<?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">JAMP</journal-id><journal-title-group><journal-title>Journal of Applied Mathematics and Physics</journal-title></journal-title-group><issn pub-type="epub">2327-4352</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jamp.2015.312180</article-id><article-id pub-id-type="publisher-id">JAMP-61692</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>
 
 
  Thermal Properties and Phonon Dispersion of Bi&lt;sub&gt;2&lt;/sub&gt;Te&lt;sub&gt;3&lt;/sub&gt; and CsBi&lt;sub&gt;4&lt;/sub&gt;Te&lt;sub&gt;6&lt;/sub&gt; from First-Principles Calculations
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>hen</surname><given-names>Li</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Clas</surname><given-names>Persson</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref></contrib></contrib-group><aff id="aff2"><addr-line>Department of Physics, University of Oslo, Oslo, Norway</addr-line></aff><aff id="aff1"><addr-line>Department of Materials Science and Engineering, Royal Institute of Technology, Stockholm, Sweden</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>shenl@kth.se(HL)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>04</day><month>12</month><year>2015</year></pub-date><volume>03</volume><issue>12</issue><fpage>1563</fpage><lpage>1570</lpage><history><date date-type="received"><day>29</day>	<month>October</month>	<year>2015</year></date><date date-type="rev-recd"><day>accepted</day>	<month>1</month>	<year>December</year>	</date><date date-type="accepted"><day>4</day>	<month>December</month>	<year>2015</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>
 
 
  The narrow-gap semiconductor CsBi
  <sub>4</sub>Te
  <sub>6</sub> is a promising material for low temperature thermoelectric applications. Its thermoelectric property is significantly better than the well-explored, high-performance thermoelectric material Bi
  <sub>2</sub>Te
  <sub>3</sub> and related alloys. In this work, the thermal expansion and the heat capacity at constant pressure of CsBi
  <sub>4</sub>Te
  <sub>6</sub> are determined within the quasiharmonic approximation within the density functional theory. Comparisons are made with available experimental data, as well as with calculated and measured data for Bi
  <sub>2</sub>Te
  <sub>3</sub>. The phonon band structures and the partial density of states are also investigated, and we find that both CsBi
  <sub>4</sub>Te
  <sub>6</sub> and Bi
  <sub>2</sub>Te
  <sub>3</sub> exhibit localized phonon states at low frequencies. At high temperatures, the decrease of the volume expansion with temperature indicates the potential of a good thermal conductivity in this temperature region.
 
</p></abstract><kwd-group><kwd>Quasi Harmonic Approximation</kwd><kwd> Thermal Expansion</kwd><kwd> Heat Capacity</kwd><kwd> Phonon Dispersion</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>In the recent years, thermoelectric (TE) materials have been studied extensively due to the advances in the material synthesis and an improved device performance [<xref ref-type="bibr" rid="scirp.61692-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.61692-ref2">2</xref>] . Special attention has been paid on searching for new compounds, alloys, and/or nanostructures with higher thermoelectric performance. The efficiency of the thermoelectric materials can be evaluated from the figure of merit ZT = (S<sup>2</sup>/rk)∙T where T is the absolute temperature; S is the Seebeck coefficient; r is the electrical resistivity; and k is the thermal conductivity. k has contribution from the electronic k<sub>e</sub> and the lattice thermal k<sub>L</sub> conductivities [<xref ref-type="bibr" rid="scirp.61692-ref3">3</xref>] . The power factor S<sup>2</sup>/r defines the characterized electrical properties. A good thermoelectric material shall typically exhibit low thermal conductivity and a large power factor. In the past years, many research groups have reported enhanced ZT in superlattices such as the Bi<sub>2</sub>Te<sub>3</sub>/Sb<sub>2</sub>Te<sub>3</sub> systems, where the superlattice structures reduce the lattice thermal conductivity. Also, novel bulk and alloy compounds, such as antimony slivery telluride and its alloys with skutterudites, have shown improved ZT value which indicates that the materials can be suitable for thermoelectric applications. Bi<sub>2</sub>Te<sub>3</sub> is already a well-established thermoelectric material at room temperature. Incorporating Cs in Bi<sub>2</sub>Te<sub>3</sub> yields a somewhat more complex electronic structure, and this CsBi<sub>4</sub>Te<sub>6</sub> compound is a potentially thermoelectric material with ZT<sub>max</sub> = 0.8 at T = −23˚C, which thus is suitable for low temperatures.</p><p>All factors related to an optimized ZT are strongly influenced by the crystal structure, the electronic band structure, and the actual carrier concentration of the material. For the considered compounds (i.e., Bi<sub>2</sub>Te<sub>3</sub> and CsBi<sub>4</sub>Te<sub>6</sub>) several investigations of the electronic structure and the electronic conductivity have been reported; see for instance Refs. [<xref ref-type="bibr" rid="scirp.61692-ref4">4</xref>] -[<xref ref-type="bibr" rid="scirp.61692-ref8">8</xref>] . The electronic part k<sub>e</sub> of the thermal conductivity can be calculated from the electronic structure through the Wiedemann-Franz relation k<sub>e</sub> = L<sub>0</sub>T/r (where L<sub>0</sub> is the Lorenz number) but the corresponding lattice part k<sub>L</sub> cannot be calculated that easily. Analyzing the thermal properties makes it possible to at least better understand and describe the lattice part k<sub>L</sub> of thermal conductivity. In this study, we have therefore theoretically studied the thermal properties of Bi<sub>2</sub>Te<sub>3</sub> and CsBi<sub>4</sub>Te<sub>6</sub>. We have computed the thermal expansions, the heat capacities at constant pressure, and the isothermal bulk moduli at finite temperatures; this can serve as a help to understand the underlying mechanism for the low k<sub>L</sub> for these two compounds. The computational study is based on the density functional theory (DFT) within the quasi harmonic approximation (QHA), which is known to provide reasonable good description of the thermal properties below the melting point of bulk materials [<xref ref-type="bibr" rid="scirp.61692-ref9">9</xref>] -[<xref ref-type="bibr" rid="scirp.61692-ref11">11</xref>] . The phonon frequencies in the first Brillouin zone are calculated by means of the density functional perturbation theory (DFPT). Recently, QHA based on DFPT has successfully been employed for several related materials, such as Ti<sub>3</sub>SiC<sub>2</sub>, Al<sub>3</sub>Mg, Al<sub>3</sub>Sc, and GaN [<xref ref-type="bibr" rid="scirp.61692-ref12">12</xref>] -[<xref ref-type="bibr" rid="scirp.61692-ref14">14</xref>] .</p></sec><sec id="s2"><title>2. Computational Method</title><sec id="s2_1"><title>2.1. Theoretical Background</title><p>The most fundamental thermal properties of solids can be determined from the phonon dispersion ω<sub>q</sub><sub>,v</sub> (for wave vector q of the vth mode) and the corresponding phonon density of states (DOS) as a function of frequency. The Helmholtz free energy at the temperature T and for a constant volume V is given by <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-1720419x6.png" xlink:type="simple"/></inline-formula>, where E<sub>0</sub>(V) is the ground state total energy at T = 0 K, F<sub>ph</sub>(V,T) is the vibration free energy from the phonon contribution, and F<sub>el</sub>(V,T) is the free energy from the electronic excitations. From the phonon frequencies, the temperature dependent vibrational heat capacity C<sub>V</sub> at constant volume is determined through</p><disp-formula id="scirp.61692-formula14"><label>, (1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-1720419x7.png"  xlink:type="simple"/></disp-formula><p>where k<sub>B</sub> is the Boltzmann’s constant. The thermal properties at constant pressure are analyzed from the free energy F(V,T). For a given temperature T, the equilibrium volume V<sub>0</sub> is determined by minimizing the Gibbs free energy G(T,p) with respect to volume. This is utilized to further analyze the thermal properties, such as the thermal expansion ΔV/V<sub>0</sub>. The heat capacity at constant pressure is obtained from the derivative of G(T,p) as</p><disp-formula id="scirp.61692-formula15"><label>. (2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-1720419x8.png"  xlink:type="simple"/></disp-formula><p>Here, S(T,p) is the entropy of the system and V(T,p) is the equilibrium volume at a specific pressure p and</p><p>temperature T. Moreover, the thermal expansion coefficient is given by<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-1720419x9.png" xlink:type="simple"/></inline-formula>, and the bulk modulus at zero pressure is given by<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-1720419x10.png" xlink:type="simple"/></inline-formula>.</p></sec><sec id="s2_2"><title>2.2. Computational Details</title><p>The computational study is based on the first-principles DFT approach as implement in the VASP program package [<xref ref-type="bibr" rid="scirp.61692-ref15">15</xref>] [<xref ref-type="bibr" rid="scirp.61692-ref16">16</xref>] , employing the projector augmented wave method (PAW) and using the Perdew-Burke-Ern- zerhof (PBE) exchange-correlation functional [<xref ref-type="bibr" rid="scirp.61692-ref17">17</xref>] . We fully relax the structure parameter and volume V<sub>0</sub> of the primitive unit cell with a convergence of 10<sup>−5</sup> eV/cell for the total energy, and 10<sup>−4</sup> eV/&#197; for the forces on each atom. The energy cutoff was 500 eV. The k-space integration was performed with the tetrahedron method, involving a Γ-centered 10 &#215; 10 &#215; 10 k-mesh for Bi<sub>2</sub>Te<sub>3 </sub>and corresponding 4 &#215; 4 &#215; 4 k-mesh for the larger CsBi<sub>4</sub>Te<sub>6</sub> compound. QHA was employed to compute the thermal properties at constant pressure. The thermodynamic functions were fitted to the integral form of Vinet’s equation of state (EOS) at zero pressure [<xref ref-type="bibr" rid="scirp.61692-ref18">18</xref>] . The Helmholtz free energy and the Gibbs free energy were obtained from the minimum values of the thermodynamic functions at finite temperatures, whereupon the equilibrium volume and the bulk moduli were obtained through the EOS. The heat capacity C<sub>p</sub> (see, Equation (2)) was determined by a numerical differentiation ∂V/∂T and by polynomial fitting for both C<sub>V</sub> and S.</p><p>When calculating the phonon dispersion, we have employed the supercell approach and the force-constant method. The real space force constants of the supercells were calculated by the DFPT, whereupon the phonon modes were calculated from the force constants using the PHONOPY package [<xref ref-type="bibr" rid="scirp.61692-ref19">19</xref>] . Here, the phonon dispersions and the phonon DOS were calculated with a 2 &#215; 2 &#215; 2 supercell for Bi<sub>2</sub>Te<sub>3</sub> and a 1 &#215; 1 &#215; 2 supercell for CsBi<sub>4</sub>Te<sub>6</sub>, which implies 40 atoms and 88 atoms, respectively. In those calculations, 41 &#215; 41 &#215; 41 Monkhorst- Pack grids were used which is expected to be sufficient to avoid the mean relative error of the DOS.</p></sec></sec><sec id="s3"><title>3. Results</title><sec id="s3_1"><title>3.1. Crystal Structure</title><p>Bi<sub>2</sub>Te<sub>3</sub> is a semiconductor with a narrow band gap. Although its primitive unit cell has rhombohedral symmetry with the space group<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-1720419x11.png" xlink:type="simple"/></inline-formula>, the crystal structure is usually described by hexagonal coordinates. With a hexagonal unit cell [see <xref ref-type="fig" rid="fig1">Figure 1</xref>(a)], there are five layers consisting of Te(1)-Bi-Te(2)-Bi-Te(1) chains along the hexagonal axis. From our relaxation, we find that the calculated average bond length of Te-Te, Bi-Te(1), and Bi-Te(2) are 3.60, 3.06, and 3.22 &#197;, respectively. The crystalline structure of CsBi<sub>4</sub>Te<sub>6</sub> is related to that of Bi<sub>4</sub>Te<sub>6</sub>, however it crystallizes with the space group C2/m; see <xref ref-type="fig" rid="fig1">Figure 1</xref>(b). The layered structure of CsBi<sub>4</sub>Te<sub>6</sub> is composed by infinitely long anionic [Bi<sub>4</sub>Te<sub>6</sub>]<sup>−</sup> blocks with the Cs<sup>+</sup> ions reside between the anionic layers. The [Bi<sub>4</sub>Te<sub>6</sub>]<sup>−</sup> blocks can be seen as fragments of NaCl-like lattices, and each block is a two-Bi octahedral thick and four-Bi octahedral wide in the ac-plane while infinitely along the b-axis. The compound can be considered as a one-dimensional like</p><fig-group id="fig1"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> Crystal structure of (a) hexagonal layered Bi<sub>2</sub>Te<sub>3</sub> and (b) CsBi<sub>4</sub>Te<sub>6</sub>. The layered structure of CsBi<sub>4</sub>Te<sub>6</sub> is composed of anionic, infinitely long [Bi<sub>4</sub>Te<sub>6</sub>]<sup>−</sup> blocks where the Cs<sup>+</sup> ions are located between two anionic blocks. The main Bi-Bi bond in CsBi<sub>4</sub>Te<sub>6</sub> is indicated by the arrow.</title></caption><fig id ="fig1_1"><label>(b)</label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-1720419x12.png"/></fig><fig id ="fig1_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-1720419x13.png"/></fig></fig-group><p>crystal structure, and therefore the structure is strongly anisotropic. CsBi<sub>4</sub>Te<sub>6</sub> can be regarded as a reduced structure of Bi<sub>2</sub>Te<sub>3</sub>. From comparing the crystal structure of CsBi<sub>4</sub>Te<sub>6</sub> and Bi<sub>4</sub>Te<sub>6</sub> = 2(Bi<sub>2</sub>Te<sub>3</sub>) one finds that the additional electron per two formula units of Bi<sub>2</sub>Te<sub>3</sub> implies a complete reorganization of the Bi<sub>2</sub>Te<sub>3</sub> framework. Thereby, the extra valence electrons in CsBi<sub>4</sub>Te<sub>6</sub> localize on the Bi atoms which leads to a new formation along the a-axis with Bi-Bi bonds. Our calculated length of this Bi-Bi bond in CsBi<sub>4</sub>Te<sub>6</sub> is 3.23 &#197;, which is thus close to the bond length of Bi-Te(2) in Bi<sub>2</sub>Te<sub>3</sub>.</p></sec><sec id="s3_2"><title>3.2. Thermal Expansion, Bulk Modulus, and Heat Capacities</title><p><xref ref-type="table" rid="table1">Table 1</xref> summarizes the volume expansion ΔV/V<sub>0</sub>, thermal expansion coefficient a, as well as the heat capacities C<sub>p</sub> and C<sub>V</sub> of Bi<sub>2</sub>Te<sub>3 </sub>and CsBi<sub>4</sub>Te<sub>6</sub>; we present the results for the temperatures T = 300 and 600 K. The temperature dependence of the volume expansion for T = 0 - 900 K are shown in <xref ref-type="fig" rid="fig2">Figure 2</xref>. The volume expansion is defined as ΔV/V<sub>0</sub>, with ΔV = V − V<sub>0</sub> and where V<sub>0</sub> is the corresponding volume at T = 300 K, and by definition ΔV/V<sub>0</sub> is negative below this 300 K. The volume expansions of the two considered compounds have almost the same linear increase at low temperature (in the region 50 - 300 K), but this consistency disappeared for higher temperatures. This is obvious for temperatures above 400 K where Bi<sub>2</sub>Te<sub>3</sub> has somewhat larger volume expansion than CsBi<sub>4</sub>Te<sub>6</sub>.</p><p><xref ref-type="fig" rid="fig3">Figure 3</xref> displays the thermal expansion coefficient <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-1720419x14.png" xlink:type="simple"/></inline-formula> of Bi<sub>2</sub>Te<sub>3</sub> and CsBi<sub>4</sub>Te<sub>6</sub>. The results reveal that the thermal expansion increases considerably with increasing temperatures in the low temperature region below 170 K. In this region the two compounds have almost equivalent thermal expansion, which is in agreement with similar volume expansions for low temperatures. Moreover, the expansion coefficient reaches a maximum value of roughly 55 &#215; 10<sup>−5</sup> K<sup>−1</sup> for both Bi<sub>2</sub>Te<sub>3</sub> (maximum at T ~ 300 K) and CsBi<sub>4</sub>Te<sub>6</sub> (at T ~ 150 K). For higher</p><table-wrap id="table1" ><label><xref ref-type="table" rid="table1">Table 1</xref></label><caption><title> The volume expansion ΔV/V<sub>0</sub>, the thermal expansion coefficient a, and the heat capacities C<sub>p</sub> and C<sub>V</sub> of Bi<sub>2</sub>Te<sub>3</sub> and CsBi<sub>4</sub>Te<sub>6</sub> at the temperatures T = 300 and 600 K. The unit J∙mol<sup>−1</sup>∙K<sup>−1</sup> for the heat capacities refers to formula unit cell: 40 atoms for Bi<sub>2</sub>Te<sub>3</sub> and 88 atoms for CsBi<sub>4</sub>Te<sub>6</sub></title></caption><table><tbody><thead><tr><th align="center" valign="middle"  rowspan="2"  ></th><th align="center" valign="middle"  colspan="2"  >Bi<sub>2</sub>Te<sub>3</sub></th><th align="center" valign="middle"  colspan="2"  >CsBi<sub>4</sub>Te<sub>6</sub></th></tr></thead><tr><td align="center" valign="middle" >300 K</td><td align="center" valign="middle" >600 K</td><td align="center" valign="middle" >300 K</td><td align="center" valign="middle" >600 K</td></tr><tr><td align="center" valign="middle" >ΔV/V<sub>0</sub></td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.017</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.014</td></tr><tr><td align="center" valign="middle" >a [10<sup>−5</sup> K<sup>−1</sup>]</td><td align="center" valign="middle" >55</td><td align="center" valign="middle" >54</td><td align="center" valign="middle" >52</td><td align="center" valign="middle" >39</td></tr><tr><td align="center" valign="middle" >C<sub>p</sub> [J∙mol<sup>−1</sup>∙K<sup>−1</sup>]</td><td align="center" valign="middle" >126</td><td align="center" valign="middle" >131</td><td align="center" valign="middle" >280</td><td align="center" valign="middle" >285</td></tr><tr><td align="center" valign="middle" >C<sub>V</sub> [J∙mol<sup>−1</sup>∙K<sup>−1</sup>]</td><td align="center" valign="middle" >121</td><td align="center" valign="middle" >123</td><td align="center" valign="middle" >271</td><td align="center" valign="middle" >273</td></tr></tbody></table></table-wrap><fig id="fig2"  position="float"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> Relative volume expansion ΔV/V<sub>0</sub> as a function of temperature T, where V<sub>0</sub> is the corresponding volume at T = 300 K (figure caption)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-1720419x15.png"/></fig><fig id="fig3"  position="float"><label><xref ref-type="fig" rid="fig3">Figure 3</xref></label><caption><title> Thermal expansion coefficient α of Bi<sub>2</sub>Te<sub>3</sub> and CsBi<sub>4</sub>Te<sub>6</sub> as function of temperature. The dashed line indicates the temperature T = 230 K where the expansion coefficients are equal for the two compounds</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-1720419x16.png"/></fig><p>temperatures, the thermal expansion of Bi<sub>2</sub>Te<sub>3</sub> is significantly larger than that of CsBi<sub>4</sub>Te<sub>6</sub>. Moreover, whereas the expansion coefficient of Bi<sub>2</sub>Te<sub>3</sub> tends to be rather stable at ~(50 - 55) &#215; 10<sup>−5</sup> K<sup>−1</sup> for high temperatures, the corresponding coefficient of CsBi<sub>4</sub>Te<sub>6</sub> drops almost linearly to about half its maximum value, that is, from ~57 &#215; 10<sup>−5</sup> K<sup>−1</sup> to ~28 &#215; 10<sup>−5</sup> K<sup>−1</sup> at T = 900 K.</p><p>It is noticeable that for many similar compounds the thermal expansion coefficient is increasing with increasing temperature. However, for Bi<sub>2</sub>Te<sub>3</sub> we thus find a rather constant (and slightly decreasing) expansion coefficient, and for CsBi<sub>4</sub>Te<sub>6</sub>, we observe a strong decrease of the expansion coefficient in the high temperature region. This is a direct consequence of the decrease of the volume expansion slope for large T for CsBi<sub>4</sub>Te<sub>6</sub>; see <xref ref-type="fig" rid="fig2">Figure 2</xref>.</p><p>The bulk modulus is determined from the EOS calculation, and the resulting values for T = 0 K are B<sub>0</sub> = 47.8 GPa for Bi<sub>2</sub>Te<sub>3</sub> and 37.8 GPa for CsBi<sub>4</sub>Te<sub>6</sub>. Thus, we find that the bulk modulus of Bi<sub>2</sub>Te<sub>3</sub> is about 25% larger than that of CsBi<sub>4</sub>Te<sub>6</sub>.</p><p>The heat capacities C<sub>V</sub> and C<sub>p</sub> are investigated directly from the phonon frequency dispersion using the QHA approach, and the resulting C<sub>V</sub> and C<sub>p</sub> for Bi<sub>2</sub>Te<sub>3</sub> and CsBi<sub>4</sub>Te<sub>6</sub> are presented in <xref ref-type="fig" rid="fig4">Figure 4</xref>. We find that the two compounds have very similar heat capacities. C<sub>p</sub> is roughly 3% - 4% larger than C<sub>V</sub> at T = 300 K and 4% - 7% larger at T = 600 K (<xref ref-type="table" rid="table1">Table 1</xref>). Moreover, C<sub>p</sub> and C<sub>V</sub> for both Bi<sub>2</sub>Te<sub>3</sub> and CsBi<sub>4</sub>Te<sub>6</sub> obey the law of T<sup>3</sup> behavior at low temperatures. At high temperatures however, C<sub>V</sub> reaches a constant value which is approximately given by the classic equipartition law <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-1720419x17.png" xlink:type="simple"/></inline-formula> where N is the number of atoms of the considered system. Here, N = 5 for Bi<sub>2</sub>Te<sub>3</sub> and 11 for CsBi<sub>4</sub>Te<sub>6</sub>, yielding <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-1720419x18.png" xlink:type="simple"/></inline-formula> and 281.2 J∙mol<sup>−1</sup>∙K<sup>−1</sup>, respectively, in the classical limit. At ambient pressure and at room temperature T = 300 K, the calculated value of C<sub>p</sub> for Bi<sub>2</sub>Te<sub>3</sub> is 126 J∙mol<sup>−1</sup>∙K<sup>−1</sup> (<xref ref-type="table" rid="table1">Table 1</xref>) which agree with the experimental data 126 J∙mol<sup>−1</sup>∙K<sup>−1</sup> [<xref ref-type="bibr" rid="scirp.61692-ref20">20</xref>] [<xref ref-type="bibr" rid="scirp.61692-ref21">21</xref>] . We find also that the calculated results fit very well with the experimental data [<xref ref-type="bibr" rid="scirp.61692-ref20">20</xref>] [<xref ref-type="bibr" rid="scirp.61692-ref21">21</xref>] in the whole low temperature region apart from the measure data point for the lowest temperature; see <xref ref-type="fig" rid="fig4">Figure 4</xref>. The corresponding calculated C<sub>p</sub> value at T = 300 K for CsBi<sub>4</sub>Te<sub>6</sub> is 280 J∙mol<sup>−1</sup>∙K<sup>−1</sup>. This is roughly twice as large value compared with Bi<sub>2</sub>Te<sub>3</sub>, and the reason is that the unit cell of CsBi<sub>4</sub>Te<sub>6</sub> contains roughly twice as many atoms (88 atoms) as in the unit cell of Bi<sub>2</sub>Te<sub>3</sub> (40 atoms) and the mol<sup>−1</sup> describes formula unit cell. In the units of J∙kg<sup>−1</sup>∙K<sup>−1</sup>, the corresponding value is C<sub>p</sub> = 391 J∙kg<sup>−1</sup>∙K<sup>−1</sup> for Bi<sub>2</sub>Te<sub>3</sub> and 400 J∙kg<sup>−1</sup>∙K<sup>−1</sup> for CsBi<sub>4</sub>Te<sub>6</sub>.</p></sec><sec id="s3_3"><title>3.3. Phonon Dispersion and Phonon Density of States</title><p>The dispersion curves for Bi<sub>2</sub>Te<sub>3</sub> and CsBi<sub>4</sub>Te<sub>6</sub> are shown along the high symmetry directions in their respective Brillouin zones (<xref ref-type="fig" rid="fig5">Figure 5</xref>). For Bi<sub>2</sub>Te<sub>3</sub>, the atom-resolved DOS reveals that the phonon states in the lower energy</p><fig id="fig4"  position="float"><label><xref ref-type="fig" rid="fig4">Figure 4</xref></label><caption><title> The heat capacity at constant pressure C<sub>p</sub> and the heat capacity at constant volume C<sub>V</sub> as functions of temperature. The curves of C<sub>V</sub> follow roughly the T<sup>3</sup>-law at low temperature and tend to be fairly constant at higher temperatures. Here, the unit J∙mol<sup>−1</sup>∙K<sup>−1</sup> refers to formula unit cell, and due to a larger unit cell the values of the heat capacity of CsBi<sub>4</sub>Te<sub>6</sub> is about 2.2 times larger than of Bi<sub>2</sub>Te<sub>3</sub></title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-1720419x19.png"/></fig><fig-group id="fig5"><label><xref ref-type="fig" rid="fig5">Figure 5</xref></label><caption><title> Phonon band structure and its corresponding total and atomic-resolved DOS of (a) Bi<sub>2</sub>Te<sub>3</sub> and (b) CsBi<sub>4</sub>Te<sub>6</sub>. The difference in the frequency at the Brillouin zone edge (1.12 THz for Bi<sub>2</sub>Te<sub>3</sub> whereas 0.76 THz for CsBi<sub>4</sub>Te<sub>6</sub>) is due to the Cs atoms in CsBi<sub>4</sub>Te<sub>6</sub> which have atomic mass between that of Bi and Te. The CsBi<sub>4</sub>Te<sub>6</sub> structure implies also the presence of Bi-Bi bond (see <xref ref-type="fig" rid="fig1">Figure 1</xref>).</title></caption><fig id ="fig5_1"><label> (b)</label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-1720419x20.png"/></fig><fig id ="fig5_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-1720419x21.png"/></fig></fig-group><p>region compose mainly of Bi-like states, while Te-like states contribute more in the higher energy region since the atomic mass of Te is significantly lighter than that of Bi.</p><p>When comparing the phonon dispersions of atomic-resolved DOS of Bi<sub>2</sub>Te<sub>3</sub> [<xref ref-type="fig" rid="fig5">Figure 5</xref>(a)] with CsBi<sub>4</sub>Te<sub>6</sub> [<xref ref-type="fig" rid="fig5">Figure 5</xref>(b)], it is clear the shapes of the dispersions and DOS of Bi<sub>2</sub>Te<sub>3</sub> and CsBi<sub>4</sub>Te<sub>6</sub> shows both similarities and differences. The flat regions of phonon dispersion curves in Bi<sub>2</sub>Te<sub>3</sub> lead to two main peaks in the atom-re- solved DOS indicating localizations of states that behave as the “atomic states” for Bi and Te atoms, respectively. Similar atom-like characters were also found in the atom-resolved DOS of CsBi<sub>4</sub>Te<sub>6</sub> for the Cs and Te atoms, whereas the Bi atoms show more delocalization in CsBi<sub>4</sub>Te<sub>6</sub> because the Bi-Bi bonds are influenced by the Cs<sup>+</sup>.</p><p>The acoustic modes in Bi<sub>2</sub>Te<sub>3</sub> are rather disperse up to 1.12 THz and they depend primarily the Bi atoms, while the acoustic modes in CsBi<sub>4</sub>Te<sub>6</sub> are disperse up to 0.76 THz and involve mainly contribution from the Cs atoms. It has been discussed that the low frequency phonons as a function of temperature play an important role in the thermal expansion [<xref ref-type="bibr" rid="scirp.61692-ref22">22</xref>] .</p><p>In Bi<sub>2</sub>Te<sub>3</sub>, the phonon dispersion with frequencies lower than 1.7 THz is a mixture between acoustic and optical modes, and these phonons contribute significantly to the thermal expansion below 300 K. CsBi<sub>4</sub>Te<sub>6</sub> on the other hand, shows relatively delocalized states in the whole phonon dispersion curve because the Cs atom is rather different from Bi. The differences in the phonon vibration modes are mainly due to the different crystal symmetry and the distribution of atom mass in Bi<sub>2</sub>Te<sub>3</sub> and CsBi<sub>4</sub>Te<sub>6</sub>, which also lead to the different in the thermal expansions as shown in <xref ref-type="fig" rid="fig3">Figure 3</xref>.</p></sec></sec><sec id="s4"><title>4. Conclusion</title><p>In this work, the thermal properties and the phonon dispersions of Bi<sub>2</sub>Te<sub>3</sub> and CsBi<sub>4</sub>Te<sub>6</sub> have been calculated, employing the DFT and the DFPT within the quasi-harmonic approximation. The volume expansions of these two compounds have similar linear increase for temperatures below 300 K, and Bi<sub>2</sub>Te<sub>3</sub> has slightly larger volume expansion than CsBi<sub>4</sub>Te<sub>6</sub> for temperatures above 300 K. However, both compounds show a decrease of the volume expansion in the high temperature region. For Bi<sub>2</sub>Te<sub>3</sub> the calculated value of C<sub>p</sub> is 126 J∙mol<sup>−1</sup>∙K<sup>−1</sup> at ambient pressure and room temperature which supports the experimental data. From the calculated phonon dispersion and phonon DOS, we conclude that CsBi<sub>4</sub>Te<sub>6</sub> has relatively delocalized states in the phonon dispersion curve due to the Cs atomic mass which is between those of Bi and Te.</p></sec><sec id="s5"><title>Acknowledgements</title><p>This work is supported by the European EM-ECW scholarship program Tandem, the Swedish Energy Agency, and the Swedish Research Council. C.P. acknowledges support from the Research Council of Norway (contracts No. 228854 and 221469). We acknowledge access to the high-performance computing resources at the NSC and HPC2N centers through SNIC and Matter network.</p></sec><sec id="s6"><title>Cite this paper</title><p>ShenLi,ClasPersson, (2015) Thermal Properties and Phonon Dispersion of Bi<sub>2</sub>Te<sub>3</sub> and CsBi<sub>4</sub>Te<sub>6</sub> from First-Principles Calculations. Journal of Applied Mathematics and Physics,03,1563-1570. doi: 10.4236/jamp.2015.312180</p></sec></body><back><ref-list><title>References</title><ref id="scirp.61692-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Chung, D.Y., Hogan, T., Brazis, P., Rocci-Lane, M., Kannewurf, C., Bastea, M., Uher, C. and Kanatzidis, M.G. (2000) CsBi4Te6: A High-Performance Thermoelectric Material for Low-Temperature Applications. Science, 287, 1024.http://dx.doi.org/10.1126/science.287.5455.1024</mixed-citation></ref><ref id="scirp.61692-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">Youn, S.J. and Freeman, A.J. (2001) First-Principles Electronic Structure and Its Relation to Thermoelectric Properties of Bi2Te3. Physical Review B, 63, Article ID: 085112. http://dx.doi.org/10.1103/PhysRevB.63.085112</mixed-citation></ref><ref id="scirp.61692-ref3"><label>3</label><mixed-citation publication-type="other" xlink:type="simple">Tritt, T.M. (1999) Holey and Unholey Semiconductors. Science, 283, 804. http://dx.doi.org/10.1126/science.283.5403.804</mixed-citation></ref><ref id="scirp.61692-ref4"><label>4</label><mixed-citation publication-type="other" xlink:type="simple">Sofo, J.O. and Mahan, G.D. (1998) Electronic Structure of CoSb3: A Narrow-Band-Gap Semiconductor. Physical Review B, 58, 15620. http://dx.doi.org/10.1103/PhysRevB.58.15620</mixed-citation></ref><ref id="scirp.61692-ref5"><label>5</label><mixed-citation publication-type="other" xlink:type="simple">Bell, L.E. (2008) Cooling, Heating, Generating Power, and Recovering Waste Heat with Thermoelectric Systems. Science, 321, 1457. http://dx.doi.org/10.1126/science.1158899</mixed-citation></ref><ref id="scirp.61692-ref6"><label>6</label><mixed-citation publication-type="other" xlink:type="simple">Katsuki, S. (1969) The Band Structure of Bismuth Telluride. Journal of the Physical Society of Japan, 26, 58.http://dx.doi.org/10.1143/JPSJ.26.58</mixed-citation></ref><ref id="scirp.61692-ref7"><label>7</label><mixed-citation publication-type="other" xlink:type="simple">Larson, P., Mahanti, S.D., Chung, D.-Y. and Kanatzidis, M.G. (2002) Electronic Structure of CsBi4Te6: A High-Performance Thermoelectric at Low Temperatures. Physical Review B, 65, 45205. http://dx.doi.org/10.1103/PhysRevB.65.045205</mixed-citation></ref><ref id="scirp.61692-ref8"><label>8</label><mixed-citation publication-type="other" xlink:type="simple">Lykke, L., Iversen, B.B. and Madesen, G.K.H. (2006) Electronic Structure and Transport in the Low-Temperature Thermoelectric CsBi4Te6: Semiclassical Transport Equations. Physical Review B, 73, Article ID: 195121.http://dx.doi.org/10.1103/PhysRevB.73.195121</mixed-citation></ref><ref id="scirp.61692-ref9"><label>9</label><mixed-citation publication-type="other" xlink:type="simple">Biernacki, S. and Scheffler, M. (1989) Negative Thermal Expansion of Diamond and Zinc-Blende Semiconductors. Physical Review Letters, 63, 290. http://dx.doi.org/10.1103/PhysRevLett.63.290</mixed-citation></ref><ref id="scirp.61692-ref10"><label>10</label><mixed-citation publication-type="other" xlink:type="simple">Pavone, P., Karch, K., Schutt, O., Strauch, D., Windl, W., Giannozzi, P. and Baroni S. (1993) Ab Initio Lattice Dynamics of Diamond. Physical Review B, 48, 3156. http://dx.doi.org/10.1103/PhysRevB.48.3156</mixed-citation></ref><ref id="scirp.61692-ref11"><label>11</label><mixed-citation publication-type="other" xlink:type="simple">Nie, Y.Z. and Xie, Y.Q. (2007) Ab Initio Thermodynamics of the HCP Metals Mg, Ti, and Zr. Physical Review B, 75, Article ID: 174117. http://dx.doi.org/10.1103/PhysRevB.75.174117</mixed-citation></ref><ref id="scirp.61692-ref12"><label>12</label><mixed-citation publication-type="other" xlink:type="simple">Togo, A., Chaput, L., Tanaka, I. and Hug, G. (2010) First-Principles Phonon Calculations of Thermal Expansion in Ti3SiC2, Ti3AlC2, and Ti3GeC2. Physical Review B, 81, Article ID: 174301.http://dx.doi.org/10.1103/PhysRevB.81.174301</mixed-citation></ref><ref id="scirp.61692-ref13"><label>13</label><mixed-citation publication-type="other" xlink:type="simple">Li, D.-L., Chen, P., Yi, J.-X., Tang, B.-Y., Peng, L.-M. and Ding, W.-J. (2009) Ab Initio Study on the Thermal Properties of the FCC Al3Mg and Al3Sc Alloys. Journal of Physics D: Applied Physics, 42, Article ID: 225407.http://dx.doi.org/10.1088/0022-3727/42/22/225407</mixed-citation></ref><ref id="scirp.61692-ref14"><label>14</label><mixed-citation publication-type="other" xlink:type="simple">Xu, L.-C., Wang, R.-Z., Yang, X.-D. and Yan, H. (2011) Thermal Expansions in Wurtzite AlN, GaN, and InN: First-Principle Phonon Calculations. Journal of Applied Physics, 110, Article ID: 043528.http://dx.doi.org/10.1063/1.3627237</mixed-citation></ref><ref id="scirp.61692-ref15"><label>15</label><mixed-citation publication-type="other" xlink:type="simple">Kresse, G. and Hafner, J. (1993) Ab Initio Molecular Dynamics for Liquid Metals. Physical Review B, 47, 558-561.http://dx.doi.org/10.1103/PhysRevB.47.558</mixed-citation></ref><ref id="scirp.61692-ref16"><label>16</label><mixed-citation publication-type="other" xlink:type="simple">Kresse, G. and Furthmüller, J. (1996) Efficient Iterative Schemes for ab Initio Total-Energy Calculations Using a Plane-Wave Basis Set. Physical Review B, 54, 11169-11186. http://dx.doi.org/10.1103/PhysRevB.54.11169</mixed-citation></ref><ref id="scirp.61692-ref17"><label>17</label><mixed-citation publication-type="other" xlink:type="simple">Perdew, J.P., Burke, K. and Ernzerhof, M. (1996) Generalized Gradient Approximation Made Simple. Physical Review Letters, 77, 3865-3868. http://dx.doi.org/10.1103/PhysRevLett.77.3865</mixed-citation></ref><ref id="scirp.61692-ref18"><label>18</label><mixed-citation publication-type="other" xlink:type="simple">Vinet, P., Rose, J.H., Ferrante, J. and Smith, J.R. (1989) Universal Features of the Equation of State of Solids. Journal of Physics: Condensed Matter, 1, 1941-1963. http://dx.doi.org/10.1088/0953-8984/1/11/002</mixed-citation></ref><ref id="scirp.61692-ref19"><label>19</label><mixed-citation publication-type="other" xlink:type="simple">Togo, A., Oba, F. and Tanaka, I. (2008) First-Principles Calculations of the Ferroelastic Transition between Rutile-Type and CaCl2-Type SiO2 at High Pressures. Physical Review B, 78, Article ID: 134106.http://dx.doi.org/10.1103/PhysRevB.78.134106</mixed-citation></ref><ref id="scirp.61692-ref20"><label>20</label><mixed-citation publication-type="other" xlink:type="simple">Pavlova, L.M., Shtern, Y.I. and Mironov, R.E. (2011) Thermal Expansion of Bismuth Telluride. High Temperature, 49, 369-379. http://dx.doi.org/10.1134/S0018151X1103014X</mixed-citation></ref><ref id="scirp.61692-ref21"><label>21</label><mixed-citation publication-type="other" xlink:type="simple">Gorbachuk, N.P., Bolgar, A.S., Sidorko, V.R. and Goncharuk, L.V. (2004) Heat Capacity and Enthalpy of Bi2Si3 and Bi2Te3 in the Temperature Range 58-1012 K. Powder Metallurgy and Metal Ceramics, 43, 284-290.http://dx.doi.org/10.1023/B:PMMC.0000042464.28118.a3</mixed-citation></ref><ref id="scirp.61692-ref22"><label>22</label><mixed-citation publication-type="other" xlink:type="simple">Zwanziger, J.W. (2007) Phonon Dispersion and Grüneisen Parameters of Zinc Dicyanide and Cadmium Dicyanide from First Principles: Origin of Negative Thermal Expansion. Physical Review B, 76, Article ID: 052102.http://dx.doi.org/10.1103/physrevb.76.052102</mixed-citation></ref></ref-list></back></article>