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Journal of Luminescence 107 (2004) - Department of Physics ...

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ARTICLE IN PRESS<br />

M. Drobizhev et al. / <strong>Journal</strong> <strong>of</strong> <strong>Luminescence</strong> <strong>107</strong> (<strong>2004</strong>) 194–202 201<br />

Phase shift, ∆ϕ (rad) Modulation amplitude, M<br />

0.2<br />

0.1<br />

(a)<br />

4<br />

3<br />

2<br />

1<br />

20 40 60 80 100 120<br />

Modulation amplitude, M<br />

(a)<br />

Phase shift, ∆ϕ (rad)<br />

0.2<br />

0.1<br />

2<br />

1.5<br />

1<br />

0.5<br />

20 40 60 80 100 120<br />

(b)<br />

20 40 60 80 100 120<br />

T, K<br />

Fig. 8. Temperature dependence <strong>of</strong> the amplitude M (a) and<br />

phase shift Dj (b) <strong>of</strong> spectral grating observed in SiNc:PVB and<br />

corresponding fits <strong>of</strong> these data to Eq. (8) and (16) in nonmirror-symmetrical<br />

model.<br />

phonon frequency n m ¼ 39 cm 1 seems to be<br />

overestimated.<br />

Our next attempt was to simulate the data with<br />

asymmetrical model with four independent parameters<br />

(Figs. 8a and b). One-photon parameters<br />

were fixed to the values, known from hole-burning<br />

spectroscopy: a 1 ð0Þ ¼0:9andn 1 ¼ 17 cm 1 , and x 2<br />

and n 2 were varied. The best fitting values obtained<br />

for these parameters are x 2 ¼ 1:0(a 2 ð0Þ ¼0:37) and<br />

n 2 ¼ 56 cm 1 . It is obvious that this fit fails again<br />

in describing the phase shift <strong>of</strong> Fig. 8b.<br />

We could obtain a reasonablygood fit (Figs. 9a<br />

and b) onlyif we artificiallyset a 2 ðTÞ ¼0ðx 2 ¼<br />

10 000Þ and let other three parameters vary<br />

independently. This implies no ZPL in TPA<br />

spectrum even at the lowest temperature. For the<br />

emission spectrum we obtain reasonable x 1 ¼ 0:46<br />

and n 1 ¼ 27 cm 1 , while the Debye–Waller factor<br />

again occurs smaller than measured in Ref. [14]<br />

(0.63 vs 1.0). Note that the homogeneous TPA<br />

spectrum turns out to be stronglyasymmetric with<br />

(b)<br />

20 40 60 80 100 120<br />

T, K<br />

Fig. 9. Temperature dependence <strong>of</strong> the amplitude M (a) and<br />

phase shift Dj (b) <strong>of</strong> spectral grating observed in SiNc:PVB and<br />

corresponding fits <strong>of</strong> these data to Eq. (8) and (16) in nonmirror-symmetrical<br />

model, where the Debye–Waller factor for<br />

TPA (a 2 ) was set to zero.<br />

respect to homogeneous one-photon emission<br />

spectrum. Not onlydoes this absorption contain<br />

no ZPL (a 2 ð0Þ ¼0), but its PW is shifted byonly<br />

n 2 ¼ 10 cm 1 from the zero-phonon origin.<br />

Several important conclusions can be drawn<br />

from these observations. First <strong>of</strong> all, mirrorsymmetric<br />

spectral model works well for Chl. This<br />

is not verysurprising result because this molecule<br />

does not possesses the center <strong>of</strong> inversion, and,<br />

therefore, selection rules for one- and two-photon<br />

transitions should be the same. On the other hand,<br />

TPA gratings in SiNc:PVB system are best<br />

described bystronglyasymmetrical model in<br />

which ZPL <strong>of</strong> TPA is completelymissing. This<br />

fact can be explained if we consider selection rules<br />

for pure electronic transition in this centrosymmetrical<br />

molecule. Since we are dealing with<br />

gerade2ungerade; S 0 2S 1 one-photon transition,<br />

it must be stronglyforbidden for pure electronic

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