Electronic structure, phonon spectra and electron–phonon interaction in ScB₂

The electronic structure, Fermi surface, angle dependence of the cyclotron masses and extremal cross sections of the Fermi surface, phonon spectra, electron–phonon Eliashberg and transport spectral functions, temperature dependence of electrical resistivity of the ScB₂ diboride were investigated fro...

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spelling irk-123456789-1186692017-05-31T03:03:12Z Electronic structure, phonon spectra and electron–phonon interaction in ScB₂ Sichkar, S.M. Antonov, V.N. Электронные свойства проводящих систем The electronic structure, Fermi surface, angle dependence of the cyclotron masses and extremal cross sections of the Fermi surface, phonon spectra, electron–phonon Eliashberg and transport spectral functions, temperature dependence of electrical resistivity of the ScB₂ diboride were investigated from first principles using the fully re-lativistic and full potential linear muffin-tin orbital methods. The calculations of the dynamic matrix were carried out within the framework of the linear response theory. A good agreement with experimental data of electron–phonon spectral functions, electrical resistivity, cyclotron masses and extremal cross sections of the Fermi sur-face was achieved. 2013 Article Electronic structure, phonon spectra and electron–phonon interaction in ScB₂ / S.M. Sichkar, V.N. Antonov // Физика низких температур. — 2013. — Т. 39, № 7. — С. 771–779. — Бібліогр.: 40 назв. — англ. 0132-6414 PACS: 75.50.Cc, 71.20.Lp, 71.15.Rf http://dspace.nbuv.gov.ua/handle/123456789/118669 en Физика низких температур Фізико-технічний інститут низьких температур ім. Б.І. Вєркіна НАН України
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
language English
topic Электронные свойства проводящих систем
Электронные свойства проводящих систем
spellingShingle Электронные свойства проводящих систем
Электронные свойства проводящих систем
Sichkar, S.M.
Antonov, V.N.
Electronic structure, phonon spectra and electron–phonon interaction in ScB₂
Физика низких температур
description The electronic structure, Fermi surface, angle dependence of the cyclotron masses and extremal cross sections of the Fermi surface, phonon spectra, electron–phonon Eliashberg and transport spectral functions, temperature dependence of electrical resistivity of the ScB₂ diboride were investigated from first principles using the fully re-lativistic and full potential linear muffin-tin orbital methods. The calculations of the dynamic matrix were carried out within the framework of the linear response theory. A good agreement with experimental data of electron–phonon spectral functions, electrical resistivity, cyclotron masses and extremal cross sections of the Fermi sur-face was achieved.
format Article
author Sichkar, S.M.
Antonov, V.N.
author_facet Sichkar, S.M.
Antonov, V.N.
author_sort Sichkar, S.M.
title Electronic structure, phonon spectra and electron–phonon interaction in ScB₂
title_short Electronic structure, phonon spectra and electron–phonon interaction in ScB₂
title_full Electronic structure, phonon spectra and electron–phonon interaction in ScB₂
title_fullStr Electronic structure, phonon spectra and electron–phonon interaction in ScB₂
title_full_unstemmed Electronic structure, phonon spectra and electron–phonon interaction in ScB₂
title_sort electronic structure, phonon spectra and electron–phonon interaction in scb₂
publisher Фізико-технічний інститут низьких температур ім. Б.І. Вєркіна НАН України
publishDate 2013
topic_facet Электронные свойства проводящих систем
url http://dspace.nbuv.gov.ua/handle/123456789/118669
citation_txt Electronic structure, phonon spectra and electron–phonon interaction in ScB₂ / S.M. Sichkar, V.N. Antonov // Физика низких температур. — 2013. — Т. 39, № 7. — С. 771–779. — Бібліогр.: 40 назв. — англ.
series Физика низких температур
work_keys_str_mv AT sichkarsm electronicstructurephononspectraandelectronphononinteractioninscb2
AT antonovvn electronicstructurephononspectraandelectronphononinteractioninscb2
first_indexed 2025-07-08T14:25:19Z
last_indexed 2025-07-08T14:25:19Z
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fulltext Low Temperature Physics/Fizika Nizkikh Temperatur, 2013, v. 39, No. 7, pp. 771–779 Electronic structure, phonon spectra and electron–phonon interaction in ScB2 S.M. Sichkar1 and V.N. Antonov1,2 1Institute of Metal Physics, 36 Vernadsky Str., 03680 Kiev-142, Ukraine 2Ames Laboratory, U.S. Department of Energy, Ames, Iowa 50011, USA E-mail: antonov@imp.kiev.ua Received February 11, 2013, revised March 1, 2013 The electronic structure, Fermi surface, angle dependence of the cyclotron masses and extremal cross sections of the Fermi surface, phonon spectra, electron–phonon Eliashberg and transport spectral functions, temperature dependence of electrical resistivity of the ScB2 diboride were investigated from first principles using the fully re- lativistic and full potential linear muffin-tin orbital methods. The calculations of the dynamic matrix were carried out within the framework of the linear response theory. A good agreement with experimental data of electron– phonon spectral functions, electrical resistivity, cyclotron masses and extremal cross sections of the Fermi sur- face was achieved. PACS: 75.50.Cc Other ferromagnetic metals and alloys; 71.20.Lp Intermetallic compounds; 71.15.Rf Relativistic effects. Keywords: diborides, superconductivity, Fermi surface. 1. Introduction The discovery of superconductivity in MgB2 at 39 K by Akimitsu [1] has lead to booming activity in the phys- ics community and activated a search for superconductivi- ty in other diborides. Natural candidates for this search are AB2-type light metal diborides (A = Li, Be, Al). However, up to now superconductivity has not been reported in the majority of these compounds [2]. Only very recently su- perconductivity below 1 K (Tc = 0.72 K) has been re- ported in BeB2.75 [3]. According to Ref. 4 no supercon- ducting transition down to 0.42 K has been observed in powders of diborides of transition metals (M = Ti, Zr, Hf, V, Cr, Mo, U). NbB2 is expected to superconduct with a rather low transition temperature (< 1 K), and contradicto- ry reports about superconductivity up to Tc = 9.5 K in TaB2 can be found in Ref. 4. For ScB2 only low- temperature superconductivity was found with Tc ~ 1.5 K [5]. Finally, the reported Tc = 7 K in ZrB2 encourages further studies of these diborides [2]. Quite a number of theoretical studies of the electronic properties of the diborides are known to date [6–23]. Iva- novskii et al. [9] performed full potential linear muffin-tin orbital (FP-LMTO) calculations of all hexagonal diborides of 3d (Sc, Ti, ..., Fe), 4d (Y, Zr, ..., Ru), and 5d (La, Hf, ..., Os) metals and analyzed the variations in their chemical stability and some other properties (e.g., melting tempera- tures, enthalpies of formation). They found that the evolu- tion of their band structures can be described within a ri- gid-band model. For M = Ti, Zr, Hf energy Fermi ( )Fε falls near the density of state (DOS) minimum (pseudogap) between the fully occupied bonding bands and unoccupied antibonding bands. Sc, Y, La diborides have partially un- occupied bonding bands. Vajeeston et al. [11] investigated the electronic structure and ground state properties of AlB2 type transition metal diborides MB2 (M = Sc, Ti, V, Cr, Mn, Fe, Y, Zr, Nb, Mo, Hf, Ta) using the self consistent tight-binding linear muffin-tin orbital method. The equili- brium volume, bulk moduli, pressure derivative of bulk moduli, cohesive energy, heat of formation, and electronic specific heat coefficient were calculated for these systems and compared with the available experimental and other theoretical results. The bonding nature of these diborides was analyzed via the density of states histogram as well as the charge density plots, and the chemical stability was analyzed using the band filling principle. The variation in the calculated cohesive properties of these materials was correlated with the band filling effect. The existence of a pseudogap in the total density of states was found to be a common feature for all these compounds. The reason for the creation of the pseudogap was found to be due to the strong covalent interaction between boron p states. Fedor- © S.M. Sichkar and V.N. Antonov, 2013 S.M. Sichkar and V.N. Antonov chenko and Grechnev with coauthors [13,14] measured the temperature dependences of the magnetic susceptibility χ and its anisotropy = ⊥∆χ χ −χ  for single crystals of tran- sition-metal diborides MB2 (M = Sc, Ti, V, Zr, Hf) in the temperature interval 4.2–300 K. A transition into the su- perconducting state was not found in any of the diborides studied, right down to liquid-helium temperature. It was found that the anisotropy is weakly temperature- dependent, a nonmonotonic function of the filling of the hybridized p–d conduction band. First-principles calcula- tions of the electronic structure of diborides and the values of the paramagnetic contributions spin and Van Vleck to their susceptibility show that the behavior of the magnetic anisotropy is due to the competition between Van Vleck paramagnetism and orbital diamagnetism of the conduction electrons. Duan et al. [23] calculated elastic constants of 24 compounds of the AlB2-type diborides including ScB2 by first-principles with the generalized gradient approximation using the Voigt–Reuss–Hill averaging scheme. Values of all independent elastic constants as well as bulk modulus in a and c directions were predicted. It was founded that AlB2 is more ductile while ScB2 is more brittle, and AlB2 has a highest elastic anisotropy in the 24 AlB2-type compounds. Deligoz et al. [15] investigated the structural and lattice dy- namical properties of MB2 (M = Sc, V, Ti) using first- principles total energy calculations. Specifically, the lattice parameters (a, c) of the stable phase, the bond lengths of M–B and B–B atoms, phonon dispersion curves and the corresponding density of states, and some thermodynami- cal quantities such as internal energy, entropy, heat capaci- ty, and their temperature-dependent behaviors, were pre- sented. The obtained results for structural parameters are in a good agreement with the available experimental data. Zhang et al. [19] presented extensive structure searches to uncover the high-pressure structures of MB2 (M = Sc, Ti, Y, and Zr) up to 300 GPa using the ab initio evolutionary algorithm [24]. They show that ZrB2 persists up to 300 GPa within an ambient-pressure AlB2-type structure, while pressure-induced transitions into monoclinic phases (C2/m, Z = 4) occur for ScB2 at 208 GPa and YB2 at 163 GPa. A tetragonal R-ThSi2 structure (I41/amd, Z = 4) for TiB2 at 215 GPa was predicted. The phase transforma- tion mechanism has been discussed. The properties of the Fermi surface of ScB2, ZrB2, and HfB2 single crystals were studied by Pluzhnikov et al. [25] using the de Haas–van Alphen effect. The angular depen- dences of the frequencies of the dHvA oscillations in the planes (1010), (1120), and (0001) and the values of their effective cyclotron masses were measured. The frequen- cies of the oscillations in ScB2 found lie in the interval (2.09–23.6)⋅102 T and the measured cyclotron masses lie in the range (0.26–0.87)m0. Despite a lot of publications, there are still many open questions related to the electronic structure and physical properties of ScB2 diboride. The theoretical efforts were devoted mostly to the lattice and mechanical properties of ScB2. There is no theoretical explanation of the Fermi sur- face as well as angle dependence of the cyclotron masses and extremal cross sections of the Fermi surface, electron– phonon interaction and electrical resistivity in ScB2. The aim of this work is a complex investigation of the electron- ic structure, Fermi surface, angle dependence of the cyclo- tron masses and extremal cross sections of the Fermi sur- face, phonon spectra, electron–phonon Eliashberg and transport spectral functions, and temperature dependence of electrical resistivity of the ScB2 diboride. The paper is organized as follows. Section 2 presents the details of the calculations. Section 3 is devoted to the electronic structure as well as the Fermi surface, angle de- pendence of the cyclotron masses and extremal cross sec- tions of the Fermi surface, phonon spectra, electron– phonon interaction and electrical resistivity using the fully relativistic and full potential LMTO band structure me- thods. The results are compared with available experimen- tal data. Finally, the results are summarized in Sec. 4. 2. Computational details Most known transition-metal (M) diborides MB2 are formed by group III–VI transition elements (Sc, Ti, Zr, Hf, V, Nb, and others) and have a layered hexagonal C32 structure of the AlB2-type with the space group symmetry 6/P mmm (number 191). It is simply a hexagonal lattice in which closely-packed transition metal layers alternating with graphite-like B layers (Fig. 1). These diborides cannot be exactly layered compounds because the interlayer inte- raction is strong even though the M layers alternate with the B layers in their crystal structure. The boron atoms lie on the corners of hexagons with the three nearest neighbor boron atoms in each plane. The M atoms lie directly in the centers of each boron hexagon, but midway between adja- cent boron layers. Each transition metal atom has 12 nearest neighbor B atoms and eight nearest neighbor transition met- al atoms (six are on the metal plane and two out of the metal plane). There is one formula unit per primitive cell and the crystal has simple hexagonal symmetry (D6h). By choosing Fig. 1. (Color online) Schematic representation of the ScB2 crys- tal structure. 772 Low Temperature Physics/Fizika Nizkikh Temperatur, 2013, v. 39, No. 7 Electronic structure, phonon spectra and electron–phonon interaction in ScB2 appropriate primitive lattice vectors, the atoms are posi- tioned at Sc (0,0,0), B (1/3,1/6,1/2), and B (2/3,1/3,1/2) in the unit cell. The distance between Sc–Sc is equal to c. This structure is quite close packed, and can be coped with effi- ciently and accurately by the atomic sphere approximation method. However, for precise calculation of the phonon spectra and electron–phonon interaction, a full potential ap- proximation should be used. The Eliashberg function (the spectral function of the electron–phonon interaction) expressed in terms of the phonon linewidths νγq has the form [26] 2 1( ) = ( ). 2 ( )F F N ν ν νν γ α ω δ ω−ω π ε ω∑ q q qq (1) The line-widths characterize the partial contribution of each phonon: 2 ,= 2 | | ( ) ( ).j F j Fj j jj g ν ′ν ν +′+ ′ γ πω δ ε − ε δ ε − ε∑ q q q k k qk q k k (2) The electron–phonon interaction constant is defined as 2 ph 0 = 2 ( ).e d F ∞ − ω λ α ω ω∫ (3) It can also be expressed in terms of the phonons line- widths: ph 2= , ( ) e FN ν − ν ν γ λ π ε ω ∑ q q q (4) were ( )FN ε is the electron density of states per atom and per spin on the Fermi level and q qj jg ν ′+k k is the electron– phonon interaction matrix element. The double summation over Fermi surface in Eq. (2) was carried out on dense mesh (793 point in the irreducible part of the Brilloin zone (BZ)). Calculations of the electronic structure and physical properties of the ScB2 diborides were performed using fully relativistic LMTO method [27] with the experimentally ob- served lattice constants: a = 3.117 Å and c = 3.407 Å [15]. For the calculation of the phonon spectra and electron– phonon interaction a scalar relativistic FP-LMTO method [28] was used. In our calculations we used the Perdew– Wang [29] parameterization of the exchange-correlation potential in general gradient approximation. BZ integra- tions were performed using the improved tetrahedron me- thod [30]. Phonon spectra and electron–phonon matrix elements were calculated for 50 points in the irreducible part of the BZ using the linear response scheme developed by Savrasov [28]. The 3s and 3p semi-core states of ScB2 were treated as valence states in separate energy windows. Variations in charge density and potential were expanded in spherical harmonics inside the MT sphere as well as 2894 plane waves in the interstitial area with 88.57 Ry cut-off energy. As for the area inside the MT spheres, we used 3k–spd LMTO basis set energy (–0.1, –1, –2.5 Ry) with one-center expansions inside the MT-spheres per- formed up to lmax = 6. 3. Results and discussion 3.1. Energy band structure Figure 2 presents the energy band structure and total density of states of ScB2. The partial DOSs ScB2 are shown in Fig. 3. Our results for the electronic structure of ScB2 are in a good agreement with earlier calculations [9,11,13,14,23]. The Sc 3d states are the dominant features in the interval from − 10.0 to 12 eV. These tightly bound states show overlap with B 2p and, to a lesser extent, with B 2s states both above and below ,Fε implying consider- Fig. 2. (Color online) Energy band structure and total DOS [in states/(cell⋅eV)] of ScB2. Fig. 3. (Color online) Partial density of states of ScB2. Low Temperature Physics/Fizika Nizkikh Temperatur, 2013, v. 39, No. 7 773 S.M. Sichkar and V.N. Antonov Fig. 4. (Color online) The calculated hole sheet of the Fermi sur- face around A symmetry point from the 3rd energy band (a) and electron sheet from the 5th energy band (b) in ScB2. able covalency. The crystal field at the Sc site (D6h point symmetry) causes the splitting of Sc d orbitals into a sing- let 1 23 1 ( )g z a d − and two doublets 1ge ( yzd and )xzd and 2ge ( xyd and 2 2 ). x y d − The crystal field at the B site (D3h point symmetry) causes the splitting of B p orbitals into a singlet 4 ( )za p and a doublet 2e ( xp and ).yp B s states occupy a bottom of valence band between − 11.1 eV and − 1.0 eV and hybridize strongly with B xp and yp and Sc xzd and yzd states. B xp and yp occupied states are located between − 11.0 eV and .Fε B zp states occu- pied a smaller energy interval from − 5.5 eV to Fε with a very strong and narrow peak structure at around − 2 eV. ScB2 diboride has partially unoccupied bonding bands. The Sc d band along MΓ − is below Fε (Fig. 2) and the large contribution to ( )FN ε is due to Sc d states. There is a small hole concentration of B ,2 x yp states at A symme- try point. Thus, one can expect for ScB2 only low- temperature superconductivity. 3.2. Fermi surface The Fermi surface (FS) of ScB2 consists of three sheets: two small almost identical closed hole ellipsoids around A symmetry point (Fig. 4(a)) and open large electron sheet derived from the crossing of the Fermi energy by the 5th energy band (Fig. 4(b)). Figure 5 shows the calculated Fermi surface cross section areas of ScB2 in the plane per- pendicular to the z direction and crossed A symmetry point, crossed Γ point and in the plane at half distance between A and Γ points. The Fermi surfaces of ScB2, ZrB2, and HfB2 were stu- died by Pluzhnikov et al. [25] using the dHvA effect. Fig- ure 6 represents angular variations of the experimentally measured dHvA frequencies [25] for ScB2 in comparison with the first-principle calculations for field direction in the (1010), (1120), and (0001) planes. The observed de- pendences ,τ ϕ, and Ψ show that these fragments of the FS are strongly anisotropic, and the dependences of π and σ are close to an ellipsoidal frequencies. The theoretical calculations reveal that π and σ oscillations indeed be- long to hole ellipsoids around the A symmetry point. The ϕ, ,τ and Ψ orbits belong to large open electron FS. Two Fig. 5. (Color online) The calculated Fermi surface cross section areas of ScB2 in the plane perpendicular to the z direction and cross A symmetry point (a), cross Γ point (c) and in the plane at half distance between A and Γ points (b). The cross sections of hole ellipsoids present by full blue curve and red dashed curve for the 3rd and 4th energy bands, respectively. The magenta curves at all three panels show the cross sections of the Fermi surface for the electron sheet corresponding to the 5th energy band. 774 Low Temperature Physics/Fizika Nizkikh Temperatur, 2013, v. 39, No. 7 Electronic structure, phonon spectra and electron–phonon interaction in ScB2 hole ellipsoids around A point have almost identical form and slightly different size, as a result they have similar Fermi surface cross section areas (π and σ orbits for the 3rd and 4th energy bands, respectively) appeared at all the three planes (Fig. 6). The theory reasonably well reproduc- es the experimentally measured frequencies for the ,σ ϕ, ,τ and Ψ orbits. However, at the (1120) plane we were not able to detect low frequency β orbit observed experi- mentally. The experiment for high frequencies detected only Ψ orbits in vicinity of the < 0001 > direction in ScB2. We found an additional ,α β and γ orbits situated at the electron FS. These orbits have not been detected in the dHvA experiment [25]. One of the possible reasons for that is the relatively large cyclotron masses for these orbits. Figure 7 shows the theoretically calculated angular depen- dence of the cyclotron masses ( )bm and the experimental- ly measured masses *( )cm in ScB2. The cyclotron effective masses were determined from the temperature depen- dences of the amplitudes of the dHvA oscillations. The cyclotron masses for the α , β and γ orbits are much larg- er than for the corresponding low-frequency oscillations ,π ,σ ,τ and .Ψ We note that band cyclotron effective masses bm are renormalized by the electron–phonon interaction * =cm (1 ),bm= + λ where λ is the constant of the electron– phonon interaction. By comparing the experimentally measured cyclotron masses with band masses we can esti- mate the .λ It is strongly varied on the orbit type and magnetic direction. We estimate the constant of the elec- tron–phonon interaction to be equal to 0.16 and 0.41 for the π and σ hole orbits, respectively, with H || <0001>. The constant λ for the electron orbits is significantly larger and equal to 0.9 and 1.1 for the Ψ and τ orbits, respectively. 3.3. Phonon spectra The unit cell of ScB2 contains three atoms, which gives in general case a nine phonon branches. Figure 8 shows theoretically calculated phonon dispersion curves along Γ–A symmetry direction in ScB2. Figure 9 shows theoretically calculated phonon density of state for ScB2 (full blue curve). The DOS for ScB2 can be separated into three dis- tinct regions. Based on our analysis of relative directions of eigenvectors for each atom in unit cell, we found that the first region (with a peak in phonon DOS at 26.9 meV) is dominated by the motion of Sc. This region belongs Fig. 6. (Color online) The calculated (open red, blue and magenta circles) and experimentally measured [25] (black full squares) angular dependence of the dHvA oscillation frequencies in the compound ScB2. Fig. 7. (Color online) The calculated angular dependence of the cyclotron masses in ScB2 (open red, blue and magenta circles) and experimentally measured ones [25] (black full squares). Fig. 8. (Color online) Theoretically calculated phonon dispersion curves along Γ–A symmetry direction in ScB2. Low Temperature Physics/Fizika Nizkikh Temperatur, 2013, v. 39, No. 7 775 S.M. Sichkar and V.N. Antonov to the acoustic phonon modes. The second wide region (54–83 meV) results from the coupled motion of Sc and the two B atoms in the unit cell. The 1 ,uE 2 ,gA 1gB pho- non modes lie in this area (see Fig. 8 and Table 1). The pho- non DOS in the third region extends from 83 to 100 meV. This is due to the movement of boron atoms and is ex- pected since boron is lighter than Sc. The covalent charac- ter of the B–B bonding is also crucial for the high frequen- cy of phonons. The in-plane 2gE mode belongs to this region. The second and third regions represent optical pho- non modes in crystals. The most significant feature in the phonon DOS is a gap around 33–54 meV. This gap is a consequence of the large mass difference between B and Sc, which leads to decoupling of the transition metal and boron vibrations. Currently, there are no data concerning the experimen- tally measured phonon DOS in ScB2. So we compare our results with theoretically calculated phonon DOS by Deli- goz et al. [15] (Fig. 9). Calculations of these authors were based on the density functional formalism and generalized gradient approximation. They used the Perdew–Burke– Ernzerhof functional [31] for the exchange-correlation energy as it is implemented in the SIESTA code [32]. This code calculates the total energies and atomic Hellmann– Feynman forces using a linear combination of atomic or- bitals as the basis set. The basis set consists of finite range pseudoatomic orbitals of the Sankey–Niklewsky type [33] was generalized to include multiplezeta decays. The inte- ractions between electrons and core ions were simulated with the separable Troullier–Martins [34] normconserving pseudopotentials. In other words, they used the so-called “frozen phonon” technique and built an optimized rhombo- hedral supercell with 36 atoms. This method is inconvenient for calculating phonon spectra for small q points as well as for compounds with large number of atoms per unit cell. There is a good agreement between our calculations and the results of Deligoz et al. [15] in a shape and energy posi- tion of the first peak in the phonon DOS. The second and third regions consist of two peak each, in both the regions high-energy peaks have smaller intensity in our calculations in comparison with results of Deligoz et al. [15] (see also Table 1). There is also small high-energy shift of the third peak in Deligoz et al. [15] in comparison with our results. 3.4. Electron–phonon interaction Figure 10(a) shows theoretically calculated Eliashberg functions for ScB2. There are two main differences in comparison with phonon DOS curve. Low-energy peak is significantly reduced and shifted downwards by 1.6 meV. Wide 62–83 meV shoulder transform into two peaks on 68.3 and 72.8 meV. Analysis of electron–phonon prefactor 2 ( )α ω 2 2( ( ) ( ) ( )/ ( ))F Fα ω ≡ α ω ω ω shows that 2gB pho- non mode has strong coupling with electronic subsystem and significantly expands middle-energy region on Eliashberg curve. As consequence, averaged electron–phonon interac- tion constant phe−λ is reasonably large and equal to 0.47. A unique feature of electron–phonon coupling in MgB2 (Tc = 39 K) is the down-shift of the in-plane 2gE mode well below the out-of-plane 1gB mode [35]. Such an in- version of the usual sequence of mode frequencies give one wide continuous peak formed from medium- and high- energy regions. ScB2 to some extend is situated in the middle between MB2 (M = Ti, Zr, and Hf) and MgB2 dibo- rides. Superconductivity in MgB2 is also related to the ex- istence of B ,2 x yp band hole along the Γ–A direction. Moreover, according to Ref. 36, the existence of degene- rate ,x yp states above Fε in the Brillouin zone is crucial Fig. 9. (Color online) Theoretically calculated phonon density of states (full blue line) for ScB2. The open circles presents the cal- culated phonon DOS of ScB2 by Deligoz et al. [15]. Table 1. Theoretically calculated phonon frequencies (in meV) in the Γ symmetry point for ScB2 and calculated ones by Deligoz et al. [15] Reference E1u A2g B1g E2g Our results 55.247 56.85 79.113 99.29 Ref. 15 55.72 56.11 77.08 99.72 Fig. 10. (Color online) Theoretically calculated Eliashberg function 2 ( )Fα ω of ScB2 (a) and electron–phonon prefactor 2( )α ω (b). 776 Low Temperature Physics/Fizika Nizkikh Temperatur, 2013, v. 39, No. 7 Electronic structure, phonon spectra and electron–phonon interaction in ScB2 for the supercondactivity in diborides. The ,2 –2 x yD p bands in ScB2 are partially filled with small hole concen- tration near A point (see Figs. 2 and 3). On the other hand, the Fermi level for MB2 (M = Ti, Zr, and Hf) diborides falls in the pseudogap and the B ,2 x yp bands are com- pletely filled [14,35,37]. A systematic experimental search in the past for superconductivity in the d diborides showed that Tc for MB2 (M = Ti, Zr, Hf, V, Nb, Cr, Mo, U) is below 0.4 K [2]. To calculate the Tc for ScB2, we used in our calcula- tions McMillan formula modified by Allen–Dynes [38]: log * 1.04(1 )= , 1.2 (1 0.62 ) cT ω  + λ −  λ −µ + λ  (5) where logω is the effective logarithmically averaged pho- non frequency, *µ is the screening Coulomb pseudopoten- tial. We obtained Tc =1.62 K *(µ = 0.14) in good agree- ment with the experimental value 1.5 K [5]. Relatively low value can be explained by smallest logω among all transi- tion metal diborides (see Table 2). This quantity represents the effective average frequency of the coupling modes and sets the energy scale for the pairing interaction. Its small value indicates that the pairing interaction is mainly me- diated by the d atom vibrations and not by the boron modes. 3.5. Electrical resistivity In the pure metals (excluding low-temperature region), the electron–phonon interaction is the dominant factor go- verning electrical conductivity of the substance. Using lowest-order variational approximation, the solution for the Boltzmann equation gives the following formula for the temperature dependence of ( ):I Tρ 2 2cell tr2 2 0 ( ) = ( ), ( ) sinh B I F I k T dT F N v ∞πΩ ω ξ ρ α ω ωε 〈 〉 ξ∫ (6) where the subscript I specifies the direction of the elec- trical current. In our work, we investigate two direction: [0001] (c axis or z direction) and [1010] (a axis or x direc- tion). 2 Iv〈 〉 is the average square of the I component of the Fermi velocity, = /2 .Bk Tξ ω Mathematically, the transport function tr ( )Fα ω dif- fers from ( )Fα ω only by an additional factor 2[1 ( ) ( )/ ],I I Iv v v′− 〈 〉k k which preferentially weights the backscattering processes. Formula (6) remains valid in the range tr tr/5 < < 2TΘ Θ [28], where 2 1/2 tr tr ,Θ ≡ 〈ω 〉 (7) 2 2 tr tr tr 0 2= ( )F d ∞ 〈ω 〉 ωα ω ω λ ∫ , (8) 2 tr tr 0 = 2 ( ) dF ∞ ω λ α ω ω∫ . (9) The low-temperature electrical resistivity is the result of electron–electron interaction, size effects, scattering on impurities, etc., however, for high temperatures it is neces- sarily to take into account the effects of anharmonicity and the temperature smearing of the Fermi surface. In our cal- culations trΘ = 606.69 K for c axis, and 500.7 for a axis for ScB2. Figure 11 represents the theoretically calculated tem- perature dependence of electrical resistivity in ScB2. We obtained anisotropy ratio of electrical resistivity at T = = 300 K: /x zρ ρ = 1.33. Among previously studied dibo- rides (HfB2, ZrB2 and TiB2) [39,40] ScB2 has the highest degree of anisotropy. 4. Summary We have studied the electronic structure and physical properties of ScB2 using fully relativistic and full potential linear muffin-tin orbital methods. We study the electron and phonon subsystems as well as the electron–phonon interaction in this compound. We investigated the Fermi surface, angle dependence of the cyclotron masses, and extremal cross sections of the Fermi surface of ScB2 in details. Theoretical calculations show that the Fermi surface of ScB2 consists of three sheets: two small almost identical closed hole ellipsoids Fig. 11. (Color online) Temperature dependence of electrical resistivity in ScB2. Theoretically calculated for the <0001> di- rection (dashed blue curve) and the basal <1010> direction (full red curve). Table 2. The values of phe−λ and logω for transition metal diborides Diborides ScB2 ZrB2 [39] TiB2 [39] HfB2 [40] phe−λ 0.47 0.14 0.15 0.17 logω 372.23 520.37 582.13 459.25 Low Temperature Physics/Fizika Nizkikh Temperatur, 2013, v. 39, No. 7 777 S.M. Sichkar and V.N. Antonov around A symmetry point and open large electron sheet derived from the crossing of the Fermi energy by the 5th energy band. The angle variation of the ,τ ϕ, and Ψ show that these fragments of the FS are strongly anisotropic, and the dependencies of π and σ are close to an ellipsoidal frequencies. The theoretical calculations reveal that π and σ oscillations belong to hole ellipsoids around the A symmetry point. The ϕ, ,τ and Ψ orbits belong to large open electron FS. Two hole ellipsoids around A point have almost identical form and slightly different size, as a result they have similar Fermi surface cross section areas. The theory reproduces the experimentally measured fre- quencies for the ,σ ϕ, ,τ and Ψ orbits reasonably well. However, at the (1120) plane we were not able to detect low frequency β orbit observed experimentally. The expe- riment for high frequencies detected only Ψ orbits in vi- cinity of the <0001> direction in ScB2. We found an addi- tional ,α β and γ orbits situated at the electron FS. These orbits have not been detected in the dHvA experi- ment [25]. One of the possible reasons for that is the rela- tively large cyclotron masses for these orbits. We found that the cyclotron masses for the ,α β and γ orbits are much larger than for the corresponding low-frequency os- cillations ,π ,σ ,τ and .Ψ Calculated phonon spectra and phonon DOSs for ScB2 is in good agreement with previous calculations. The aver- aged electron–phonon interaction constant was found to be rather large phe−λ = 0.47 for ScB2. We calculated the temperature dependence of the electrical resistivity for ScB2 in the lowest-order variational approximation of the Boltzmann equation. We obtained rather large anisotropy ratio of electrical resistivity at T = 300 K: /x zρ ρ = 1.33. Acknowledgments This work was carried out at the Ames Laboratory, which is operated for the U.S. Department of Energy by Iowa State University under Contract No. DE-AC02- 07CH11358. This work was supported by the Director for Energy Research, Office of Basic Energy Sciences of the U.S. Department of Energy. V.N.A. gratefully acknow- ledges the hospitality during his stay at Ames Laboratory. 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