Chemistry Reference
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Fig. 5.5 (a) Polarized
reflectivity spectra in
[Ni(chxn) 2 Br]Br 2 before and
at the delay time t d after the
photoexcitation at room
temperature. The excitation
energy is 1.55 eV and the
excitation density x ph is 0.5
photon/Ni site. Polarizations
of both the pump and probe
lights are parallel to the chain
axis b .(b) Optical
conductivity
s
(
o
) spectra
obtained by the
Kramers-Kronig analyses of
the reflectivity data in (a)
excitation of x ph <
0.012, a midgap absorption is observed at 0.4-0.5 eV in the
s
spectrum as depicted in Fig. 5.6 . With increase of x ph , the low-energy part of
s
below 0.2 eV remarkably grows, and for x ph >
0.1, the optical gap seems to
disappear.
To investigate the time evolution of the photoinduced I-M transition (Mott
transition), it is useful to examine the transfer of the spectral weight from the CT-
gap region to the inner-gap one. The spectral weight can be quantitatively analyzed
in terms of the effective number of electrons N eff (
o
) defined as follows [ 50 , 54 ].
Z o
2 m 0
pe 2 N
sðo 0 Þ
4
do 0
N eff ðoÞ¼
(5.1)
p
0
Here, m 0 is the free electron mass and N the number of Ni atoms per unit volume.
N eff (
.
Since the lower energy bound of the measured photoinduced signals is 0.12 eV, the
photoinduced change in N eff (
o
) is the measure for the kinetic energy of electrons on an energy scale of
ho
D N eff ) was calculated by using
s
from 0.12 eV to
ho
.
The results for various x ph at t d ¼
D N eff (
o
0.1 ps are presented in Fig. 5.7 .
)
ho
monotonically increases with
up to 1 eV, reflecting the accumulation of the
spectral weight below 1 eV. Then, it abruptly drops almost to zero at 1.3 eV due to
the bleaching around the CT band, signaling that the spectral weight of the CT-gap
transition is transferred to the inner-gap region by the photocarrier doping. The
values of
D N eff above 1.5 eV for x ph ¼
0.12 and x ph ¼
0.5 are negative as seen in
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