Crystal Growth & Design
Article
R and S enantiomers, respectively. For the other two HSP
molecules, the C2A and C2B atoms are representative of S and
R enantiomers, respectively (Figure 1b). Overall, the HSP
molecules in TMZ-HSP are a racemic mixture. There is an
intramolecular O3−H3···O2 hydrogen bond between hydroxyl
and carbonyl groups in each HSP molecule. TMZ and HSP
molecules are connected through an O5−H5···O7 hydrogen
bond to form a dimer (Figure 1a). Two dimers are further
connected via a N6−H6A···O7 hydrogen bond between amide
groups of adjacent TMZ molecules to generate a tetramer. The
tetramers are held together through an O4−H4···O2 hydrogen
bond between hydroxyl and carbonyl groups of neighboring
HSP molecules to generate a one-dimensional (1D) belt
(Figure 1c). The belts are further stacked along the c axis to
form a 3D hydrogen-bonded framework structure (Figure 1d),
within which there also exist 1D hydrogen-bonded chain
structures of TMZ molecules (Figure 1e).
subsequent exothermic peak at 182.3 °C, which could be
attributed to the decomposition of the eutectic (Figure S1 in
the Supporting Information).
1H Nuclear Magnetic Resonance (1H NMR). The
chemical components in the new cocrystalline phase were
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1
further identified and confirmed by H NMR. The H NMR
spectrum of synthesized TMZ-HSP was the superposition of
the peaks of TMZ and HSP, except for the peaks of active
hydrogen (Figure S2 in the Supporting Information), which
indicates the presence of these two components in the new
phase. The 1H NMR chemical shift assignments are as follows:
peaks of TMZ, δ 8.83 (s, 1H), 7.81 (s, 1H), 7.69 (s, 1H), 3.87
(s, 3H); peaks of HSP, δ 6.91 (dd, J = 25.3, 8.4 Hz, 3H), 5.89
(dd, J = 5.6, 2.1 Hz, 2H), 5.42 (dd, J = 12.3, 3.0 Hz, 1H), 3.78
(s, 3H), 3.17 (dd, J = 17.1, 12.4 Hz, 1H), 2.72 (dd, J = 17.1,
3.1 Hz, 1H). The ratio of TMZ and HSP in the cocrystal was
calculated to be 1:1 by integrating the characteristic proton
signals of each component.
Powder X-ray Diffraction (PXRD) and Thermal
Analyses. PXRD analysis was utilized to identify the
crystalline phase and determine the phase purity of the bulk
sample of TMZ-HSP (Figure 2).34,35 The PXRD pattern of
Fourier Transform Infrared Spectroscopy (FTIR)
Analysis. FTIR spectra can further identify the intermolecular
interactions of functional groups involved by the changes in
their vibrational frequencies. The FTIR spectra for TMZ, HSP,
TMZ-HSP, and the corresponding physical mixture are
presented in Figure 3. HSP shows characteristic peaks at
Figure 2. Comparison of experimental and simulated PXRD patterns
of TMZ-HSP, HSP and TMZ.
Figure 3. FTIR spectra of TMZ, HSP, TMZ-HSP, and a physical
mixture (TMZ + HSP).
synthesized TMZ-HSP is distinguished from those of its
parent materials, suggesting the formation of a new crystalline
phase. Moreover, the experimental PXRD pattern is consistent
with the simulated pattern calculated from single-crystal data,
confirming the crystalline phase purity of the synthesized
cocrystal. The thermodynamic stability of the parent materials
and cocrystal was investigated by means of thermogravimetric
(TG) and differential scanning calorimetry (DSC) analyses.
From TG thermograms it can be seen that TMZ, HSP, and
TMZ-HSP are free from crystalline water or solvents in the
lattice and begin to decompose at approximately 186.8, 276.4,
and 199.8 °C, respectively. The DSC curve of HSP shows an
endothermic peak of melting at 232.4 °C, while those of TMZ
and TMZ-HSP show exothermic peaks at 202.2 and 200.9 °C,
respectively, corresponding to their decomposition processes
(Figure S1 in the Supporting Information). A TG and DSC
analysis of the 1:1 physical mixture of TMZ and HSP has also
been carried out. The DSC curve of the physical mixture
exhibits an endothermic peak at 178.0 °C, which could be
ascribed to the formation of a eutectic of TMZ and HSP, and a
1637 and 3500 cm−1, which are assigned to the carbonyl CO
and O−H stretching vibrations.36 The N−H stretching of
TMZ exhibits characteristic peaks at 3421 and 3388 cm−1, and
the stretching vibrations at 1759 and 1733 cm−1 correspond to
the CO stretching vibrations from the primary and tertiary
amides of TMZ, respectively.37 After the formation of TMZ-
HSP, the CO stretching vibrations were observed at 1635,
1699, and 1743 cm−1 and the O−H and N−H stretchings were
shifted to 3464 and 3301 cm−1, respectively. These spectral
peak shifts reflect that the amide groups of TMZ and the
hydroxyl and carbonyl groups of HSP participate in the change
in hydrogen-bonding modes accompanying cocrystal forma-
tion.
Dynamic Vapor Sorption (DVS) Study. A DVS study
was carried out to compare the hygroscopicity of TMZ-HSP
with those of the parent TMZ and HSP. The resulting vapor
sorption/desorption isotherms are depicted in Figure 4. The
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Cryst. Growth Des. 2021, 21, 838−846