<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">WJCMP</journal-id><journal-title-group><journal-title>World Journal of Condensed Matter Physics</journal-title></journal-title-group><issn pub-type="epub">2160-6919</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/wjcmp.2017.73006</article-id><article-id pub-id-type="publisher-id">WJCMP-78598</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  Crystal Growth of Cu6(Ge,Si)6O18&amp;#183;6H2O and Assignment of UV-VIS Spectra in Comparison to Dehydrated Dioptase and Selected Cu(II) Oxo-Compounds Including Cuprates
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Hans</surname><given-names>Hermann Otto</given-names></name><xref ref-type="aff" rid="aff1"><sub>1</sub></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff1"><label>1</label><addr-line>Materialwissenschaftliche Kristallographie, Clausthal University of Technology, Clausthal-Zellerfeld, Germany</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>hhermann.otto@web.de</email></corresp></author-notes><pub-date pub-type="epub"><day>21</day><month>08</month><year>2017</year></pub-date><volume>07</volume><issue>03</issue><fpage>57</fpage><lpage>79</lpage><history><date date-type="received"><day>July</day>	<month>1,</month>	<year>2017</year></date><date date-type="rev-recd"><day>Accepted:</day>	<month>August</month>	<year>18,</year>	</date><date date-type="accepted"><day>August</day>	<month>21,</month>	<year>2017</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
  Low-dimensional quantum spin systems with the Cu
  <sup>2+</sup> central ion are still in the focus of experimental and theoretical research. Here is reported on growth of mm-sized single-crystals of the low-dimensional 
  S = 1/2 spin compound Cu
  <sub>6</sub>(Ge,Si)
  <sub>6</sub>O
  <sub>18</sub>
  &amp;#183;6H
  <sub>2</sub>O by a diffusion technique in aqueous solution. A route to form Si-rich crystals down to possible dioptase, the pure silicate, is discussed. Motivated by previously reported incorrect assignments of 
  UV-VIS spectra, the assignment of 
  dd excitations from such spectra of the hexahydrate and the fully dehydrated compound is proposed in comparison to dioptase and selected Cu(II) oxo-compounds using bond strength considerations. Non-doped cuprates as layer compounds show higher excitation energies than the title compound. However, when the antiferromagnetic interaction energy as 
  J
  <sub>z</sub>
  &amp;#183;ln(2) is taken into account for cuprates, a single linear relationship between the 
  Dq
  <sub>e </sub>excitation energy and equatorial Cu(II)-O bond strength is confirmed for all compounds. A linear representation is also confirmed between 
  <sup>2</sup>
  A
  <sub>1g</sub> energies and a function of axial and equatorial Cu-O bond distances if auxiliary axial bonds are used for four-coordinated compounds. The quotient 
  Dt/
  Ds
   of experimental orbital energies deviating from the general trend to smaller values indicates the existence of H
  <sub>2</sub>O respectively Cl
  <sup>&amp;minus;</sup> axial ligands in comparison to oxo-ligands, whereas larger 
  Dt/
  Dq
  <sub>e</sub> values indicate missing axial bonds. The quotient of the excitation energy 
  <sup>2</sup>
  A
  <sub>1g</sub> by 2
  &amp;#183;
  <sup>2</sup>
  E
  <sub>g</sub>
  -
  <sup>2</sup>
  B
  <sub>2g</sub> allows checking for correctness of the assignment and to distinguish between axial oxo-ligands and others like H
  <sub>2</sub>O or Cl
  <sup>&amp;minus;</sup>.
 
</p></abstract><kwd-group><kwd>Dioptase</kwd><kwd> Ge-Dioptase</kwd><kwd> Copper(II) Compounds</kwd><kwd> Cuprates</kwd><kwd> Crystal Growth</kwd><kwd> &lt;i&gt;UV-VIS&lt;/i&gt; Spectroscopy</kwd><kwd> &lt;i&gt;EPR&lt;/i&gt;</kwd><kwd> Color</kwd><kwd> d-d Excitations</kwd><kwd> Bond Strength</kwd><kwd>  Super-Exchange Interaction</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Low-dimensional quantum spin systems are of considerable theoretical and experimental interests together with some applications to which they may lead. In spite of the ability of the d<sup>9</sup> transition metal ion Cu<sup>2+</sup> to form, apart from 3D networks, chains, ladders and small clusters, copper compounds are among the most interesting phases. With equal electronegativity compared to silicon, but in contrast to its tetrahedral networks, Cu(II) mainly forms oxo-compounds with chains and networks of connected “octahedra”.</p><p>For instance, copper polygermanate, CuGeO<sub>3</sub>, has a rather simple crystal structure of “einer” single chains of GeO<sub>4</sub> tetrahedra alongside S = 1/2 spin single chains of edge-sharing CuO<sub>4+2</sub> octahedra [<xref ref-type="bibr" rid="scirp.78598-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.78598-ref2">2</xref>] . It was the unique inorganic compound showing the Spin-Peierls-transition [<xref ref-type="bibr" rid="scirp.78598-ref3">3</xref>] [<xref ref-type="bibr" rid="scirp.78598-ref4">4</xref>] . As a quasi-one-dimen- sional system, it has been the subject of an intensive experimental and theoretical work for the past years. It was a great surprise, when Otto and Meibohm [<xref ref-type="bibr" rid="scirp.78598-ref5">5</xref>] [<xref ref-type="bibr" rid="scirp.78598-ref6">6</xref>] succeeded in the synthesis of pure copper polysilicate, CuSiO<sub>3</sub>, by thermal decomposition of the mineral dioptase, Cu<sub>6</sub>Si<sub>6</sub>O<sub>18</sub>・6H<sub>2</sub>O. CuSiO<sub>3</sub> represents the example of a fully stretched silicate chain structure. It is isotypic to CuGeO<sub>3</sub>, but does not show the spin-Peierls transition, instead an antiferromagnetic ordering below T<sub>N</sub> = 7.9 K [<xref ref-type="bibr" rid="scirp.78598-ref7">7</xref>] [<xref ref-type="bibr" rid="scirp.78598-ref8">8</xref>] .</p><p>The rhombohedral title compound Cu<sub>6</sub>(Ge,Si)<sub>6</sub>O<sub>18</sub>・6H<sub>2</sub>O represents a hexacyclo-germanate (silicate) that contains copper-oxygen spiral chains along the c-axis, which are connected (intra-chain) by edge-sharing dimers (<xref ref-type="fig" rid="fig1">Figure 1</xref>).</p><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> Crystal structure of dioptase projected down [<xref ref-type="bibr" rid="scirp.78598-ref001">001</xref>]. A framework of copper oxide octahedra (yellow) screws around the c-axis with non-bonding axial water ligands (red) pointing towards empty channels. Six-membered silicate single rings are depicted in green</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-4800411x2.png"/></fig><p>This structure is interesting because it allows for a quantum phase transition between an anti-ferromagnetically ordered state and a quantum spin liquid [<xref ref-type="bibr" rid="scirp.78598-ref9">9</xref>] . Large quantum fluctuations in green dioptase have been described [<xref ref-type="bibr" rid="scirp.78598-ref10">10</xref>] . Recently, also the germanate analogue, Cu<sub>6</sub>Ge<sub>6</sub>O<sub>18</sub>・6H<sub>2</sub>O [<xref ref-type="bibr" rid="scirp.78598-ref11">11</xref>] , has been the object of detailed magnetic and structural investigations [<xref ref-type="bibr" rid="scirp.78598-ref12">12</xref>] [<xref ref-type="bibr" rid="scirp.78598-ref13">13</xref>] .</p><p>If near the empty structural channels located water molecules are removed, a screwed framework of edge-sharing disphenoids rather than flat CuO<sub>4</sub> plaquettes remains in the dehydrated compound.</p><p>As part of a systematic study of transition metal germanates, silicates and arsenates we have undertaken syntheses of rare copper minerals and new copper compounds in view of its power as low dimensional S = 1/2 spin compounds allowing for interesting physical and physicochemical properties. First, the synthesis serves not to waste rare mineral specimens for research. There is also the possibility to study an improvement in the crystal growth by replacement of copper by other elements, apart from the chance of doping with electronically or magnetically interesting ones. For example, the replacement of copper by manganese was observed in natural samples of dioptase by EPR measurements [<xref ref-type="bibr" rid="scirp.78598-ref14">14</xref>] [<xref ref-type="bibr" rid="scirp.78598-ref15">15</xref>] .</p><p>Because the assignment of the dd excitations derived from the UV-VIS spectra of copper-bearing compounds are often found to be incorrect, this work contributed some simple tools that could lead to the right assignment. It is not the intent of this paper to review UV-VIS spectroscopy of Cu<sup>2+</sup> compounds in general.</p></sec><sec id="s2"><title>2. Experimental</title><sec id="s2_1"><title>2.1. Crystal Growth and Dehydration of the Samples</title><p>The method described below was used by the author many years earlier for the synthesis of rare minerals, for instance, the synthesis of Pb<sub>3</sub>Ge(OH)<sub>6</sub>(SO<sub>4</sub>)<sub>2</sub>・3H<sub>2</sub>O, the piezoelectric Tsumeb mineral fleischerite [<xref ref-type="bibr" rid="scirp.78598-ref16">16</xref>] . For the synthesis of the title compound freshly precipitated gels of GeO<sub>2</sub> and Cu(OH)<sub>2</sub> were separately filled in 200 ml beaker glasses and thoroughly filled up with distilled water. Then a U-shaped glass pipe of 6 mm inner diameter, well annealed before use to reduce crystal nucleation frequency, was filled free of air bubbles with distilled water. This pipe is then used to connect the distinct solutions in the beakers. Finally, the water surface in the beakers is covered with a film of liquid paraffin to prevent water evaporation and entry of CO<sub>2</sub>, respectively.</p><p>The desired slow diffusion of the distinct solutions into one another leads to the formation of Cu<sub>6</sub>(Ge,Si)<sub>6</sub>O<sub>18</sub>・6H<sub>2</sub>O seeds that grow up to 1 mm size of light blue crystals within 8 weeks. Interestingly, most individual crystals form double- crystals. The symmetry situation of this finding must be investigated further. The crystals of stocky prismatic, nearly spherical habit developed {110} and {021} forms (<xref ref-type="fig" rid="fig2">Figure 2</xref>).</p><p>One can extrapolate the time scale to get a crystal of about 2 mm diameter and calculate about 1 year of growing time. Trying to exchange Ge by Si by this method</p><fig id="fig2"  position="float"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> The stocky prismatic habit of the as-grown Cu<sub>6</sub>(Ge,Si)<sub>6</sub>O<sub>18</sub>・6H<sub>2</sub>O crystals, showing a combination of the {110} prism and the {021} rhombohedron</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-4800411x3.png"/></fig><p>seems to be less efficient, only a slightly greenish sheen shows that a small exchange occurred.</p><p>The other method of co-precipitation of GeO<sub>2</sub>, SiO<sub>2</sub> and Cu(OH)<sub>2</sub> gel and longer time vigorous stirring resulted in a vivid green colored polycrystalline material of about 12 at-% Si determined from lattice parameter changes [<xref ref-type="bibr" rid="scirp.78598-ref14">14</xref>] [<xref ref-type="bibr" rid="scirp.78598-ref17">17</xref>] . Also, the substitution of some B<sup>3+</sup> for Ge<sup>4+</sup> is possible, leading to a beautiful green color [<xref ref-type="bibr" rid="scirp.78598-ref17">17</xref>] . Stirring a longer period and in addition changing the pH to more acidic milieu gives at least about 15 at-% Si (a = 14.640 &#197;, c = 7.806 &#197;, this work). The effect is based on the different solubility of the Ge-compound in comparison to dioptase. Cu<sub>6</sub>Ge<sub>6</sub>O<sub>18</sub>・6H<sub>2</sub>O is easily decomposed by a dilute acetic acid, but dioptase does not dissolve. Recently we observed a deepening of color to dioptase green, when the Si-rich solution was exposed to ultrasonic waves, in this way superseding vigorous stirring. The energy that is released when voids implodes (super-cavitation) may be able to assemble more easily and faster the six-membered silicate rings within the cuprate framework of dioptase.</p><p>A proposed approach for a possible synthesis of pure polycrystalline dioptase results as follows. The first step will be the spontaneous formation of pure germanate and exchange of maximum Ge by Si through stirring or sonochemical treatment. Then pH, as well as temperature, is altered to increase the solubility of the still Ge-rich compound combined with a simultaneous offer of more Si to form a dioptase layer. A new core of silico-germanate can be grown epitaxially and subsequently transformed to dioptase. Repetition of this process may finally form pure dioptase in mm-sized crystals. An automated process would make sense. Nature has similar tools in the quiver such as rhythmic property changes (concentration, pH, temperature) of metal bearing ascending or descending solutions, apart from a lot of time.</p><p>A single-phase crystalline powder of synthetic Ge-dioptase for the UV-VIS spectroscopic investigation is best obtained from an aqueous solution of pH 5.5 at room temperature, formed by mixing and stirring equal amounts of 0.02 M cupric acetate with freshly produced 0.02 M GeO<sub>2</sub> solution. The initially formed gel settles as fully crystalline precipitate after an induction period of two days [<xref ref-type="bibr" rid="scirp.78598-ref10">10</xref>] .</p><p>Complete dehydration of synthetic Ge-dioptase was performed by annealing of the polycrystalline sample up to 920 K for 6 h, followed by cooling down to room temperature with a moderate cooling rate of 20 K/h. The chosen annealing temperature lies about 53 K below the temperature of decomposition to the orthorhombic spin-Peierls phase CuGeO<sub>3</sub> [<xref ref-type="bibr" rid="scirp.78598-ref10">10</xref>] .</p><p>A natural dioptase samples from the locality Altyn Tyube, Kazakhstan, was used as pure silicate sample. Its complete dehydration to “black” dioptase occurs at 660 K and should be controlled by X-ray powder diffraction analysis because decomposition into CuO (tenorite) and SiO<sub>2</sub> (partly quartz and cristobalite) starts only a few degrees higher at 673 K.</p></sec><sec id="s2_2"><title>2.2. UV-VIS Spectroscopic Investigation</title><p>First results of UV-VIS spectroscopy on Cu<sub>6</sub>(Ge,Si)<sub>6</sub>O<sub>18</sub>・6H<sub>2</sub>O are given in the doctoral theses of my coworkers Brandt [<xref ref-type="bibr" rid="scirp.78598-ref17">17</xref>] and Meibohm [<xref ref-type="bibr" rid="scirp.78598-ref14">14</xref>] , respectively, whereas dioptase itself has been investigated earlier by different researchers [<xref ref-type="bibr" rid="scirp.78598-ref18">18</xref>] [<xref ref-type="bibr" rid="scirp.78598-ref19">19</xref>] [<xref ref-type="bibr" rid="scirp.78598-ref20">20</xref>] [<xref ref-type="bibr" rid="scirp.78598-ref21">21</xref>] .</p><p>Brandt [<xref ref-type="bibr" rid="scirp.78598-ref17">17</xref>] reported a color change from turquoise-green to blue on dehydration of dioptase-type copper germanate. In addition, the dehydrated compound showed thermochromic behavior on heating up to 500˚C with a reversible color change to vivid green similar to that of annealed CuGeO<sub>3</sub>. The color persists when Cu<sub>6</sub>Ge<sub>6</sub>O<sub>18</sub> is rapidly cooled down to room temperature. A possible interpretation for this effect is according to [<xref ref-type="bibr" rid="scirp.78598-ref17">17</xref>] the low relaxation rate of the four oxygen ligands around copper. Remember that the equatorial coordination in dioptase is not planar but disphenoidic, and a change to a stiffer, more tetrahedral one may occur with raising the temperature.</p><p>A reinvestigation of the fully hydrated and dehydrated compounds is primarily undertaken in order to deconvolute and understand the broad UV-VIS spectrum of the synthetic color pigment litidionite, KNaCuSi<sub>4</sub>O<sub>10</sub> [<xref ref-type="bibr" rid="scirp.78598-ref22">22</xref>] [<xref ref-type="bibr" rid="scirp.78598-ref23">23</xref>] , which shows similarity to that of dioptase.</p><p>The room temperature UV-VIS spectra of the samples were taken with the double-beam light scanning UV-2501PC CE spectrometer from Shimazu with selectable light sources (50W halogen lamp and D2 lamp). The powder sample was coated on a polished aluminum disk and measured in the reflection modus against a BaSO<sub>4</sub> standard in the wavelength range between 190 and 900 nm with a spectral bandwidth of 0.1 nm using a 50 nm/min scan and choosing 0.5 nm intervals. From the less structured absorbance profile, recalculated from the measured reflectance, the energy bands were fitted with Gaussian profile functions. The better resolved spectra of the dehydrated compounds were fitted first and then the results used as start parameters for the broad spectra of the hydrated compounds.</p></sec><sec id="s2_3"><title>2.3. EPR Data</title><p>Electron paramagnetic resonance spectroscopy (EPR) provides information about the electronic structure of transition metal ion complexes. For d<sup>1,9</sup> systems such as Cu<sup>2+</sup> centered complexes with no fine structure the principal values of the g-tensor of the spin Hamiltonian H = β<sub>e</sub>B・g・S, reflecting the symmetry of the ligand field, can be derived from the EPR spectrum, where B is the external magnetic field, S is the spin vector, and β<sub>e</sub> = g<sub>e</sub>・μ<sub>B</sub> (Land&#233; g-factor for the free electron, g<sub>e</sub> = 2.0023, Bohr magneton μ<sub>B</sub>). In this contribution g values for dioptase, Cu<sub>6</sub>Si<sub>6</sub>O<sub>18</sub>・6H<sub>2</sub>O, determined by Reddy et al. [<xref ref-type="bibr" rid="scirp.78598-ref19">19</xref>] , and data measured by Meibohm [<xref ref-type="bibr" rid="scirp.78598-ref14">14</xref>] for synthetic Cu<sub>6</sub>Ge<sub>6</sub>O<sub>18</sub>・6H<sub>2</sub>O were used as expressed in its principal axes system.</p></sec></sec><sec id="s3"><title>3. Results and Discussion</title><p>The Gaussian peak analysis of the UV-VIS spectra was performed with the aid of own Turbo-Basic programs using recast software modules once developed for X-ray powder profile analysis, supplemented by a program to provide an illustration of single Gaussian peaks besides the cumulative curve. Fortunately, the spectra of the dehydrated compounds are well-resolved and their reliably fitted profile data could serve as input for the less-resolved spectra of the as-grown respectively hydrated natural compounds, thereby applying variable constraints to parameters (mainly the band width) during successive refinement cycles. Results of a Gaussian deconvolution of the UV-VIS spectra for the hydrated and dehydrated compounds, respectively, are given in <xref ref-type="table" rid="table1">Table 1</xref> and depicted in Figures 3(a)-(d). λ(nm) and Γ(nm) represent wavelength and the full width of the excitation peaks, and the wavenumber E(cm<sup>−1</sup>) denotes the excitation energy. The</p><table-wrap id="table1" ><label><xref ref-type="table" rid="table1">Table 1</xref></label><caption><title> Results of the Gaussian profile deconvolution of the UV-VIS spectra of the dioptase family</title></caption><table><tbody><thead><tr><th align="center" valign="middle"  colspan="5"  >Cu<sub>6</sub>Si<sub>6</sub>O<sub>18</sub>・6H<sub>2</sub>O (dioptase)</th><th align="center" valign="middle"  colspan="5"  >Cu<sub>6</sub>Ge<sub>6</sub>O<sub>18</sub>・6H<sub>2</sub>O (Ge-dioptase)</th></tr></thead><tr><td align="center" valign="middle" >P</td><td align="center" valign="middle" >λ(nm)</td><td align="center" valign="middle" >Γ(nm)</td><td align="center" valign="middle" >E(cm<sup>−1</sup>)</td><td align="center" valign="middle" >Assignment</td><td align="center" valign="middle" >P</td><td align="center" valign="middle" >λ(nm)</td><td align="center" valign="middle" >Γ(nm)</td><td align="center" valign="middle" >E(cm<sup>−1</sup>)</td><td align="center" valign="middle" >Assignment</td></tr><tr><td align="center" valign="middle" >329</td><td align="center" valign="middle" >935 &#177; 37</td><td align="center" valign="middle" >208</td><td align="center" valign="middle" >10,700</td><td align="center" valign="middle" >Δ<sub>A</sub></td><td align="center" valign="middle"  rowspan="2"  >1000</td><td align="center" valign="middle"  rowspan="2"  >842 &#177; 30</td><td align="center" valign="middle"  rowspan="2"  >198</td><td align="center" valign="middle"  rowspan="2"  >11,884</td><td align="center" valign="middle"  rowspan="2"  >Δ<sub>B</sub> + Δ<sub>A</sub></td></tr><tr><td align="center" valign="middle" >815</td><td align="center" valign="middle" >869 &#177; 12</td><td align="center" valign="middle" >208</td><td align="center" valign="middle" >11,507</td><td align="center" valign="middle" >Δ<sub>B</sub></td></tr><tr><td align="center" valign="middle" >1000</td><td align="center" valign="middle" >695 &#177; 7</td><td align="center" valign="middle" >194</td><td align="center" valign="middle" >14,400</td><td align="center" valign="middle" >Δ<sub>E</sub></td><td align="center" valign="middle" >645</td><td align="center" valign="middle" >698 &#177; 24</td><td align="center" valign="middle" >166</td><td align="center" valign="middle" >14,321</td><td align="center" valign="middle" >Δ<sub>E</sub></td></tr><tr><td align="center" valign="middle" >256</td><td align="center" valign="middle" >600</td><td align="center" valign="middle" >109</td><td align="center" valign="middle" >16,670</td><td align="center" valign="middle" >ZRS?<sup> </sup></td><td align="center" valign="middle" >185</td><td align="center" valign="middle" >616</td><td align="center" valign="middle" >129</td><td align="center" valign="middle" >16,230</td><td align="center" valign="middle" >ZRS?<sup> </sup></td></tr><tr><td align="center" valign="middle" >421</td><td align="center" valign="middle" >414</td><td align="center" valign="middle" >108</td><td align="center" valign="middle" >24,160</td><td align="center" valign="middle" >SPE?</td><td align="center" valign="middle" >271</td><td align="center" valign="middle" >462</td><td align="center" valign="middle" >147</td><td align="center" valign="middle" >21,650</td><td align="center" valign="middle" >SPE?</td></tr><tr><td align="center" valign="middle" >(554)</td><td align="center" valign="middle" >326</td><td align="center" valign="middle" >102</td><td align="center" valign="middle" >30,660</td><td align="center" valign="middle" >E<sub>g</sub><sub> </sub></td><td align="center" valign="middle" >(531)</td><td align="center" valign="middle" >353</td><td align="center" valign="middle" >97</td><td align="center" valign="middle" >28,350</td><td align="center" valign="middle" >E<sub>g</sub><sub> </sub></td></tr><tr><td align="center" valign="middle"  colspan="5"  >Cu<sub>6</sub>Si<sub>6</sub>O<sub>18</sub> (dioptase dehydrated)</td><td align="center" valign="middle"  colspan="5"  >Cu<sub>6</sub>Ge<sub>6</sub>O<sub>18</sub> (Ge-dioptase dehydrated)</td></tr><tr><td align="center" valign="middle" >P</td><td align="center" valign="middle" >λ(nm)</td><td align="center" valign="middle" >Γ(nm)</td><td align="center" valign="middle" >E(cm<sup>−1</sup>)</td><td align="center" valign="middle" >Assignment</td><td align="center" valign="middle" >P</td><td align="center" valign="middle" >λ (nm)</td><td align="center" valign="middle" >Γ(nm)</td><td align="center" valign="middle" >E(cm<sup>−1</sup>)</td><td align="center" valign="middle" >Assignment</td></tr><tr><td align="center" valign="middle" >1000</td><td align="center" valign="middle" >811 &#177; 14</td><td align="center" valign="middle" >158</td><td align="center" valign="middle" >12,330</td><td align="center" valign="middle" >Δ<sub>B</sub></td><td align="center" valign="middle" >1000</td><td align="center" valign="middle" >827 &#177; 14</td><td align="center" valign="middle" >155</td><td align="center" valign="middle" >12,100</td><td align="center" valign="middle" >Δ<sub>B</sub></td></tr><tr><td align="center" valign="middle" >866</td><td align="center" valign="middle" >668 &#177; 12</td><td align="center" valign="middle" >120</td><td align="center" valign="middle" >14,960</td><td align="center" valign="middle" >Δ<sub>E</sub></td><td align="center" valign="middle" >843</td><td align="center" valign="middle" >679 &#177; 12</td><td align="center" valign="middle" >127</td><td align="center" valign="middle" >14,723</td><td align="center" valign="middle" >Δ<sub>E</sub></td></tr><tr><td align="center" valign="middle" >492</td><td align="center" valign="middle" >558 &#177; 11</td><td align="center" valign="middle" >96</td><td align="center" valign="middle" >17,930</td><td align="center" valign="middle" >Δ<sub>A</sub></td><td align="center" valign="middle" >450</td><td align="center" valign="middle" >565 &#177; 12</td><td align="center" valign="middle" >97</td><td align="center" valign="middle" >17,700</td><td align="center" valign="middle" >Δ<sub>A</sub></td></tr><tr><td align="center" valign="middle" >235</td><td align="center" valign="middle" >441</td><td align="center" valign="middle" >100</td><td align="center" valign="middle" >22,680</td><td align="center" valign="middle" >SPE?</td><td align="center" valign="middle" >355</td><td align="center" valign="middle" >437</td><td align="center" valign="middle" >108</td><td align="center" valign="middle" >22,880</td><td align="center" valign="middle" >SPE?</td></tr><tr><td align="center" valign="middle" >(869)</td><td align="center" valign="middle" >330</td><td align="center" valign="middle" >120</td><td align="center" valign="middle" >30,300</td><td align="center" valign="middle" >E<sub>g</sub><sub> </sub></td><td align="center" valign="middle" >(630)</td><td align="center" valign="middle" >357</td><td align="center" valign="middle" >102</td><td align="center" valign="middle" >28,000</td><td align="center" valign="middle" >E<sub>g </sub></td></tr></tbody></table></table-wrap><p>P integrated band intensity (arbitrary units), Γ(nm) full band width at half f, E(cm<sup>−</sup><sup>1</sup>) band energy, SPE assumed simultaneous pair excitation, ZRS less intense band observed only in the hydrated compounds around 2 eV could correspond to a Zhang-Rice singlet excitation, E<sub>g</sub> large energy gap.</p><fig id="fig3"  position="float"><label><xref ref-type="fig" rid="fig3">Figure 3</xref></label><caption><title> UV-VIS spectra of (a) dioptase; (b) dioptase dehydrated; (c) Ge-dioptase; (d) Ge-dioptase dehydrated. Measured spectra red, calculated spectra blue. A mineral sample of dioptase from Altyn Tyube, Kazakhstan was used besides synthetic Ge-dioptase</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-4800411x4.png"/></fig><p>remarkable integrated band intensity P (given in arbitrary units) is the consequence of non-zero dd transition probabilities due to the absence of symmetry elements on the Cu position with C<sub>1</sub> site symmetry and the disphenoidic (stocky tetrahedral) oxygen environment with 4 distinct equatorial bond lengths indicating Cu<sub>3d</sub>-O<sub>2p</sub> hybridization. The relative width Γ/λ of the bands of the dehydrated compounds is about 18%, whereas that of the hydrated ones suffer additional broadening to about 23% caused by a vibronic contribution of the water molecule rings and due to assumed peak overlapping according to the below presented assignment.</p><p>The steep increase of absorption at the badly resolved high energy limit of the UV-VIS spectra has been simulated by a Gaussian curve, too, and may be interpreted as absorption edge, the large gap between valence and conduction band of isolator compounds. The gap is determined around 3.80 eV for dioptase and shifts to 3.76 eV for Ge-dioptase, respectively. It is slightly lower for the dehydrated compounds, giving 3.52 and 3.47 eV, respectively (<xref ref-type="table" rid="table1">Table 1</xref>). For comparison, Rudko [<xref ref-type="bibr" rid="scirp.78598-ref24">24</xref>] observed an absorption edge near 3.5 eV for the charge transfer insulator CuGeO<sub>3</sub>. The absorption structures at high energy just before the energy gap may be attributed to simultaneous ligand field transitions, involving both metal centers of the dimer at twice the monomer transition energy (SPE), because their oscillator strengths are too weak for charge transfer (CT) transitions. The position of a less intense absorption band observed only for the hydrated compounds around 2 eV (16,670 cm<sup>−1</sup>, 16,230 cm<sup>−1</sup>) would correspond to Zhang-Rice singlet excitations (ZRS), for instance, measured at this energy on CuO (tenorite) [<xref ref-type="bibr" rid="scirp.78598-ref25">25</xref>] and CuGeO<sub>3</sub>, respectively [<xref ref-type="bibr" rid="scirp.78598-ref26">26</xref>] .</p><p>The color of Cu<sup>2+</sup> compounds with their Jahn-Teller distorted coordination polyhedra [<xref ref-type="bibr" rid="scirp.78598-ref27">27</xref>] is the conspicuously recognized property of this transition metal ion and is attributed to electronic excitations between its d-orbitals. The coordination polyhedron of copper in the d<sup>9 </sup>state with the unpaired electron in the x<sup>2</sup> − y<sup>2</sup> orbital is an elongated octahedron leading to splitting of formerly degenerated d-states. A recently found impressive example for a Jahn-Teller elongated octahedron is the new prototypic crystal structure of tetragonal CuO with a c &gt; a rock salt structure [<xref ref-type="bibr" rid="scirp.78598-ref28">28</xref>] .</p><p>The transition energies ∆<sub>n</sub> (cm<sup>−1</sup>), derived from broad Gaussian-shaped absorption bands of UV-VIS spectra, are the energy differences between the</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x5.png" xlink:type="simple"/></inline-formula>ground state and the<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x6.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x7.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x8.png" xlink:type="simple"/></inline-formula> ex- cited states and can be connected with crystal field splitting parameters repre- senting orbital energies. Bearing in mind the Cu<sup>2+</sup> site symmetry of D<sub>4h</sub> or lower, we are faced with an equatorial Dq<sub>e</sub> splitting parameter and two radial Ds and Dt ones (Gerloch and Slade, [<xref ref-type="bibr" rid="scirp.78598-ref29">29</xref>] ). The crystal field theory (CFT) allows for the following relations:</p><disp-formula id="scirp.78598-formula4"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800411x9.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.78598-formula5"><label>(2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800411x10.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.78598-formula6"><label>(3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800411x11.png"  xlink:type="simple"/></disp-formula><p>Conversely, the D parameters can be recalculated as</p><disp-formula id="scirp.78598-formula7"><label>(4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800411x12.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.78598-formula8"><label>(5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800411x13.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.78598-formula9"><label>(6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800411x14.png"  xlink:type="simple"/></disp-formula><p>Whereas ∆<sub>E</sub> is always moderately larger than ∆<sub>B</sub>, ∆<sub>A</sub> ranges from about 8500 cm<sup>−1</sup> (&lt;∆<sub>B</sub>) for shortest axial bonds to at least 21,500 cm<sup>−1</sup> (&gt;∆<sub>E</sub>) for axially non- existent bonds (squared-planar coordination).</p><p>A more quantitative description of ligand field parameters using effective charges and bond lengths results in the following relations [<xref ref-type="bibr" rid="scirp.78598-ref29">29</xref>] :</p><disp-formula id="scirp.78598-formula10"><label>(7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800411x15.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.78598-formula11"><label>(8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800411x16.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.78598-formula12"><label>(9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800411x17.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.78598-formula13"><label>(10)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800411x18.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x19.png" xlink:type="simple"/></inline-formula> represents an effective ligand charge, R<sub>e</sub> and R<sub>a</sub> are equatorial and axial bond lengths in &#197;, and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x19.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x20.png" xlink:type="simple"/></inline-formula> = 0.214 &#197;<sup>4</sup> is the mean value of the fourth power of a 3d orbital radial distance from the nucleus, respectively <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x19.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x20.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x21.png" xlink:type="simple"/></inline-formula> = 0.294 &#197;<sup>2</sup> the mean of the second power of the radial distance. For <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x19.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x20.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x21.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x22.png" xlink:type="simple"/></inline-formula> the values calculated by Haverkort within the Hartree-Fock approximation are used [<xref ref-type="bibr" rid="scirp.78598-ref30">30</xref>] . Because <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x19.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x20.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x21.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x22.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x23.png" xlink:type="simple"/></inline-formula> is a measure proportional to the Cu(II) effective nuclear charge, one should multiply this value by a factor of 4 to give a realistic value of about 0.85 for the Scott charge, which would represent 42.5% ionicity of the Cu-O bond.</p><p>Quoting Gerloch and Slade [<xref ref-type="bibr" rid="scirp.78598-ref29">29</xref>] ones more, in the crystal-field theory with its point-charge formalism charges as well as bond lengths have to be considered as effective parameters that are not independent of each other. Therefore, cationic and ligand charges should be combined to common adaptable factors <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x24.png" xlink:type="simple"/></inline-formula> respectively<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x24.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x25.png" xlink:type="simple"/></inline-formula>.</p><p>For comparison of calculated band energies with experimental ones given in cm<sup>−1</sup> an energy conversion factor <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x26.png" xlink:type="simple"/></inline-formula> is applied.</p><p>Lebernegg et al. [<xref ref-type="bibr" rid="scirp.78598-ref31">31</xref>] found no general theoretical justification for R<sup>−5</sup> dependence of ligand-field splitting. Nevertheless, one can use the inverse fifth power relationship Dq<sub>e</sub> &#181; R<sup>−5</sup> in order to calculate a linear regression curve of Dq<sub>e</sub> (or D<sub>B</sub>) values against the mean of the four equatorial copper-oxygen distances R<sub>e</sub>(&#197;) according to Equation (7) for selected compounds with a reduced connectedness with respect to equatorial sharing, at the beginning excluding sheet structures as exemplified by cuprates.</p><p>The plot is depicted in <xref ref-type="fig" rid="fig4">Figure 4</xref> and extrapolates well through the origin with<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x27.png" xlink:type="simple"/></inline-formula>, giving effective charge numbers of Q<sub>e</sub> = &#177; 1.313 assumed to be evenly distributed over Cu<sup>2+</sup> and ligands. The calculated Dq<sub>e</sub> values deviate less than 1.6% from the experimental ones.</p><p>We chose compounds of the Egyptian Blue family (cuprorivaite, wesselite, effenbergite,) with isolated D<sub>4h</sub> plaquettes, the dehydrated dioptase compounds with equatorially edge-shared dimers, further connected via water oxygen to</p><fig id="fig4"  position="float"><label><xref ref-type="fig" rid="fig4">Figure 4</xref></label><caption><title> Calculated Dq energies versus experimental ones for dioptase and related compounds. In the right plot, an additional magnetic contribution of Dq<sub>calc</sub> for cuprates was considered</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-4800411x28.png"/></fig><p>corner-shared spiral chains in the fully hydrated compounds, litidionite as characterized by pyramid-edge-shared dimers (cis-arrangement), in contrast to lammerite with infinite chains of such units and with two distinct Cu sites, further azurite with “octahedral” chains (two distinct sites), and finally conichalcite and CuGeO<sub>3</sub> showing infinite single chains with equatorially edge-shared “octahedra”. One may learn more about the structural hierarchy of special copper oxy-salt minerals from Eby and Hawthorne [<xref ref-type="bibr" rid="scirp.78598-ref32">32</xref>] . Selected crystal data as well as UV-VIS data were summarized in the <xref ref-type="table" rid="table2">Table 2</xref> and <xref ref-type="table" rid="table3">Table 3</xref> with references.</p><table-wrap id="table2" ><label><xref ref-type="table" rid="table2">Table 2</xref></label><caption><title> Coordination numbers CN, bond length and bond valence sums s for selected Cu(II) compounds. s<sub>e</sub> equatorial sum, s<sub>a</sub> axial sum, Ss overall sum (particularly striking values in red)</title></caption><table><tbody><thead><tr><th align="center" valign="middle"  rowspan="2"  >Compound</th><th align="center" valign="middle"  rowspan="2"  >CN</th><th align="center" valign="middle"  rowspan="2"  >d(Cu-O) (&#197;)</th><th align="center" valign="middle"  colspan="3"  >Bond strength</th><th align="center" valign="middle"  rowspan="2"  >Reference</th></tr></thead><tr><td align="center" valign="middle" >s<sub>e </sub></td><td align="center" valign="middle" >s<sub>a </sub></td><td align="center" valign="middle" >Ss</td></tr><tr><td align="center" valign="middle" >Ca<sub>0.5</sub>Sr<sub>0.5</sub>CuO<sub>4</sub></td><td align="center" valign="middle"  rowspan="5"  >4</td><td align="center" valign="middle" >1.945</td><td align="center" valign="middle" >1.913</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >1.913</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref41">41</xref>]</td></tr><tr><td align="center" valign="middle" >CaCuO<sub>2 </sub></td><td align="center" valign="middle" >1.928</td><td align="center" valign="middle" >2.004</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >2.004</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref33">33</xref>]</td></tr><tr><td align="center" valign="middle" >BaCuSi<sub>4</sub>O<sub>10</sub> Effenbergite</td><td align="center" valign="middle" >1.925</td><td align="center" valign="middle" >2.022</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >2.022</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref42">42</xref>]</td></tr><tr><td align="center" valign="middle" >SrCuSi<sub>4</sub>O<sub>10</sub> Wesselite</td><td align="center" valign="middle" >1.925</td><td align="center" valign="middle" >2.022</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >2.022</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref43">43</xref>]</td></tr><tr><td align="center" valign="middle" >CaCuSi<sub>4</sub>O<sub>10</sub> Cuprorivaite</td><td align="center" valign="middle" >1.929</td><td align="center" valign="middle" >1.998</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >1.998</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref44">44</xref>]</td></tr><tr><td align="center" valign="middle" >Cu<sub>6</sub>Si<sub>6</sub>O<sub>18</sub></td><td align="center" valign="middle"  rowspan="2"  >4 + (1)</td><td align="center" valign="middle" >1.9250 1.9294 1.9354 1.9466 3.3153</td><td align="center" valign="middle" >1.969</td><td align="center" valign="middle" >0.023</td><td align="center" valign="middle" >1.992</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref20">20</xref>]</td></tr><tr><td align="center" valign="middle" >Cu<sub>6</sub>Ge<sub>6</sub>O<sub>18</sub></td><td align="center" valign="middle" >1.9043 1.9284 1.9380 1.9979 3.3841</td><td align="center" valign="middle" >1.954</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >1.954</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref17">17</xref>]</td></tr><tr><td align="center" valign="middle" >Y<sub>2</sub>BaCuO<sub>5</sub></td><td align="center" valign="middle" >2 + 2 + 1</td><td align="center" valign="middle" >1.985 1.988 2.206</td><td align="center" valign="middle" >1.692</td><td align="center" valign="middle" >0.232</td><td align="center" valign="middle" >1.923</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref45">45</xref>]</td></tr><tr><td align="center" valign="middle" >CuGeO<sub>3 </sub></td><td align="center" valign="middle" >4 + 2</td><td align="center" valign="middle" >1.941 2.926</td><td align="center" valign="middle" >1.941</td><td align="center" valign="middle" >0.093</td><td align="center" valign="middle" >2.022</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.78598-ref2">2</xref>] [<xref ref-type="bibr" rid="scirp.78598-ref3">3</xref>]</td></tr><tr><td align="center" valign="middle" >Cu<sub>6</sub>Si<sub>6</sub>O<sub>18</sub>・6H<sub>2</sub>O</td><td align="center" valign="middle" >6</td><td align="center" valign="middle" >1.952 1.952 1.959 1.983 2.502 2.648</td><td align="center" valign="middle" >1.818</td><td align="center" valign="middle" >0.195</td><td align="center" valign="middle" >2.014</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref46">46</xref>]</td></tr><tr><td align="center" valign="middle" >Cu<sub>6</sub>Ge<sub>5.4</sub>Si<sub>0.6</sub>O<sub>18</sub>・6H<sub>2</sub>O</td><td align="center" valign="middle" >6</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref17">17</xref>]</td></tr><tr><td align="center" valign="middle" >Cu<sub>6</sub>Ge<sub>6</sub>O<sub>18</sub>・6H<sub>2</sub>O</td><td align="center" valign="middle" >6</td><td align="center" valign="middle" >1.9037 1.9486 1.9547 1.9884 2.6364 2.6696</td><td align="center" valign="middle" >1.894</td><td align="center" valign="middle" >0.159</td><td align="center" valign="middle" >2.053</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref11">11</xref>]</td></tr><tr><td align="center" valign="middle"  rowspan="2"  >Cu<sub>3</sub>(CO<sub>3</sub>)<sub>2</sub>(OH)<sub>2</sub> Azurite</td><td align="center" valign="middle" >2 + 2 + 2 Cu(1) site</td><td align="center" valign="middle" >1.9387 1.9455 2.9840</td><td align="center" valign="middle" >1.953</td><td align="center" valign="middle" >0.083</td><td align="center" valign="middle" >2.036</td><td align="center" valign="middle"  rowspan="2"  >[<xref ref-type="bibr" rid="scirp.78598-ref47">47</xref>]</td></tr><tr><td align="center" valign="middle" >6 Cu(2) site</td><td align="center" valign="middle" >1.9385 1.9388 1.9675 1.9947 2.3608 2.7578</td><td align="center" valign="middle" >1.830</td><td align="center" valign="middle" >0.223</td><td align="center" valign="middle" >2.053</td></tr><tr><td align="center" valign="middle"  rowspan="2"  >CuSO<sub>4</sub> ・5H<sub>2</sub>O Chalcanthite</td><td align="center" valign="middle" >2+2+2 Cu(1) site</td><td align="center" valign="middle" >1.9748 1.9770 2.3858</td><td align="center" valign="middle" >1.769</td><td align="center" valign="middle" >0.250</td><td align="center" valign="middle" >2.019</td><td align="center" valign="middle"  rowspan="2"  >[<xref ref-type="bibr" rid="scirp.78598-ref48">48</xref>]</td></tr><tr><td align="center" valign="middle" >2+2+2 Cu(2) site</td><td align="center" valign="middle" >1.9447 1.9696 2.4400</td><td align="center" valign="middle" >1.739</td><td align="center" valign="middle" >0.293</td><td align="center" valign="middle" >2.033</td></tr><tr><td align="center" valign="middle" >KNaCuSi<sub>4</sub>O<sub>10 </sub> Litidionite</td><td align="center" valign="middle" >6</td><td align="center" valign="middle" >1.9220 1.9434 1.9683 1.9799 2.6238 3.4024</td><td align="center" valign="middle" >1.863</td><td align="center" valign="middle" >0.109</td><td align="center" valign="middle" >1.972</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref22">22</xref>] ; this work</td></tr><tr><td align="center" valign="middle"  rowspan="2"  >Cu<sub>3</sub>(AsO<sub>4</sub>)<sub>2</sub> Lammerite</td><td align="center" valign="middle" >2 + 2 + 2 Cu(1) site</td><td align="center" valign="middle" >1.933 1.974 2.923</td><td align="center" valign="middle" >1.864</td><td align="center" valign="middle" >0.093</td><td align="center" valign="middle" >1.957</td><td align="center" valign="middle"  rowspan="2"  >[<xref ref-type="bibr" rid="scirp.78598-ref49">49</xref>]</td></tr><tr><td align="center" valign="middle" >6 Cu(2) site</td><td align="center" valign="middle" >1.941 1.947 1.972 2.028 2.282 2.782</td><td align="center" valign="middle" >1.772</td><td align="center" valign="middle" >0.254</td><td align="center" valign="middle" >2.026</td></tr><tr><td align="center" valign="middle" >CaCuAsO<sub>4</sub>OH Conichalcite</td><td align="center" valign="middle" >6</td><td align="center" valign="middle" >1.8850 1.8855 2.0666 2.0688 2.2976 2.3882</td><td align="center" valign="middle" >1.811</td><td align="center" valign="middle" >0.332</td><td align="center" valign="middle" >2.143</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref50">50</xref>] ; this work</td></tr><tr><td align="center" valign="middle" >La<sub>2</sub>CuO<sub>4</sub></td><td align="center" valign="middle" >4 + 2</td><td align="center" valign="middle" >1.9043 2.4145</td><td align="center" valign="middle" >2.151</td><td align="center" valign="middle" >0.278</td><td align="center" valign="middle" >2.439</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref51">51</xref>]</td></tr><tr><td align="center" valign="middle" >Sr<sub>2</sub>CuO<sub>2</sub>Cl<sub>2 </sub></td><td align="center" valign="middle" >4 + 2</td><td align="center" valign="middle" >1.9864 2.860</td><td align="center" valign="middle" >1.687</td><td align="center" valign="middle" >0.292</td><td align="center" valign="middle" >1.979</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref52">52</xref>]</td></tr></tbody></table></table-wrap><table-wrap id="table3" ><label><xref ref-type="table" rid="table3">Table 3</xref></label><caption><title> Collection of some properties and data for selected Cu(II) oxo-compounds.<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x29.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x29.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x30.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x29.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x30.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x31.png" xlink:type="simple"/></inline-formula>, energies in cm<sup>−1</sup>. Other transitions: CT charge transfer, SPE simultaneous pair excitation, ZRS? Zhang Rice excitation, E<sub>g</sub> energy gap</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Compound</th><th align="center" valign="middle" >Color</th><th align="center" valign="middle" >Cu site symmetry</th><th align="center" valign="middle" >Δ<sub>B </sub></th><th align="center" valign="middle" >Δ<sub>E</sub></th><th align="center" valign="middle" >Δ<sub>A </sub></th><th align="center" valign="middle" >Other Transition</th><th align="center" valign="middle" >Reference</th></tr></thead><tr><td align="center" valign="middle" >CaCuO<sub>2 </sub> (infinite layer)</td><td align="center" valign="middle" >dark-grey</td><td align="center" valign="middle" >D<sub>4h </sub></td><td align="center" valign="middle" >13,230</td><td align="center" valign="middle" >15,730</td><td align="center" valign="middle" >21,370</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref33">33</xref>]</td></tr><tr><td align="center" valign="middle" >Tenorite CuO</td><td align="center" valign="middle" >brownish</td><td align="center" valign="middle" >C<sub>i</sub></td><td align="center" valign="middle" >12,170</td><td align="center" valign="middle" >12,930 15,530</td><td align="center" valign="middle" >16,670</td><td align="center" valign="middle" >many</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref53">53</xref>] **</td></tr><tr><td align="center" valign="middle" >Conichalcite synth. CaCuAsO<sub>4</sub>OH</td><td align="center" valign="middle" >light green</td><td align="center" valign="middle" >C<sub>1</sub></td><td align="center" valign="middle" >10,575</td><td align="center" valign="middle" >12,500</td><td align="center" valign="middle" >8585</td><td align="center" valign="middle" >15,313 ZRS?<sup> </sup> 31,370 (E<sub>g</sub>)</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref54">54</xref>]</td></tr><tr><td align="center" valign="middle" >Lammerite synth. Cu<sub>3</sub>(AsO<sub>4</sub>)<sub>2 </sub></td><td align="center" valign="middle" >dark green</td><td align="center" valign="middle" >C<sub>1</sub> C<sub>i</sub></td><td align="center" valign="middle" >11,530</td><td align="center" valign="middle" >12,400 14,050</td><td align="center" valign="middle" >10,200 14,050</td><td align="center" valign="middle" >23,260 CuO 31,250 (E<sub>g</sub>)</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref22">22</xref>] ; this work*</td></tr><tr><td align="center" valign="middle"  rowspan="2"  >Y<sub>2</sub>BaCuO<sub>5</sub></td><td align="center" valign="middle"  rowspan="2"  >vivid green</td><td align="center" valign="middle"  rowspan="2"  >D<sub>4h </sub></td><td align="center" valign="middle"  colspan="2"  >12,500</td><td align="center" valign="middle"  rowspan="2"  >14,700</td><td align="center" valign="middle"  rowspan="2"  >25,970 CT</td><td align="center" valign="middle"  rowspan="2"  >[<xref ref-type="bibr" rid="scirp.78598-ref55">55</xref>] **</td></tr><tr><td align="center" valign="middle" >10,700</td><td align="center" valign="middle" >13,200</td></tr><tr><td align="center" valign="middle" >Azurite Cu<sub>3</sub>(CO<sub>3</sub>)<sub>2</sub>(OH)<sub>2</sub></td><td align="center" valign="middle" >blue</td><td align="center" valign="middle" >C<sub>i</sub> C<sub>1</sub></td><td align="center" valign="middle" >11,806 11,806</td><td align="center" valign="middle" >16,484 11,806</td><td align="center" valign="middle" >16,484 11,806</td><td align="center" valign="middle" >19,793 17,952</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref56">56</xref>] ** T = 80 K</td></tr><tr><td align="center" valign="middle" >Chalcanthite CuSO<sub>4</sub>・5H<sub>2</sub>O</td><td align="center" valign="middle" >deep blue</td><td align="center" valign="middle" >C<sub>1</sub> C<sub>1</sub></td><td align="center" valign="middle" >11,407 11,860</td><td align="center" valign="middle" >13,308 13,488</td><td align="center" valign="middle" >9699 9735</td><td align="center" valign="middle" >15,234 ZRS?<sup> </sup> 15,567<sup> </sup></td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref57">57</xref>]</td></tr><tr><td align="center" valign="middle" >Litidionite synth. KNaCuSi<sub>4</sub>O<sub>10 </sub></td><td align="center" valign="middle" >light blue</td><td align="center" valign="middle" >C<sub>i </sub></td><td align="center" valign="middle" >11,723</td><td align="center" valign="middle" >14,700</td><td align="center" valign="middle" >13,900</td><td align="center" valign="middle" >21,400 SPE 31,600 (E<sub>g</sub>)</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref22">22</xref>] [<xref ref-type="bibr" rid="scirp.78598-ref23">23</xref>] ; this work</td></tr><tr><td align="center" valign="middle" >Cu<sub>6</sub>Ge<sub>6</sub>O<sub>18</sub></td><td align="center" valign="middle" >dirty blue</td><td align="center" valign="middle" >C<sub>1 </sub></td><td align="center" valign="middle" >12,100</td><td align="center" valign="middle" >14,723</td><td align="center" valign="middle" >17,700</td><td align="center" valign="middle" >22,880 SPE</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref17">17</xref>] ; this work</td></tr><tr><td align="center" valign="middle" >Cu<sub>6</sub>Ge<sub>6</sub>O<sub>18</sub>・6H<sub>2</sub>O</td><td align="center" valign="middle" >bluish-green</td><td align="center" valign="middle" >C<sub>1 </sub></td><td align="center" valign="middle" >11,880</td><td align="center" valign="middle" >14,320</td><td align="center" valign="middle" >11,880</td><td align="center" valign="middle" >16,230 ZRS?<sup> </sup> 21,650 CT 30,300 (E<sub>g</sub>)</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref17">17</xref>] ; this work</td></tr><tr><td align="center" valign="middle" >Cu<sub>6</sub>Ge<sub>5.4</sub>Si<sub>0.6</sub>O<sub>18</sub>・6H<sub>2</sub>O<sub> </sub></td><td align="center" valign="middle" >dark green</td><td align="center" valign="middle" >C<sub>1</sub></td><td align="center" valign="middle"  colspan="2"  >13,300</td><td align="center" valign="middle" >19,400</td><td align="center" valign="middle" >23,900 CT</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref17">17</xref>]</td></tr><tr><td align="center" valign="middle" >CuGeO<sub>3 </sub></td><td align="center" valign="middle" >turquoise</td><td align="center" valign="middle" >D<sub>2h </sub></td><td align="center" valign="middle" >12,570</td><td align="center" valign="middle" >13,970</td><td align="center" valign="middle" >12,920</td><td align="center" valign="middle" >15,733 ZRS? 15,800</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref24">24</xref>] ; this work</td></tr><tr><td align="center" valign="middle" >BaCuSi<sub>4</sub>O<sub>10</sub> synth. (Effenbergite)</td><td align="center" valign="middle"  rowspan="3"  >deep blue</td><td align="center" valign="middle"  rowspan="3"  >D<sub>4h</sub></td><td align="center" valign="middle" >12,200</td><td align="center" valign="middle" >15,950</td><td align="center" valign="middle" >18,520</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref58">58</xref>]</td></tr><tr><td align="center" valign="middle" >SrCuSi<sub>4</sub>O<sub>10</sub> synth. (Wesselite)</td><td align="center" valign="middle" >12,480</td><td align="center" valign="middle" >16,050</td><td align="center" valign="middle" >18,520</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref58">58</xref>]</td></tr><tr><td align="center" valign="middle" >CaCuSi<sub>4</sub>O<sub>10</sub> synth. (Cuprorivaite)</td><td align="center" valign="middle" >12,590 12,740</td><td align="center" valign="middle" >15760 16130</td><td align="center" valign="middle" >18,530 18,520</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref44">44</xref>] [<xref ref-type="bibr" rid="scirp.78598-ref59">59</xref>]</td></tr><tr><td align="center" valign="middle" >Dioptase dehydrated Dioptase partly dehydrated</td><td align="center" valign="middle" >black dark blue</td><td align="center" valign="middle" >C<sub>1</sub></td><td align="center" valign="middle" >12,330 12,500</td><td align="center" valign="middle" >14,960 14,500</td><td align="center" valign="middle" >17,930 17,600</td><td align="center" valign="middle" >22,680 SPE -</td><td align="center" valign="middle" >This work; [<xref ref-type="bibr" rid="scirp.78598-ref19">19</xref>]</td></tr><tr><td align="center" valign="middle"  rowspan="2"  >Dioptase Cu<sub>6</sub>Si<sub>6</sub>O<sub>18</sub>・6H<sub>2</sub>O</td><td align="center" valign="middle"  rowspan="2"  >emerald green</td><td align="center" valign="middle"  rowspan="2"  >C<sub>1</sub></td><td align="center" valign="middle" >11,500 12,495</td><td align="center" valign="middle" >14,500 15,010</td><td align="center" valign="middle" >17,000 10,200</td><td align="center" valign="middle" ></td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref18">18</xref>] [<xref ref-type="bibr" rid="scirp.78598-ref19">19</xref>]</td></tr><tr><td align="center" valign="middle" >11,507</td><td align="center" valign="middle" >14,400</td><td align="center" valign="middle" >10,700</td><td align="center" valign="middle" >16,670 ZRS?<sup> </sup> 24,160 CT 30,660 (E<sub>g</sub>)</td><td align="center" valign="middle" >This work</td></tr></tbody></table></table-wrap><p>*synthetic lammerite with an amount of CuO; **for this work a different assignment as given in the reference was used.</p><p>Recently, the energy and symmetry of dd excitations of some undoped layered cuprates have been measured by CuL<sub>3</sub> resonant X-ray scattering [<xref ref-type="bibr" rid="scirp.78598-ref33">33</xref>] . The well- assigned dd excitations of these compounds with high connectedness were found to be higher than the energies of the compounds described before. Multiferroic CuO as limiting case can be added to this group with due allowance.<sub> </sub>Applying Equation (a), a steeper slope with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x32.png" xlink:type="simple"/></inline-formula> results, representing higher excitation energies and effective charges (Q<sub>e</sub> &#177; 1.35) than for the dioptase group.</p><p>The different connectedness of cuprates in comparison to the dioptase group is manifested in a larger contribution of the principal magnetic super-exchange interaction J<sub>z</sub> to the optical excitation energies. In <xref ref-type="fig" rid="fig5">Figure 5</xref>, this contribution is depicted versus the Cu-O-Cu bond angle Φ, a representation first used by Rocquefelte et al. [<xref ref-type="bibr" rid="scirp.78598-ref34">34</xref>] , and here applied in an extended form, illustrating both dioptase group compounds and cuprate ones. A data fit resulted in the relation</p><disp-formula id="scirp.78598-formula14"><label>. (11)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800411x33.png"  xlink:type="simple"/></disp-formula><p>with an exponent near 5/3, explained by chemical pressure (Rocquefelte et al., 2012) [<xref ref-type="bibr" rid="scirp.78598-ref34">34</xref>] [<xref ref-type="bibr" rid="scirp.78598-ref35">35</xref>] . Adding J<sub>z</sub>(Φ)・ln(2) as bond angle dependent contribution to the bond length dependent one, a surprisingly good agreement is achieved between the two groups of compounds, now giving<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x34.png" xlink:type="simple"/></inline-formula>, respectively Q<sub>e</sub> = 1.312. It should be noticed that for the dioptase group an antiferromagnetic contribution is not included because T<sub>N</sub> is lower than room temperature<sub>, </sub>at which<sub> </sub>the<sub> </sub>optical spectra are taken.</p><p>The R<sup>−5</sup> inverse power of Cu-O bond lengths is nearly a measure for the bond strength. Therefore, the reliability of the fit can be enhanced applying the empirical Cu-O bond strength relation s = Σ(R/R<sub>0</sub>)<sup>−N</sup> [<xref ref-type="bibr" rid="scirp.78598-ref36">36</xref>] by choosing only the</p><fig id="fig5"  position="float"><label><xref ref-type="fig" rid="fig5">Figure 5</xref></label><caption><title> Principal superexchange interaction J<sub>z</sub> versus Cu-O-Cu bond angle Φ [<xref ref-type="bibr" rid="scirp.78598-ref34">34</xref>] [<xref ref-type="bibr" rid="scirp.78598-ref35">35</xref>] </title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-4800411x35.png"/></fig><p>bond strength sum s<sub>e</sub> of the four equatorial bonds. New values R<sub>0</sub> = 1.713(9) &#197;, N = 5.76(16) were re-calculated for this work [<xref ref-type="bibr" rid="scirp.78598-ref37">37</xref>] . Results of a double-regression yielded for the cuprate group</p><disp-formula id="scirp.78598-formula15"><label>(12a)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800411x36.png"  xlink:type="simple"/></disp-formula><p>respectively <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x37.png" xlink:type="simple"/></inline-formula> (12b)</p><p>for both the dioptase group and cuprates. Δ<sub>B</sub> of the last mentioned group is corrected by a bond angle dependent (magnetic) contribution (<xref ref-type="fig" rid="fig6">Figure 6</xref>). It is recommended to extend the analytic bond strength-bond length expression by a magnetic (angle dependent) contribution. In contrast to this result, the quoted authors [<xref ref-type="bibr" rid="scirp.78598-ref33">33</xref>] fitted their cuprate data with a lower slope of N = 4.2. On the other hand, the selection of compounds for such fit is not convincing, because an influence of some equatorial O<sup>−</sup> ions in La<sub>2</sub>CuO<sub>4</sub> (high bond strength, see <xref ref-type="table" rid="table2">Table 2</xref>) on the excitation energies can be expected. In addition, the epitaxially grown infinite-layer structure of Ca<sub>0.5</sub>Sr<sub>0.5</sub>CuO<sub>2</sub> is obviously strained.</p><p>Turning now to the calculation of splitting parameters Ds (Equation (9)) and Dt (Equation (10)) involving axial ligands one has to distinguish according to the Nephelauxetic Effect between pure oxo-ligands and such ones as H<sub>2</sub>O or Cl<sup>−</sup> with increased cationic charge and assumed higher Dq<sub>a</sub> values [<xref ref-type="bibr" rid="scirp.78598-ref29">29</xref>] . H<sub>2</sub>O (as equatorial ligands) are found in chalcanthite, and hydroxyl groups in azurite and conichalcite. The last compound has the most distorted “octahedron” and should show a pronounced splitting of the <sup>2</sup>E<sub>g</sub> term, which is not considered here.</p><fig id="fig6"  position="float"><label><xref ref-type="fig" rid="fig6">Figure 6</xref></label><caption><title> A linear relation between Dq (cm<sup>−1</sup>) and the equatorial bond strength s<sub>e</sub>, in case of cuprates (red curve) corrected by a bond angle dependent (magnetic) contribution to show a single linear plot (green curve) with dioptase group compounds (yellow) besides cuprates (now green)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-4800411x38.png"/></fig><p>In the case of square-planar environment it is useful to limit the extent of the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x39.png" xlink:type="simple"/></inline-formula> orbital with “long” auxiliary axial bonds. Dehydrated dioptase and the germanate analogue already have some far distant oxygen ions (see <xref ref-type="table" rid="table2">Table 2</xref>) within the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x40.png" xlink:type="simple"/></inline-formula> orbital sphere of influence. For the group of M<sup>2+</sup>CuO<sub>2</sub> layered cuprates the limit is given by the layer separation down c of about 3.3 &#197;. Again the results differ somewhat for the two groups of compounds with slightly different effective charges. From the fitted values for Ds and Dt the Δ<sub>E</sub> (Equation (2)) and Δ<sub>A</sub> (Equation (3)) energies have been calculated as well as <sup>2</sup>E<sub>g</sub> and <sup>2</sup>A<sub>1g</sub>. Results are summarized in <xref ref-type="table" rid="table4">Table 4</xref>.</p><p>In order to check the correct assignment one can use a relation between experimental B<sub>2g</sub>, E<sub>g</sub> and A<sub>1g</sub> values of form<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x41.png" xlink:type="simple"/></inline-formula>, which results from Equations (1) to (3). Obviously, this relation holds only for shortest axial bonds and more octahedral ligand environment, such fulfilling the precondition for the underlying ionic model. For non-existent axial bonds the value for the quotient is close to unity. The values listed in <xref ref-type="table" rid="table4">Table 4</xref> indicate clearly bond length dependence. An empirical function <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x41.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x42.png" xlink:type="simple"/></inline-formula> may serve as a correction giving quotients f(Δ)/f(R) near unity when using α<sub>1</sub> = 0.59 for dioptase group compounds respectively 0.70 for cuprates. Compounds with axial water ligands or Cl<sup>−</sup> can clearly be identified by relatively small values. Another possibility here published the first time ever is to use the linear relation</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x43.png" xlink:type="simple"/></inline-formula>, where<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x43.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x44.png" xlink:type="simple"/></inline-formula>, (13)</p><p>with a R<sub>a</sub>/R<sub>e</sub> ratio including well adapted auxiliary R<sub>a</sub> bonds for compounds of coordination number 4, but different ε values for the dioptase group (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x45.png" xlink:type="simple"/></inline-formula>) and cuprates (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x45.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x46.png" xlink:type="simple"/></inline-formula>) to guide the regression line well through the origin (<xref ref-type="fig" rid="fig7">Figure 7</xref> and <xref ref-type="table" rid="table5">Table 5</xref>).</p><p>It should be stressed with respect to the use of mean bond distances in Equation (13) that also in the Equations (7) to (10) the mean of corresponding bond distances is taken first and then their inverse fifth power is calculated to yield the convincing results of <xref ref-type="table" rid="table4">Table 4</xref>.</p><p>An additional scaling <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x47.png" xlink:type="simple"/></inline-formula> between 1.7 and 2.0 (Equation (10)) is needed to fit the Dt values of compounds with H<sub>2</sub>O respectively Cl<sup>−</sup> as axial bonds. Also, La<sub>2</sub>CuO<sub>4</sub> needs such correction (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x47.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x48.png" xlink:type="simple"/></inline-formula>) possibly caused by some O<sup>- </sup>expected as axial ligands. Applied scaling factors were summarized as supplemented material in the <xref ref-type="table" rid="table7">Table 7</xref>.</p><p>Indeed, the connectedness of copper-ligand units, representing the number of shared copper-oxygen polyhedra, should be important for the dd excitation energy. Therefore, besides the equatorial ligand sums that are calculated as fit coordinate, we used the bond valence sums to check for inconsistent structural details and signs for mixed valences. Copper polygermanate in the Pbmm prototypic structure [<xref ref-type="bibr" rid="scirp.78598-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.78598-ref2">2</xref>] shows too high a sum with Σs = 2.08. There is evidence from EPR [<xref ref-type="bibr" rid="scirp.78598-ref38">38</xref>] , X-ray diffraction [<xref ref-type="bibr" rid="scirp.78598-ref39">39</xref>] and NQR measurements [<xref ref-type="bibr" rid="scirp.78598-ref40">40</xref>] that copper is statistically out of center of the CuO<sub>2</sub> plaquette, in this way the copper bond</p><table-wrap id="table4" ><label><xref ref-type="table" rid="table4">Table 4</xref></label><caption><title> Comparison of experimental and calculated excitation energies and orbital ones in cm<sup>−1</sup>. Δ<sub>B</sub> is sorted from high values to low ones down the table;<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x49.png" xlink:type="simple"/></inline-formula>,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x49.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x50.png" xlink:type="simple"/></inline-formula>. Experimental and calculated Δ values are arranged one above the other</title></caption><table><tbody><thead><tr><th align="center" valign="middle"  colspan="15"  >Isolated CuO plaquettes, clusters and chains: Calculation with<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x51.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x52.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x53.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x54.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x55.png" xlink:type="simple"/></inline-formula></th></tr></thead><tr><td align="center" valign="middle"  rowspan="2"  >Phase</td><td align="center" valign="middle"  rowspan="2"  >Δ<sub>B</sub><sub> </sub></td><td align="center" valign="middle"  colspan="2"   rowspan="2"  >Δ<sub>E</sub><sub> </sub></td><td align="center" valign="middle"  rowspan="2"  >Δ<sub>A</sub><sub> </sub></td><td align="center" valign="middle"  rowspan="2"  >Ds</td><td align="center" valign="middle"  rowspan="2"  >Dq</td><td align="center" valign="middle"  rowspan="2"  >Dt</td><td align="center" valign="middle"  rowspan="2"  >Dt/Dq</td><td align="center" valign="middle"  rowspan="2"  >Dt/Ds</td><td align="center" valign="middle"  colspan="2"   rowspan="2"  >f(Δ)</td><td align="center" valign="middle"  rowspan="2"  >f(Δ)/f(R)</td><td align="center" valign="middle"  colspan="2"  >Ligands</td></tr><tr><td align="center" valign="middle" >equat.</td><td align="center" valign="middle" >axial</td></tr><tr><td align="center" valign="middle" >Cuprorivaite</td><td align="center" valign="middle" >12,590 12,501</td><td align="center" valign="middle"  colspan="2"  >15,760 15,446</td><td align="center" valign="middle" >18,530 18,414</td><td align="center" valign="middle" >3100 3051</td><td align="center" valign="middle" >1259 1250</td><td align="center" valign="middle" >1226 1241</td><td align="center" valign="middle" >0.974</td><td align="center" valign="middle" >0.395</td><td align="center" valign="middle"  colspan="2"  >0.979</td><td align="center" valign="middle" >0.956</td><td align="center" valign="middle" >oxygen</td><td align="center" valign="middle" >no</td></tr><tr><td align="center" valign="middle" >CuGeO<sub>3</sub></td><td align="center" valign="middle" >12,570 12,439</td><td align="center" valign="middle"  colspan="2"  >13,970 14,209</td><td align="center" valign="middle" >13,970 14,324</td><td align="center" valign="middle" >2196 2299</td><td align="center" valign="middle" >1257 1244</td><td align="center" valign="middle" >1037 1026</td><td align="center" valign="middle" >0.825</td><td align="center" valign="middle" >0.472</td><td align="center" valign="middle"  colspan="2"  >0.909</td><td align="center" valign="middle" >1.081</td><td align="center" valign="middle" >oxygen</td><td align="center" valign="middle" >oxygen</td></tr><tr><td align="center" valign="middle" >Effenbergite</td><td align="center" valign="middle" >12,500 12,566</td><td align="center" valign="middle"  colspan="2"  >15,950 15,895</td><td align="center" valign="middle" >18,520 18,591</td><td align="center" valign="middle" >3139 3132</td><td align="center" valign="middle" >1250 1257</td><td align="center" valign="middle" >1139 1213</td><td align="center" valign="middle" >0.955</td><td align="center" valign="middle" >0.380</td><td align="center" valign="middle"  colspan="2"  >0.955</td><td align="center" valign="middle" >0.930</td><td align="center" valign="middle" >oxygen</td><td align="center" valign="middle" >no</td></tr><tr><td align="center" valign="middle" >Wesselite</td><td align="center" valign="middle" >12,480 12,566</td><td align="center" valign="middle"  colspan="2"  >16,050 15,895</td><td align="center" valign="middle" >18,520 18,591</td><td align="center" valign="middle" >3156 3132</td><td align="center" valign="middle" >1248 1257</td><td align="center" valign="middle" >1179 1213</td><td align="center" valign="middle" >0.945</td><td align="center" valign="middle" >0.374</td><td align="center" valign="middle"  colspan="2"  >0.944</td><td align="center" valign="middle" >0.920</td><td align="center" valign="middle" >oxygen</td><td align="center" valign="middle" >no</td></tr><tr><td align="center" valign="middle" >Dioptase black</td><td align="center" valign="middle" >12,330 12,324</td><td align="center" valign="middle"  colspan="2"  >14,960 15,057</td><td align="center" valign="middle" >17,930 17,850</td><td align="center" valign="middle" >2937 2940</td><td align="center" valign="middle" >1233 1232</td><td align="center" valign="middle" >1236 1218</td><td align="center" valign="middle" >1.003</td><td align="center" valign="middle" >0.421</td><td align="center" valign="middle"  colspan="2"  >1.019</td><td align="center" valign="middle" >1.013</td><td align="center" valign="middle" >oxygen</td><td align="center" valign="middle" >no</td></tr><tr><td align="center" valign="middle" >Cu<sub>6</sub>Ge<sub>6</sub>O<sub>18 </sub></td><td align="center" valign="middle" >12,100 12,123</td><td align="center" valign="middle"  colspan="2"  >14,723 14,845</td><td align="center" valign="middle" >17,700 17,606</td><td align="center" valign="middle" >2903 2904</td><td align="center" valign="middle" >1210 1212</td><td align="center" valign="middle" >1217 1198</td><td align="center" valign="middle" >1.006</td><td align="center" valign="middle" >0.419</td><td align="center" valign="middle"  colspan="2"  >1.020</td><td align="center" valign="middle" >1.017</td><td align="center" valign="middle" >oxygen</td><td align="center" valign="middle" >no</td></tr><tr><td align="center" valign="middle" >Ge-Dioptase</td><td align="center" valign="middle" >11,884 11,929</td><td align="center" valign="middle"  colspan="2"  >14,321 14,434</td><td align="center" valign="middle" >11,884 12,084</td><td align="center" valign="middle" >2046 2084</td><td align="center" valign="middle" >1188 1193</td><td align="center" valign="middle" >740 750</td><td align="center" valign="middle" >0.623</td><td align="center" valign="middle" >0.362</td><td align="center" valign="middle"  colspan="2"  >0.709</td><td align="center" valign="middle" >0.866</td><td align="center" valign="middle" >oxygen</td><td align="center" valign="middle" >H<sub>2</sub>O</td></tr><tr><td align="center" valign="middle" >Azurite (1)</td><td align="center" valign="middle" >11,806 12,070</td><td align="center" valign="middle"  colspan="2"  >16,484 14,162</td><td align="center" valign="middle" >16,484 15,014</td><td align="center" valign="middle" >− 2444</td><td align="center" valign="middle" >1181 1207</td><td align="center" valign="middle" >− 1048</td><td align="center" valign="middle" >0.770</td><td align="center" valign="middle" >0.317</td><td align="center" valign="middle"  colspan="2"  >0.809</td><td align="center" valign="middle" >1.024</td><td align="center" valign="middle" >OH<sup>−</sup>/ oxygen<sup> </sup></td><td align="center" valign="middle" >oxygen</td></tr><tr><td align="center" valign="middle" >Azurite (2)</td><td align="center" valign="middle" >11,550 11,589</td><td align="center" valign="middle"  colspan="2"  >12,770 12,924</td><td align="center" valign="middle" >11,300 11,669</td><td align="center" valign="middle" >1789 1858</td><td align="center" valign="middle" >1155 1159</td><td align="center" valign="middle" >829 848</td><td align="center" valign="middle" >0.718</td><td align="center" valign="middle" >0.464</td><td align="center" valign="middle"  colspan="2"  >0.808</td><td align="center" valign="middle" >1.067</td><td align="center" valign="middle" >OH<sup>−</sup>/ oxygen</td><td align="center" valign="middle" >oxygen</td></tr><tr><td align="center" valign="middle" >Litidionite</td><td align="center" valign="middle" >11,723 11,794</td><td align="center" valign="middle"  colspan="2"  >14,700 14,465</td><td align="center" valign="middle" >13,900 13,917</td><td align="center" valign="middle" >2411 2397</td><td align="center" valign="middle" >1172 1179</td><td align="center" valign="middle" >851 866</td><td align="center" valign="middle" >0.726</td><td align="center" valign="middle" >0.353</td><td align="center" valign="middle"  colspan="2"  >0.786</td><td align="center" valign="middle" >0.915</td><td align="center" valign="middle" >oxygen</td><td align="center" valign="middle" >oxygen</td></tr><tr><td align="center" valign="middle" >Lammerite (1)</td><td align="center" valign="middle" >11,780 11,735</td><td align="center" valign="middle"  colspan="2"  >13,744 13,744</td><td align="center" valign="middle" >14,356 14,357</td><td align="center" valign="middle" >2331 2328</td><td align="center" valign="middle" >1178 1174</td><td align="center" valign="middle" >1006 1000</td><td align="center" valign="middle" >0.854</td><td align="center" valign="middle" >0.432</td><td align="center" valign="middle"  colspan="2"  >0.914</td><td align="center" valign="middle" >0.914</td><td align="center" valign="middle" >oxygen</td><td align="center" valign="middle" >oxygen</td></tr><tr><td align="center" valign="middle" >Lammerite (2)</td><td align="center" valign="middle" >11,280 11,231</td><td align="center" valign="middle"  colspan="2"  >12,400 12,425</td><td align="center" valign="middle" >10,200 10,279</td><td align="center" valign="middle" >1617 1639</td><td align="center" valign="middle" >1128 1123</td><td align="center" valign="middle" >746 745</td><td align="center" valign="middle" >0.662</td><td align="center" valign="middle" >0.461</td><td align="center" valign="middle"  colspan="2"  >0.754</td><td align="center" valign="middle" >1.023</td><td align="center" valign="middle" >oxygen</td><td align="center" valign="middle" >oxygen</td></tr><tr><td align="center" valign="middle" >Chalcanthite (1)</td><td align="center" valign="middle" >11,407 11,135</td><td align="center" valign="middle"  colspan="2"  >12,600 12,302</td><td align="center" valign="middle" >8900 8828</td><td align="center" valign="middle" >1442 1428</td><td align="center" valign="middle" >1141 1113</td><td align="center" valign="middle" >627 623</td><td align="center" valign="middle" >0.549</td><td align="center" valign="middle" >0.435</td><td align="center" valign="middle"  colspan="2"  >0.645</td><td align="center" valign="middle" >0.906</td><td align="center" valign="middle" >H<sub>2</sub>O</td><td align="center" valign="middle" >oxygen</td></tr><tr><td align="center" valign="middle" >Chalcanthite (2)</td><td align="center" valign="middle" >11,860 11,678</td><td align="center" valign="middle"  colspan="2"  >13,488 13,369</td><td align="center" valign="middle" >9735 98,108</td><td align="center" valign="middle" >1623 1643</td><td align="center" valign="middle" >1186 1168</td><td align="center" valign="middle" >648 648</td><td align="center" valign="middle" >0.547</td><td align="center" valign="middle" >0.399</td><td align="center" valign="middle"  colspan="2"  >0.644</td><td align="center" valign="middle" >0.875</td><td align="center" valign="middle" >H<sub>2</sub>O</td><td align="center" valign="middle" >oxygen</td></tr><tr><td align="center" valign="middle" >Dioptase green</td><td align="center" valign="middle" >11,508 11,491</td><td align="center" valign="middle"  colspan="2"  >14,398 14,094</td><td align="center" valign="middle" >10,700 10,325</td><td align="center" valign="middle" >1940 1847</td><td align="center" valign="middle" >1151 1149</td><td align="center" valign="middle" >588 587</td><td align="center" valign="middle" >0.511</td><td align="center" valign="middle" >0.303</td><td align="center" valign="middle"  colspan="2"  >0.619</td><td align="center" valign="middle" >0.801</td><td align="center" valign="middle" >oxygen</td><td align="center" valign="middle" >H<sub>2</sub>O</td></tr><tr><td align="center" valign="middle" >Conichalcite</td><td align="center" valign="middle" >11,400 11,119</td><td align="center" valign="middle"  colspan="2"  >12,195 11,922</td><td align="center" valign="middle" >8585 8449</td><td align="center" valign="middle" >1340 1339</td><td align="center" valign="middle" >1140 1141</td><td align="center" valign="middle" >645 658</td><td align="center" valign="middle" >0.566</td><td align="center" valign="middle" >0.481</td><td align="center" valign="middle"  colspan="2"  >0.661</td><td align="center" valign="middle" >0.940</td><td align="center" valign="middle" >OH<sup>−</sup></td><td align="center" valign="middle" >oxygen</td></tr><tr><td align="center" valign="middle"  rowspan="2"  >Y<sub>2</sub>BaCuO<sub>5</sub></td><td align="center" valign="middle"  colspan="3"  >10,700 13,200*)</td><td align="center" valign="middle"  rowspan="2"  >14,700 14,571</td><td align="center" valign="middle"  rowspan="2"  >2457 2435</td><td align="center" valign="middle"  rowspan="2"  >1070 1073</td><td align="center" valign="middle"  rowspan="2"  >974 966</td><td align="center" valign="middle"  rowspan="2"  >0.911</td><td align="center" valign="middle"  rowspan="2"  >0.397</td><td align="center" valign="middle"  colspan="2"   rowspan="2"  >0.936</td><td align="center" valign="middle"  rowspan="2"  >0.904</td><td align="center" valign="middle"  rowspan="2"  >oxygen</td><td align="center" valign="middle"  rowspan="2"  >oxygen</td></tr><tr><td align="center" valign="middle"  colspan="2"  >10,732</td><td align="center" valign="middle" >13,205</td></tr><tr><td align="center" valign="middle"  colspan="15"  >Cuprates (undoped): Calculation with<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x56.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x57.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x58.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x59.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x60.png" xlink:type="simple"/></inline-formula></td></tr><tr><td align="center" valign="middle"  rowspan="2"  >Phase</td><td align="center" valign="middle"  rowspan="2"  >Δ<sub>B </sub></td><td align="center" valign="middle"  colspan="2"   rowspan="2"  >Δ<sub>E</sub><sub> </sub></td><td align="center" valign="middle"  rowspan="2"  >Δ<sub>A</sub><sub> </sub></td><td align="center" valign="middle"  rowspan="2"  >Ds</td><td align="center" valign="middle"  rowspan="2"  >Dq</td><td align="center" valign="middle"  rowspan="2"  >Dt</td><td align="center" valign="middle"  rowspan="2"  >Dt/Dq</td><td align="center" valign="middle"  rowspan="2"  >Dt/Ds</td><td align="center" valign="middle"  rowspan="2"  >f(Δ)</td><td align="center" valign="middle"  colspan="2"   rowspan="2"  >f(Δ)/f(R)</td><td align="center" valign="middle"  colspan="2"  >Ligands</td></tr><tr><td align="center" valign="middle" >equat.</td><td align="center" valign="middle" >axial</td></tr><tr><td align="center" valign="middle" >La<sub>2</sub>CuO<sub>4</sub></td><td align="center" valign="middle" >14,516 14,308</td><td align="center" valign="middle"  colspan="2"  >17,097 16,833</td><td align="center" valign="middle" >13,710 13,664</td><td align="center" valign="middle" >2327 2313</td><td align="center" valign="middle" >1452 1431</td><td align="center" valign="middle" >880 883</td><td align="center" valign="middle" >0.606</td><td align="center" valign="middle" >0.378</td><td align="center" valign="middle" >0.697</td><td align="center" valign="middle"  colspan="2"  >0.788</td><td align="center" valign="middle" >oxygen</td><td align="center" valign="middle" >O<sup>−</sup>?</td></tr><tr><td align="center" valign="middle" >CaCuO<sub>2</sub></td><td align="center" valign="middle" >13,226 13,322</td><td align="center" valign="middle"  colspan="2"  >15,726 15,982</td><td align="center" valign="middle" >21,370 21,671</td><td align="center" valign="middle" >3410 3476</td><td align="center" valign="middle" >1323 1332</td><td align="center" valign="middle" >1546 1554</td><td align="center" valign="middle" >1.169</td><td align="center" valign="middle" >0.453</td><td align="center" valign="middle" >1.173</td><td align="center" valign="middle"  colspan="2"  >0.994</td><td align="center" valign="middle" >oxygen</td><td align="center" valign="middle" >no</td></tr><tr><td align="center" valign="middle" >Sr<sub>0.5</sub>Ca<sub>0.5</sub>CuO<sub>2</sub></td><td align="center" valign="middle" >12,581 12,744</td><td align="center" valign="middle"  colspan="2"  >15,565 15,494</td><td align="center" valign="middle" >21,452 21,026</td><td align="center" valign="middle" >3491 3397</td><td align="center" valign="middle" >1258 1274</td><td align="center" valign="middle" >1498 1488</td><td align="center" valign="middle" >1.190</td><td align="center" valign="middle" >0.429</td><td align="center" valign="middle" >1.157</td><td align="center" valign="middle"  colspan="2"  >0.976</td><td align="center" valign="middle" >oxygen</td><td align="center" valign="middle" >no</td></tr><tr><td align="center" valign="middle" >NdBa<sub>2</sub>Cu<sub>3</sub>O<sub>6 </sub></td><td align="center" valign="middle" >12,258 12,372</td><td align="center" valign="middle"  colspan="2"  >14,113 13,741</td><td align="center" valign="middle" >15,968 15,940</td><td align="center" valign="middle" >2546 2473</td><td align="center" valign="middle" >1226 1237</td><td align="center" valign="middle" >1157 1210</td><td align="center" valign="middle" >0.944</td><td align="center" valign="middle" >0.454</td><td align="center" valign="middle" >1.000</td><td align="center" valign="middle"  colspan="2"  >1.072</td><td align="center" valign="middle" >oxygen</td><td align="center" valign="middle" >oxygen</td></tr><tr><td align="center" valign="middle" >CuO (tenorite)</td><td align="center" valign="middle" >12,170 12,254</td><td align="center" valign="middle"  colspan="2"  >14,230 14,520</td><td align="center" valign="middle" >16,670 16,878</td><td align="center" valign="middle" >2676 2735</td><td align="center" valign="middle" >1217 1225</td><td align="center" valign="middle" >1193 1188</td><td align="center" valign="middle" >0.981</td><td align="center" valign="middle" >0.446</td><td align="center" valign="middle" >1.023</td><td align="center" valign="middle"  colspan="2"  >1.027</td><td align="center" valign="middle" >oxygen</td><td align="center" valign="middle" >oxygen</td></tr><tr><td align="center" valign="middle" >Sr<sub>2</sub>CuO<sub>2</sub>Cl<sub>2</sub></td><td align="center" valign="middle" >12,097 11,838</td><td align="center" valign="middle"  colspan="2"  >14,839 14,756</td><td align="center" valign="middle" >15,887 16,021</td><td align="center" valign="middle" >2661 2706</td><td align="center" valign="middle" >1210 1184</td><td align="center" valign="middle" >1048 1040</td><td align="center" valign="middle" >0.867</td><td align="center" valign="middle" >0.394</td><td align="center" valign="middle" >0.904</td><td align="center" valign="middle"  colspan="2"  >0.897</td><td align="center" valign="middle" >oxygen<sup> </sup></td><td align="center" valign="middle" >Cl<sup>−</sup></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr></tbody></table></table-wrap><p>*) The broad band at 12,500 cm<sup>−</sup><sup>1</sup> is proven to split into two bands at about 10,700 cm<sup>−</sup><sup>1</sup> and 13,200 cm<sup>−</sup><sup>1</sup>, respectively.</p><table-wrap id="table5" ><label><xref ref-type="table" rid="table5">Table 5</xref></label><caption><title> Experimental ∆<sub>A</sub> energies versus calculated ones using the relation: ∆<sub>A</sub> = 17,892・(<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x61.png" xlink:type="simple"/></inline-formula>) (cm<sup>−1</sup>), <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x61.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x62.png" xlink:type="simple"/></inline-formula>for dioptase group and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x61.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x62.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x63.png" xlink:type="simple"/></inline-formula> for cuprates. Auxiliary bonds introduced in case of compounds with coordination number CN = [<xref ref-type="bibr" rid="scirp.78598-ref4">4</xref>] are underlined</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Phase</th><th align="center" valign="middle" >CN</th><th align="center" valign="middle" >e&gt; (&#197;)</th><th align="center" valign="middle" >a&gt; (&#197;)</th><th align="center" valign="middle" >Δ<sub>A</sub> (exp.)</th><th align="center" valign="middle" >Δ<sub>A</sub> (calc.)</th></tr></thead><tr><td align="center" valign="middle" >Cuprorivaite</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref4">4</xref>]</td><td align="center" valign="middle" >1.9307</td><td align="center" valign="middle" >3.35</td><td align="center" valign="middle" >18,530</td><td align="center" valign="middle" >18,393</td></tr><tr><td align="center" valign="middle" >CuGeO<sub>3</sub></td><td align="center" valign="middle" >[4 + 2]</td><td align="center" valign="middle" >1.9326</td><td align="center" valign="middle" >2.7549</td><td align="center" valign="middle" >12,920</td><td align="center" valign="middle" >12,854</td></tr><tr><td align="center" valign="middle" >Effenbergite</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref4">4</xref>]</td><td align="center" valign="middle" >1.9265</td><td align="center" valign="middle" >3.35</td><td align="center" valign="middle" >18,520</td><td align="center" valign="middle" >18,460</td></tr><tr><td align="center" valign="middle" >Wesselite</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref4">4</xref>]</td><td align="center" valign="middle" >1.9265</td><td align="center" valign="middle" >3.35</td><td align="center" valign="middle" >18,520</td><td align="center" valign="middle" >18,460</td></tr><tr><td align="center" valign="middle" >Dioptase black</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref4">4</xref>]</td><td align="center" valign="middle" >1.9340</td><td align="center" valign="middle" >3.30</td><td align="center" valign="middle" >17,930</td><td align="center" valign="middle" >17,874</td></tr><tr><td align="center" valign="middle" >Cu<sub>6</sub>Ge<sub>6</sub>O<sub>18 </sub></td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref4">4</xref>]</td><td align="center" valign="middle" >1.9404</td><td align="center" valign="middle" >3.30</td><td align="center" valign="middle" >17,700</td><td align="center" valign="middle" >17,777</td></tr><tr><td align="center" valign="middle" >Ge-Dioptase</td><td align="center" valign="middle" >[4 + 2]</td><td align="center" valign="middle" >1.9474</td><td align="center" valign="middle" >2.6622</td><td align="center" valign="middle" >11,884</td><td align="center" valign="middle" >11,808</td></tr><tr><td align="center" valign="middle" >Azurite (1)</td><td align="center" valign="middle" >[4 + 2]</td><td align="center" valign="middle" >1.9434</td><td align="center" valign="middle" >2.9840</td><td align="center" valign="middle" >16,488 (?)</td><td align="center" valign="middle" >14,821</td></tr><tr><td align="center" valign="middle" >Azurite (2)</td><td align="center" valign="middle" >[4 + 1 + 1]</td><td align="center" valign="middle" >1.9593</td><td align="center" valign="middle" >2.5143</td><td align="center" valign="middle" >11,806</td><td align="center" valign="middle" >10,309</td></tr><tr><td align="center" valign="middle" >Litidionite</td><td align="center" valign="middle" >[4 + 2]</td><td align="center" valign="middle" >1.9525</td><td align="center" valign="middle" >2.8434</td><td align="center" valign="middle" >13,900</td><td align="center" valign="middle" >13,404</td></tr><tr><td align="center" valign="middle" >Lammerite (1)</td><td align="center" valign="middle" >[4 + 2]</td><td align="center" valign="middle" >1.9529</td><td align="center" valign="middle" >2.9230</td><td align="center" valign="middle" >14,350</td><td align="center" valign="middle" >14,128</td></tr><tr><td align="center" valign="middle" >Lammerite (2)</td><td align="center" valign="middle" >[4 + 1 + 1]</td><td align="center" valign="middle" >1.9703</td><td align="center" valign="middle" >2.4609</td><td align="center" valign="middle" >10,200</td><td align="center" valign="middle" >9695</td></tr><tr><td align="center" valign="middle" >Chalcanthite (1)</td><td align="center" valign="middle" >[4 + 2]</td><td align="center" valign="middle" >1.9759</td><td align="center" valign="middle" >2.3858</td><td align="center" valign="middle" >8900</td><td align="center" valign="middle" >8952</td></tr><tr><td align="center" valign="middle" >Chalcanthite (2)</td><td align="center" valign="middle" >[4 + 2]</td><td align="center" valign="middle" >1.9569</td><td align="center" valign="middle" >2.4400</td><td align="center" valign="middle" >9735</td><td align="center" valign="middle" >9657</td></tr><tr><td align="center" valign="middle" >Dioptase green</td><td align="center" valign="middle" >[4 + 2]</td><td align="center" valign="middle" >1.9613</td><td align="center" valign="middle" >2.5688</td><td align="center" valign="middle" >10,700</td><td align="center" valign="middle" >10,735</td></tr><tr><td align="center" valign="middle" >Conichalcite</td><td align="center" valign="middle" >[2 + 2 + 2]</td><td align="center" valign="middle" >1.9640</td><td align="center" valign="middle" >2.3403</td><td align="center" valign="middle" >8585</td><td align="center" valign="middle" >8668</td></tr><tr><td align="center" valign="middle" >Y<sub>2</sub>BaCuO<sub>5</sub></td><td align="center" valign="middle" >[4 + 1]</td><td align="center" valign="middle" >1.9899</td><td align="center" valign="middle" >2.196 + 3.90</td><td align="center" valign="middle" >14,700</td><td align="center" valign="middle" >14,754</td></tr><tr><td align="center" valign="middle" >La<sub>2</sub>CuO<sub>4</sub></td><td align="center" valign="middle" >[4 + 2]</td><td align="center" valign="middle" >1.9043</td><td align="center" valign="middle" >2.4045</td><td align="center" valign="middle" >13,710</td><td align="center" valign="middle" >13,646</td></tr><tr><td align="center" valign="middle" >CaCuO<sub>2</sub></td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref4">4</xref>]</td><td align="center" valign="middle" >1.9281</td><td align="center" valign="middle" >3.26</td><td align="center" valign="middle" >21,370</td><td align="center" valign="middle" >21,306</td></tr><tr><td align="center" valign="middle" >Sr<sub>0.5</sub>Ca<sub>0.5</sub>CuO<sub>2</sub></td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.78598-ref4">4</xref>]</td><td align="center" valign="middle" >1.9440</td><td align="center" valign="middle" >3.30</td><td align="center" valign="middle" >21,452</td><td align="center" valign="middle" >21,426</td></tr><tr><td align="center" valign="middle" >NdBa<sub>2</sub>Cu<sub>3</sub>O<sub>7-δ </sub></td><td align="center" valign="middle" >[4 + 1]</td><td align="center" valign="middle" >1.9609</td><td align="center" valign="middle" >2.275 + 3.25</td><td align="center" valign="middle" >15,968</td><td align="center" valign="middle" >16,260</td></tr><tr><td align="center" valign="middle" >CuO (tenorite)</td><td align="center" valign="middle" >[4 + 2]</td><td align="center" valign="middle" >1.9558</td><td align="center" valign="middle" >2.7842</td><td align="center" valign="middle" >16,670</td><td align="center" valign="middle" >16,524</td></tr><tr><td align="center" valign="middle" >Sr<sub>2</sub>CuO<sub>2</sub>Cl<sub>2</sub></td><td align="center" valign="middle" >[4 + 2]</td><td align="center" valign="middle" >1.9864</td><td align="center" valign="middle" >2.8600</td><td align="center" valign="middle" >15,887</td><td align="center" valign="middle" >16,841</td></tr></tbody></table></table-wrap><p>strength is reduced towards the net charge of 2+. Even large thermal displacement ellipsoids indicate structural features that require a careful evaluation. Bond lengths should be corrected for “thermal” displacement because not less than their inverse fifth power is used in calculations (see for instance [<xref ref-type="bibr" rid="scirp.78598-ref51">51</xref>] ).</p></sec><sec id="s4"><title>4. EPR Analysis</title><p>Finally, the assignment of the dd excitations can be compared with results of EPR measurements. For 3d<sup>9</sup> ions in (nearly) tetragonal ligand symmetry one can apply the following two formulas for the principal components g<sub>||</sub> and g<sub>﬩</sub>, if the ground state is <sup>2</sup>B<sub>1g</sub>:</p><disp-formula id="scirp.78598-formula16"><label>, (14)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800411x64.png"  xlink:type="simple"/></disp-formula><fig id="fig7"  position="float"><label><xref ref-type="fig" rid="fig7">Figure 7</xref></label><caption><title> Δ<sub>A</sub> excitation energies (cm<sup>−1</sup>) depicted versus a function of axial to equatorial bond distances. Again the cuprate group excitations (in red) must be corrected by a (magnetic) contribution to reliably represent all data in a single regression line. Auxiliary axial bonds (see the yellow field) were introduced in case of compounds with really missing axial bonds (coordination number 4)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-4800411x65.png"/></fig><disp-formula id="scirp.78598-formula17"><label>, (15)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800411x66.png"  xlink:type="simple"/></disp-formula><p>where g<sub>e</sub> = 2.0023 is the g-value for the free electron, and λ is the spin-orbital coupling parameter, which yields for the free Cu<sup>2+</sup> ion λ<sub>o</sub> = 829 cm<sup>−1</sup> [<xref ref-type="bibr" rid="scirp.78598-ref60">60</xref>] .</p><p>The k values are the spin orbital reduction factors used to scale the coupling parameters to the free Cu<sup>2+</sup> ion value, k = λ/λ<sub>o</sub>. This parameter reduction is attributed to covalence effects. <xref ref-type="table" rid="table6">Table 6</xref> compares the results for dioptase and Ge- dioptase, respectively. Not surprisingly, the found covalence reduction effect is markedly smaller for the copper germanate than for the copper silicate, in accordance with crystal-chemical experience, confirming higher ionicity of the germanate (<xref ref-type="table" rid="table6">Table 6</xref>). Unfortunately, EPR data for the dehydrated compounds were not available.</p><table-wrap id="table6" ><label><xref ref-type="table" rid="table6">Table 6</xref></label><caption><title> EPR analysis of dioptase related compounds</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Notation</th><th align="center" valign="middle" >Dioptase</th><th align="center" valign="middle" >Ge-Dioptase</th></tr></thead><tr><td align="center" valign="middle" >Δ<sub>B</sub></td><td align="center" valign="middle" >11,508</td><td align="center" valign="middle" >11,884</td></tr><tr><td align="center" valign="middle" >Δ<sub>E</sub><sub> </sub></td><td align="center" valign="middle" >14,395</td><td align="center" valign="middle" >14,321</td></tr><tr><td align="center" valign="middle" >Δ<sub>A</sub><sub> </sub></td><td align="center" valign="middle" >10,700</td><td align="center" valign="middle" >11,884</td></tr><tr><td align="center" valign="middle" >g<sub>|| </sub></td><td align="center" valign="middle" >2.3601</td><td align="center" valign="middle" >2.3780</td></tr><tr><td align="center" valign="middle" >g<sub>﬩</sub></td><td align="center" valign="middle" >2.0511</td><td align="center" valign="middle" >2.0970</td></tr><tr><td align="center" valign="middle" >λ<sub>|| </sub></td><td align="center" valign="middle" >−504.08</td><td align="center" valign="middle" >−545.53</td></tr><tr><td align="center" valign="middle" >k<sub>|| </sub></td><td align="center" valign="middle" >0.608</td><td align="center" valign="middle" >0.658</td></tr><tr><td align="center" valign="middle" >λ<sub> ﬩</sub><sub> </sub></td><td align="center" valign="middle" >−346.91</td><td align="center" valign="middle" >−662.63</td></tr><tr><td align="center" valign="middle" >k<sub>﬩</sub></td><td align="center" valign="middle" >0.418</td><td align="center" valign="middle" >0.799</td></tr></tbody></table></table-wrap></sec><sec id="s5"><title>5. Conclusion</title><p>As shown, a comparative reappraisal of Cu<sup>2+</sup> UV-VIS spectra benefits from a special consideration of crystal-chemically similar groups of compounds, com- paring exemplarily the dioptase group, covering minerals as well as synthetic samples, with cuprates. The assignment of dd excitations and their representa- tion each on a single curve is possible by attributing a magnetic (bond angle de- pendent) contribution to the cuprate group. It is recommended to extend the bond strength-bond length relation by a bond angle dependent (magnetic) con- tribution. Deviations of the linear representation of orbital excitation energies may be helpful to discriminate results of compounds with peculiar orbital features from those with normal behavior. Fortunately, the first done assignment of well-resolved spectra of dehydrated dioptase Cu<sub>6</sub>(Ge,Si)<sub>6</sub>O<sub>18</sub> served as input data to deconvolute the badly resolved spectra of as-grown Cu<sub>6</sub>(Ge,Si)<sub>6</sub>O<sub>18</sub>・6H<sub>2</sub>O samples. At present, the deconvolution of superposed spectra resulting from different Cu sites of a structure is inadequate. However, a pre-calculation of the expected energy levels can serve as input for fitting the experimental spectra. This has been successfully applied to lammerite. It is recommended to take a series of UV-VIS spectra step by step over the entire temperature range from hydrated to fully dehydrated dioptase as a didactic tool to follow the energy levels and their correct assignment, thereby simultaneously controlling the crystal water content by IR spectroscopy with a device that offers both analytical possibilities. Especially it should be investigated whether a Zhang-Rice excitation like that observed for CuGeO<sub>3</sub> can be confirmed for the hydrated compounds of the dioptase family, too. In addition, the proposed assignment of the dd excitations of the green phase YBa<sub>2</sub>CuO<sub>5</sub> should be supported by a CuL<sub>3</sub> resonant X-ray scattering investigation.</p></sec><sec id="s6"><title>Acknowledgements</title><p>The author would like to thank colleague Prof. Bernd Lehmann for supporting this work by the donation of wonderful dioptase pieces from Altyn-Tyube, Kazakhstan. Also my teacher, the late Prof. Hugo Strunz, donated dioptase pieces from the Tsumeb mine, Namibia.</p></sec><sec id="s7"><title>Conflict of Interest</title><p>The author declares no conflict of interest.</p></sec><sec id="s8"><title>Cite this paper</title><p>Otto, H.H. (2017) Crystal Growth of Cu<sub>6</sub>(Ge,Si)<sub>6</sub>O<sub>18</sub>•6H<sub>2</sub>O and Assignment of UV-VIS Spectra in Comparison to Dehydrated Dioptase and Selected Cu(II) Oxo-Compounds Including Cuprates. World Journal of Condensed Matter Physics, 7, 57-79. https://doi.org/10.4236/wjcmp.2017.73006</p></sec><sec id="s9"><title>Supplemented Material</title><table-wrap id="table7" ><label><xref ref-type="table" rid="table7">Table 7</xref></label><caption><title> Comparison of scaling factors used for Cuprates in comparison to dioptase group compounds</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Scaling factor notation</th><th align="center" valign="middle" >Cuprates</th><th align="center" valign="middle" >Dioptase group</th><th align="center" valign="middle"  colspan="2"  >Ratio</th></tr></thead><tr><td align="center" valign="middle" ><sup><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x67.png" xlink:type="simple"/></inline-formula> </sup></td><td align="center" valign="middle" >1.755</td><td align="center" valign="middle" >1.733</td><td align="center" valign="middle"  colspan="2"  >1.013</td></tr><tr><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x68.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" >0.936</td><td align="center" valign="middle" >0.761</td><td align="center" valign="middle" >1.230</td><td align="center" valign="middle"  rowspan="3"  >1.243</td></tr><tr><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x69.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" >1.587</td><td align="center" valign="middle" >1.276</td><td align="center" valign="middle" >1.244</td></tr><tr><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800411x70.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" >2.180</td><td align="center" valign="middle" >1.738</td><td align="center" valign="middle" >1.254</td></tr></tbody></table></table-wrap></sec></body><back><ref-list><title>References</title><ref id="scirp.78598-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Ginetti, Y. 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