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Defects in inorganic photorefractive materials and their investigations

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<strong>Defects</strong> <strong>in</strong> <strong>in</strong>organic <strong>photorefractive</strong> <strong>materials</strong> <strong>and</strong> <strong>their</strong> <strong>in</strong>vestigations 23<br />

(BCT), with the congruently melt<strong>in</strong>g composition at x =0.23 [130]. BCT is<br />

tetragonal between 100 ◦ C <strong>and</strong> at least 50 K [131] <strong>and</strong> thus avoids the phase<br />

transition problem imped<strong>in</strong>g the use of BT. The <strong>photorefractive</strong> properties of<br />

BCT as a host material are similarly favorable as those of BT [132]. The EPR<br />

detection of defects <strong>in</strong> BCT meets with difficulties: Because of the irregular<br />

lattice positions caused by the statistical replacement of Ba 2+ (161 pm) by<br />

the much smaller Ca 2+ (134 pm), the local crystal fields at the defect sites<br />

are rather non-uniform, lead<strong>in</strong>g to superpositions of rather diverse signals.<br />

The result<strong>in</strong>g wide <strong>and</strong> odd-shaped EPR patterns are hard to evaluate with<br />

respect to the underly<strong>in</strong>g defect models. Furthermore, because of so far unknown<br />

reasons, the presence of Ca causes strong microwave losses. In spite of<br />

these difficulties, it has been possible to identify several defects <strong>in</strong> BCT:Rh<br />

by EPR [133]. Such crystals usually have sizeable background concentrations<br />

of iron. In all of the <strong>in</strong>vestigated BCT:Rh samples Fe 3+ , isolated as well as <strong>in</strong><br />

various low symmetry associations, was identified.<br />

Besides BCT:Fe [134, 135], the system BCT:Rh has so far received the<br />

most attention <strong>in</strong> <strong>photorefractive</strong> studies, because also <strong>in</strong> BCT dop<strong>in</strong>g with<br />

Rh <strong>in</strong>creases the <strong>in</strong>frared sensitivity. Initial <strong>in</strong>vestigations of BCT:Rh are described<br />

by Veenhuis et al. [136] <strong>and</strong> by Bernhardt et al. [137, 138]. Because<br />

of the similarity of BCT:Rh to BT:Rh, also the optical absorptions b<strong>and</strong>s<br />

<strong>in</strong> both cases are quite similar. Based on the EPR <strong>in</strong>formation on defects <strong>in</strong><br />

BT:Rh [139] it thus was possible to elucidate all <strong>photorefractive</strong>ly relevant<br />

light-<strong>in</strong>duced charge transfer processes <strong>in</strong> BCT:Rh qualitatively [138] as well<br />

as quantitatively [106] <strong>in</strong> the same way as described above for BT:Rh. On<br />

the basis of the determ<strong>in</strong>ed absorption cross-sections, the defect densities <strong>and</strong><br />

the charge transfer parameters, aga<strong>in</strong> the <strong>photorefractive</strong> performance of the<br />

system is predicted. Bernhardt et al. [138] discovered that rather high pump<br />

light <strong>in</strong>tensities - about hundred times higher than <strong>in</strong> BT:Rh - are necessary<br />

that the photoconductivity of the material outweighs the dark conductivity.<br />

Under this condition the space charge fields are saturated at <strong>their</strong> maxima.<br />

The authors attributed this fact to the higher relative background Fe content<br />

<strong>in</strong> BCT:Rh. Meyer et al. [106], however, could show that the Fe content <strong>in</strong> the<br />

samples is not as high as assumed by Bernhardt et al. [138]. It is proposed that<br />

the high dark conductivity of BCT might <strong>in</strong>stead be caused by shallow hole<br />

traps <strong>in</strong>duced by disorder [106]. With reduced BCT:Fe it was shown [135],<br />

us<strong>in</strong>g comb<strong>in</strong>ed EPR/optical studies, that Fe 2+ has a wide absorption b<strong>and</strong><br />

peaked at 1.9 eV.<br />

5.3 KNbO 3 (KN)<br />

Chapter 7 deals with the favorable <strong>photorefractive</strong> properties of this material<br />

<strong>in</strong> detail. In KNbO 3 , orthorhombic below ∼ 200 ◦ C, the defects Mn 2+ ,Fe 3+ ,<br />

Fe 3+ -V O ,Co 2+ ,Co 2+ -V O ,Ir 4+ ,Ti 4+ -O − could be identified with<br />

EPR [25]. An extended EPR- <strong>and</strong> comb<strong>in</strong>ed EPR/optical absorption study<br />

of KNbO 3 :Fe is <strong>in</strong>cluded <strong>in</strong> Ref. [86]. This dop<strong>in</strong>g is known to improve the

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