The simulated optical absorption spectra may be directly compared with the observable time-resolved or final spectra of radiolysis. When fitting with the experimental ones, they give essential insights into the mechanisms of oxidation. It was mentioned in
Section 2.3 that the extraction of absorption spectra from molecular simulations is conditioned by the
fwhm parameter, i.e. the broadness of the gaussian function used for the convolution of TDDFT lines, and by the spin screening parameter, used for the empirical reduction of spin contamination in radical species. The choice of these parameters is discussed in SI, Section 5.0 and Figure SI 10 on the case of the R
•C
a radical. According to this discussion, three values of the
fwhm parameter will be used:
fwhm = 0.7 eV for the broadening of TDDFT lines of optimized structures,
fwhm = 0.50 eV for the broadening of TDDFT lines of the intense bands and for the weak, high energy bands of the simulation, and
fwhm = 0.20 eV for the weak, low energy bands of the simulation. The spin screening parameter will be 20%.
5.1. Absorption spectrum of Me2-crocetin
The absorption spectrum of crocin, obtained experimentally (Figure SI 1) is rather complex, with two weak, high energy bands at 260 and 320 nm and an intense, dissymmetrical and structured band at 441 nm. The simulated spectrum of Me
2-crocetin, unconstrained and initialized with the all-trans conformer, is shown in
Figure 10 (a), calculated with the pSDD basis, the fwhm value 0.50 eV and 60 000 MC steps. This spectrum displays some of the features observed for crocin: the weak bands at 260 and 320 nm, and an intense band at 448 nm. However, this intense band is symmetrical and displays no structure.
Figure 10 (b) shows the same spectrum, calculated with the larger pSDD+ basis, but this only produces a slight redshift. This raises the question, whether the discrepancies between measurement and simulation are due to a defective simulation of Me
2-crocetin, or to our modeling of crocin by Me
2-crocetin.
The answer to this question is given by the conformation analysis: in fact, the isomerization free energies of Table SI 3: 0.07, 0.08 and 0.11 eV, are rather large, but the DFT calculations and harmonic analysis makes them rather inaccurate. Actually, these free energies only suggest that the interference of bent conformers cannot be excluded. Therefore, we have performed
constrained 20 000 steps MC simulations of all the bent conformers of Me
2-crocetin, with only atom multi-stretch moves and no dihedral angle fluctuation. Typical structures of the most stable four conformers of Me
2-crocetin according to Table SI 3, namely the
all-trans one and the (2,3), (6,7) and (8,8’) bent ones, are shown in Figure SI 11.
Figure 11 (a) presents their spectra. It can be seen that: (i) the weak band at 250 nm can be attributed to the
all-trans and (2,3) bent conformers, (ii) the weak band at 320 nm to the bent (6,7) and (8,8’) conformers, (iii) the
all-trans, (2,3) bent and (6,7) bent conformers have very close maxima: 438, 444 and 440 nm respectively, but the bent (8,8’) conformer at 451 nm undergoes a 13 nm red shift compared to the
all-trans one. The conformers spectral features of Me
2-crocetin (
Figure 11 (a)) provide a plausible interpretation of the shape of the experimental spectrum of crocin in
Figure 11 (b). In particular, the striking shoulder on the red wing of the spectrum is assigned to the (8,8’) conformation.
Note that the lengthy simulated,
unconstraint spectrum of
Figure 10 (a), with λ
max = 448 nm is close to the constraint,
all-trans spectrum of
Figure 11 (a) with λ
max = 438 nm. This unconstraint simulation has been initialized with the
all-trans conformer indeed, and keeps it all the time. According to the large free energies of Table SI 3, this is quite normal. Therefore, the present unconstrained simulation, even if extended, cannot yield the structure of the observed spectrum. The right Monte-Carlo treatment of these conformation issues would be the
parallel tempering Monte-Carlo method [
14], with several parallel, coupled MC simulations at different temperatures. However, the analysis of
Section 4.3 shows that parallel tempering is not necessary, and that ordinary, unconstraint MC simulations of the main conformers provide a realistic investigation of the absorption spectra.
We conclude that Me
2-crocetin is an adequate model of crocin. The present results for Me
2-crocetin, including the interference of
cis-trans conformers, emphasizes the predominant influence of the polyene chain on the optical spectrum. Significantly, they may explain not only the spectrum of crocin, but also the spectrum shape of β-caroten and of numerous carotenoids, mainly the same intense and dissymmetrical band [
44].
5.2. Absorption spectra of Me2-crocetin radicals
The spectra of all the possible oxidation products of Me
2-crocetin were then simulated. Since the reaction barriers of
Figure 9 show that the methyl groups are easily oxidable, the spectra of the R
•C
a and R
•C
b species are given with more details. In
Figure 10 the focus is made on the intense bands with
fwhm = 0.50 eV and the small
pSDD (a) and large
pSDD+ (b) bases, and in
Figure 12 we focus on the weak bands only, at higher (a) and lower (b) energies with the large basis only. We label ‘½ ½’ the half-sum of the spectra of R
•C
a and R
•C
b species, assuming equal oxidation probabilities and ‘5/6 1/6’ another combination of the spectra assuming that R
•C
a is predominant, these numbers will be explained. The spectra of the R
•C
2, R
•C
3, R
•C
4, R
•C
6 and R
•C
7 species are given in Figure SI 12, together with that of the cation.
We now compare Figures 3 (a) and (b) of the experimental spectrum and
Figure 10 and
Figure 12 of the simulated ones, respectively.
Figure 3 (a) shows that the oxidation product has an intense absorption band very similar to that of crocin, with a slight decrease of intensity.
Figure 10 (a) shows that the two possible products, R
•C
a and R
•C
b, have an intense band with very different maxima at 467 nm and 415 nm, respectively. From the large blue shift of 33 nm (0.20 eV) and the large absorption intensity decrease obtained for R
•C
b alone, it appears that this radical is not predominant in contrast with R
•C
a, yielding a slight decrease of intensity and a 20 nm redshift (0.10 eV). If R
•C
a and R
•C
b were equally formed (‘½ ½’ hypothesis), they would yield a larger decrease of intensity and a tiny 5 nm blue shift. Using the larger basis does not change this situation (
Figure 10 (b)).
Figure 12 (a) (to be compared with
Figure 3 (b)) shows that the weak, high energy band observed at 330 nm must be attributed to R
•C
a only. The simulated band (in red) lies at 343 nm (error: 13 nm, 0.1 eV).
Figure 12 (b) shows that the observed weak, low energy absorption band must be also attributed to R
•C
a only. Note that the observed maximum lies at 678 nm and that the simulated values are 646 nm with the small basis (not shown, error: 0.1 eV) and 654 nm with the larger basis (error: 0.05 eV). Figures 12 (b) also shows that the little bump at 620 nm, which is present in the measured spectrum, may be attributed to R
•C
b alone. The simulated band lies at 592 nm (error: 0.10 eV). This bump appears to be the only direct interference of R
•C
b in the spectrum. In brief,
Figure 10 and
Figure 12 suggest that R
•C
a is predominant, and R
•C
b observable but rare, in contradiction with thermochemistry which rather implies equal probabilities of the two radicals and the ½ ½ spectra of
Figure 10 and
Figure 12. The predominant formation of R
•C
a now requests supplementary arguments.
We first note that the real crocin molecule offers to the OH• radical a polyene chain and two bulky sugar substituents of comparable sizes. The probability that OH• first meets the polyene chain amounts to ≈ 1/3 only. Therefore, and according to thermochemistry, the oxidation probabilities of R•Ca and R•Cb are the same: ½ x 1/3 = 1/6.
We then consider that, arriving on a sugar substituent, the OH
• radical might undergo an electrostatic attraction by the sugar. Actually, the partial charges of the oxygen atoms of the gentiobiose unit (between - 0.9 and - 1.1 a. u.) are higher than the partial charge of oxygen in the water molecules (- 0.7 a. u.), and the charge of the H atom of the OH
• radical (+ 0.4 a. u.) is higher than that in the water molecule (+ 0.34) (Figure SI 13). However, note also that due to thermodynamical barriers and despite this electrostatic attraction, the OH
• radical cannot oxidize the sugar moieties and will rather migrate from site to site on their surface. This favors the encounter and oxidation of the neighbor -C
aH
3, rather than -C
bH
3 (
Figure 13). The
sugar-driven probabilities of R
•C
a formation becomes: 2/3 + 1/6 = 5/6 and of R
•C
b: 0 + 1/6 = 1/6. The corresponding spectra are labelled ‘5/6 1/6’ in
Figure 10 and
Figure 12.
According to this discussion, the formation probabilities of the R
•C
a and R
•C
b products should lie between the extreme cases: (1/2 1/2) (no interference of the sugar substituents) and (5/6, 1/6) (sugar driven oxidation of -C
aH
3). Obviously, this probability 5/6 has been roughly estimated and simply says that the R
•C
a product is predominant.
Figure 10 and
Figure 12 suggest that this is the case. Note also that the cation, with its spectrum on Figure SI 12, is clearly not observed.
5.3. Absorption spectra of covalent dimers.
The R
•C
a and R
•C
b species may undergo covalent dimerization, through singlet pairing of their two unpaired electrons. In
Figure 5 (b) the dimer displays an intense band, with a slight redshift and an absorbance enhancement, with respect to crocin, and also a weaker band at 320 nm, with a ~ 50 % absorbance enhancement with respect to the weak band of crocin at 250 nm. However, the corresponding dimers are too large for the present method of molecular simulation. We could perform simplified simulations, nevertheless, with dimers made of
frozen monomers, taken in the optimized structures of the dimers, shown in Figure SI 14. This yields the spectra of
Figure 14, where the spectrum of
frozen Me
2-crocetin, namely of its structure at 0 K, is added for comparison.
In
Figure 14 we also extended to the dimers our two hypotheses about the R
•C
a and R
•C
b monomers: if the monomers have the probabilities (½ ½), then the dimers must have the probabilities (1/2)
2 = 0.25 for C
aC
a, 2 x (1/2)
2 = 0.5 for C
aC
b and 0.25 for C
bC
b; if the monomers have the probabilities (5/6 1/6), then the dimers must have the probabilities (5/6)
2 = 0.69 for C
aC
a, 2 x (5/6) x (1/6) = 0.28 for C
aC
b and (1/6)
2 = 0.03 for C
bC
b.
Figure 14 (a) shows that dimerization modifies the intense band of Me
2-crocetin, with a little redshift and an intensity enhancement, in agreement with the measurement of
Figure 5 (b).
Figure 14 (b) shows that the observed band at 330 nm is reproduced by the calculations. The ratio between the intensity of this band and that of the band at 250 nm of Me
2-crocetin amounts to ≈ 2.6 for the (1/2 1/2) combination of the monomers, to ≈ 1 for their (5/6 1/6) combination, to be compared to the 1.5 factor of
Figure 5 (b). This suggests that the predominance of the R
•C
a product, as concluded from the results at shorter times, is still observed in the spectra of their dimers, and that the 5/6 probability of this product is probably overestimated. Actually, the spectra of the dimers would deserve more rigorous simulations.
5.4. Absorption spectra of products of radical’s disproportionation
In γ-radiolysis (at weak dose rate), the final products (
Figure 6 (b)) have a spectrum much different from that of radical dimers. One significant difference in γ radiolysis, compared to pulse radiolysis, is the low concentration of radicals and the formation of van der Waals complexes, (crocin, crocin (- H))
• between radicals and non-oxidized crocin (reactions 7, 8).
Investigation of such complexes is at the limit of our present methods, because of the size of the systems involved. We first considered the complexes (Me
2-crocetin, Me
2-crocetin(-H))
•. The optimized structures of the complexes of the R
•C
a and R
•C
b radicals are shown in Figure SI 15. The complexes display a
parallel arrangement of the polyene chains, thus achieving a mutual solvation of these hydrophobic moieties. The formation free energies of these complexes are very negative (- 0.5 eV) (
Table 2). This means that if such a complex forms, then it does not separate. Unfortunately, these structures are disappointing because the encounter of two such complexes can provoke either disproportionation, if the H transfer occurs, or dimerization as well, if one radical center, C
aH
2 or C
bH
2, of one of the complexes, comes close to the radical center of the other complex. However, this possibility of dimerization should be reduced by bulky substituents. To this aim we introduced glucose moieties and optimized a few structures of the (Glu
2-crocetin, Glu
2-crocetin(-H))
• complexes. At this stage, we do not claim to a general view of such complexes. One typical structure involving the R
•C
a radical is shown in Figure SI 15. Note that this structure is ruled by parallel polyen chains, like in the Me
2-crocetin complex, and also by hydrogen bonds between neighbor glucose moieties.
If now two such complexes encounter, it seems clear that a parallel arrangement is hindered by the substituents, and that crossed structures, with a X shape or a T shape, will be rather favored. Then the dimerization vs disproportionation alternative occurs if in the resulting dimer of complexes, both radicals are in contact inside the structure. If these radicals are both of the predominant R•Ca type, then the crossed shape will forbid dimerization, and allow H atom transfer and disproportionation. If one of these radicals is of the rare R•Cb type, dimerization cannot be excluded but will be rare as well.
It can be seen in
Table 2 that disproportionation involves two steps: first transfer of one H atom from one radical to the other one, yielding a
primary, twice oxidized species, then cyclization of this species. In the following we note Me
2-crocetin(-2H) C
xC
y the product of disproportionation, where the C
x and C
y carbon atoms have been oxidized. It can be seen also that in most cases the primary species is a closed shell molecule with alternate single and double CC bonds between two =CH
2 groups. This is the case for the Me
2-crocetin(-2H) C
aC
a’, C
aC
b’ or C
bC
b’ species, see Figure SI 16. This is due to an odd number of bonds between the two oxidized carbon atoms (
Figure 1).
Table 2 shows that the formation free energies of these species amount to about - 0.3 eV. In one case only, Me
2-crocetin(-2H)C
a•C
b•, the primary species is not a closed shell molecule, because of an even number (6) of CC bonds. This species is a diradical, made of two -CH
2• groups, for which the triplet state can be calculated by DFT, but the singlet state cannot. In
Table 2 we consider that in this case the triplet state is more stable than the singlet, thus suggesting that the formation free energy of this singlet species is positive, and the species inaccessible. In any case both -CH
2 groups can come close to each other and fuse as a -CH
2-CH
2- bond, leaving a cyclic, closed shell molecule (Figure SI 16). Note that cyclisation is also possible for the
unexpected Me
2-crocetin(-2H) C
aC
b system. It is clear that the
primary twice oxidized radicals are transients and cannot be observed in γ radiolysis.
In
Figure 15 the absorption spectra of the four possible cyclic products are shown: Me
2-crocetin(-2H) C
aC
a’, C
aC
b, C
aC
b’, and C
bC
b’, and of three of their possible combinations. The spectra of the three accessible transients, primary products are also shown in Figure SI 17.
The mechanism of the crocin oxidation by γ-radiolysis may be derived from the best fitting between the experimental absorption spectrum of the product in
Figure 6 (b), and the simulated ones of Figures 15 and SI 17.
Figure 15 (a) shows that, in contrast with
Figure 6 (b), the cyclic C
aC
b (or the symmetric C
a’C
b’) molecule has an intense absorption spectrum similar to that of Me
2-crocetin (with a 15 nm blue shift). The three other
accessible cyclic products: C
aC
b’, C
aC
a’ and C
bC
b’ have rather close spectra very different from that of Me
2-crocetin, and with only weak bands in the 400-450 nm zone. If we consider the 1/3 1/3 1/6 1/6 combination, assuming that the R
•C
a and R
•C
b species have the same probability, and that the C
aC
b cyclic is also present, this spectrum would have still an intense band at 425 nm, which is clearly not observed. The 0 1/2 1/4 1/4 combination makes the same assumption on the R
•C
a and R
•C
b species, but discards the C
aC
b cycle. This spectrum, with a weak band at 321 nm and a still weaker one at 407 nm is in fair agreement with the observed spectrum. The 0 1/2 5/12 1/12 combination also discards the C
aC
b cycle and reflects the probabilities 5/6 and 1/6 for R
•C
a and R
•C
b. Actually, the corresponding spectrum, with a weak band at 323 nm and a still weaker band at 414 nm, is also very close to the observed one, because the spectra of the involved cyclic products are themselves close to each other.
Figure 6 shows that after γ radiolysis the absorbance of the sample is drastically reduced, up to ≈ 1/9 of that of crocin at 441 nm.
Figure 15 (b) shows that the simulations well reproduce this fact, with the same factor 1/9. Figure SI 17 presents the spectra of the
transient primary species and their 0 1/2 1/4 1/4 combination. It can be seen that all the spectra are different from those of the final cyclic molecules, and that their combined spectrum is clearly not observed.
In brief, this section provides the interpretation of the observed spectrum after γ radiolysis (weak dose rate). The Me2-crocetin(-2H) CaCb product is not observed. The three accessible cyclic products are observed through their superposition, with a weak band at ≈ 320 nm, to be compared with the observed one at ≈ 330 nm, and a weaker low energy band at ≈ 410 nm to be compared with the observed one at 430 nm. The drastic absorption coefficient collapse after γ-radiolysis is well reproduced, but the spectra cannot help discriminate the assumptions about the probabilities of the R•Ca and R•Cb species.
The critical point is that the R•Ca species is predominant and has a radical center close to a bulky substituent. This prevents from the close approach of two reactive -CaH2 groups to each other, and thus from a covalent dimerization. Note that this is true only if (crocin, crocin (-H)• radical) complexes predominantly exist, with high steric requirements. In pulse radiolysis, such complexes do not exist, the approach of the radicals is ruled by chance and the sugars may step aside and give way to dimerization.