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a splitting corresponding to the spin–spin coupling J
of
with more dilute samples, as illustrated by the NMR signal
shown in Figure S4 and obtained with a 40 mm VA solution.
This indicates that PHIP RASER occurs at relatively low
concentrations of the HP substrate; in particular, lower
concentrations than those reported previously for the sponta-
neous emission of NMR signals with the dissolution dynamic
HAꢀHB
7
.0 Hz between proton HA and H in EA and HEP
B
[21]
(
Figures 2b and 3b, respectively).
While the HP state
decays, the number of RASER-active lines changes, for
example from two RASER-active lines in Figures 2b and 3b
to one single line in Figures 2c and 3c. This can be explained
by different transverse relaxation rates and multiplicities of
each RASER line. For instance, at low polarization, only one
line with the highest amplitude in the NMR spectrum and
with the smallest linewidth overcomes the RASER threshold
and is RASER-active.
[23]
nuclear polarization (d-DNP) technique.
ALTADENA
RASER activity was also observed while leaving the catheter
(1/16’’ outer diameter, 1/32’’ inner diameter) inside the NMR
tube, thus creating more stringent conditions for its occur-
rence because the presence of the catheter leads to a signifi-
All ALTADENA-hyperpolarized RASER spectra in
Figures 2 and 3 differ significantly from the corresponding
PHIP spectra in Figures 2g and 3g. The latter feature the HP
resonances of H and H with the quartet and triplet lines of
cant susceptibility-induced B gradient and effectively shorter
0
T * (see Figures S5,S6). Note that in additional PASADENA
2
experiments, the hydrogenation reactions were performed
within the RF coil, and RASER was detected immediately
A
B
opposite signs. These are separated by ꢁ 2.8 ppm ( ꢁ 174 Hz)
for EA and ꢁ 1.2 ppm ( ꢁ 74 Hz) for HEP. Specifically, the
linewidth of the quartet FWHM of ꢁ 4 Hz in Figure 2g is
significantly broader compared to the linewidth of each of the
triplet lines with a FWHM of ꢁ 2 Hz. This is more pro-
nounced in Figure 2e, where the difference in linewidth is
more than one order of magnitude. The same trend is
observed in Figure 3e,g. The reason for this is the sign and the
magnitude of the HP state, which introduce a broadening with
ktot > 1/T * of the quartet lines and a narrowing with k < 1/
after the cessation of p-H bubbling because the bubbles
2
induce a significant degradation of T * (likely below 1 ms)
2
that prevents RASER activity at this magnetic field.
These findings are crucial in the context of PHIP studies
and biomedical applications. The HP substrates used here can
indeed be employed as in-vivo contrast agents. For example,
HP HEP has been extensively studied as a potential contrast
[
24–26]
agent in angiography studies.
techniques rely on the application of RF pulses, especially in
Because some of the PHIP
1
3
the case of polarization transfer from protons to
C
2
tot
[
27–35]
T * of the triplet lines. For the RASER lines in Figure 2b and
2
nuclei,
the RF coils may interact with the highly
3
b, ktot is negative and the linewidth, in principal, is only
proton-hyperpolarized compounds, resulting in complicated
non-linear effects and depletion of hyperpolarization via
RASER activity. Therefore, RASER effects may be consid-
ered as an obstacle in this context. The use of untuned RF
limited by the finite measurement time and ultimately by the
[
22]
Cramꢁr–Rao condition.
spectra of VA and HEP hyperpolarized by ALTADENA
allow the J-coupling constant J to be determined with
We conclude that the RASER
[
36,37]
coils
may help mitigate the occurrence of RASER, so
HAꢀHB
enhanced precision but the chemical-shift difference between
that the hyperpolarized proton pool is not depleted prior to its
utilization during contrast-agent preparation. Moreover, the
recent advent of PHIP via side-arm hydrogenation (SAH)
significantly expanded the range of biomolecules (including
H and H is not measurable in this RASER experiment.
A
B
The analysis of the RASER-active signals in the PASA-
DENA case (Figures 2h and 3h) renders other interesting
observations in addition to the anticipated line-narrowing. In
particular, the Fourier spectra of the RASER-active signals
[17,38]
ethyl acetate) that can be hyperpolarized via PHIP.
With
this technique, a wide range of carboxylic acids have been
hyperpolarized and employed in vivo for metabolism track-
(
Figures 2i and 3i) exhibit two large central RASER lines
[
21,27,38–42]
separated by the chemical-shift difference dHA ꢀd between
ing.
Amid the peer-review evaluation of the present work,
another interesting study regarding PHIP-RASER by Prav-
HB
the HA and HB protons, that is, dHA ꢀd = 2.8 ppm
HB
(
ꢁ 174 Hz) for EA and 1.2 ppm ( ꢁ 74 Hz) for HEP. The
[
43]
two central lines are accompanied by evenly spaced small
sidebands, and the distance between two consecutive lines is
divtsev and co-workers was reported. In contrast with the
common and somewhat ordinary conditions we have pre-
sented here, Pravdivtsev et al. designed a specific experiment
dedicated to observe parahydrogen-induced RASER activity
under PASADENA conditions at a magnetic field of 14 T
exactly dHA ꢀd . This can be explained by the non-linear
HB
interaction between different RASER-active modes (here:
[
2]
two) leading to a frequency-comb-like spectrum. We also
even found frequency-comb-like spectra in the case of the
ALTADENA-pumped RASER, where the two central modes
[
43]
(600 MHz) and with a cryogenically cooled coil (Q ꢁ 500).
The catalyst activity was tuned for building up polarization
throughout an extended period of time (about 10 min) with
a continuous delivery of p-H . The pairwise p-H addition was
and all sidebands are spaced by J
. Moreover, the
HAꢀHB
resonance frequencies of the RASER-active protons (Figur-
es 2b,c and 3b,c) are sometimes shifted by about 1 ppm when
compared with the partial RASER and hyperpolarized ones.
We speculate that this is due to the magnetic-field fluctuations
induced by RASER. A detailed evaluation of these and other
non-linear phenomena will be published elsewhere.
A series of additional experiments were performed,
demonstrating further that the experimental conditions
necessary for observing RASER through PHIP reactions
are not stringent at all. RASER bursts can indeed be observed
2
2
performed with two substrates incorporating CꢂC triple
bonds. Without RF-pulse excitation, RASER activity was
detected only after bubbling p-H2 for about 90 s. Only
chemical shifts but no J-couplings could be determined in
these very-high-field experiments and the reported linewidths
(in the order of 1 Hz) of the RASER-active lines do not differ
significantly from the linewidth obtained by a corresponding
standard NMR spectrum (a few ppb at 600 MHz). The work
presented in this article differs in many regards. First and
&
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ꢀ 2020 Wiley-VCH Verlag GmbH & Co. KGaA, Weinheim
Angew. Chem. Int. Ed. 2020, 59, 2 – 9
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