12500 | ∼−33 | 10.2(1.1) | 66.8(0.5) | ∼25000 | ∼−0.3 | ∼90 |
| 4) catalyst activated with 15N-Py, then Py- | ∼2000 | ∼−520 | 10.1(0.8) | 69.9(0.3) | ∼4000 | ∼−2.6 | ∼90 |
| 5) catalyst activated with
Py- | ∼1800 | ∼−400 | 15.1(2.3) | 73.2(0.3) | ∼3600 | ∼−2.7 | ∼90 |
| 6) catalyst activated with 15N-Py, then in n.a. Py is added | ∼1800 | ∼−450 | 9.9(1.1) | 70.0(0.3) | ∼3600 | ∼−1.0 | ∼90 |
| 7) catalyst activated with n.a. Py, then 15N-Py is added | ∼1800 | ∼−380 | 8.2(1.1) | 69.9(0.3) | ∼3600 | ∼−0.6 | ∼90 |
Note the activation sequence, which determines the axial non-exchangeable ligand of the activated Ir-hydride catalyst complex. See the SI for details.
Conducted with >90% para-H2, while the rest of the data is collected using 65–75% para-H2, resulting in ∼30–40% lower signal enhancements compared with those shown in row 1. Note that the data for pairs 2 and 3, 4 and 5, and 6 and 7 were respectively collected on the same day at the same level of para-H2 enrichment and stored in a pressurized aluminum cylinder as previously described (and thus should be directly comparable).[40]
Figure 4Diagrams of para-H2 exchange and 15N SABRE-SHEATH hyperpolarization in the absence (A) and in the presence (B) of 14N-Py excess. Note that the exchange with 14N-Py does not cause a significant reduction in the spin order of the para-H2 pool. It should also be noted that both equatorial pyridines of the active complex undergo the chemical exchange with free Py in solution, while the axial pyridine (labeled as “Py”) is not exchangeable.
Figure 3Spin systems used for analytical derivation of the resonance conditions for (A) 15N-Py solutions and (B) n.a. Py solutions. In panel A, in addition to the displayed couplings, JHN = JH′N′ and JHN′ = JH′N. Couplings to spins in axial positions are ignored because they generally are smaller than equatorial couplings and play a subordinate role. (Additionally, this site does not exchange with free substrate.)
Figure 5Maximum 15N SABRE-SHEATH signal enhancements obtained for pyridine, picolines, and lutidines in neat liquids using ∼45 mM catalyst concentration and naturally abundant levels of 15N (∼0.35%) under ∼7 atm of para-H2 pressure and flow rate of 100–120 sccm. Note that the value labeled with a single asterisk (*) corresponds to the optimized catalyst concentration of ∼90 mM, the values labeled with double asterisks (**) correspond to the experiments conducted at 5 atm of para-H2 and the flow rate of 60 sccm, and n.d. stands for none detected.