PhysicaC 216 (1993) 12-16 North-Holland Electronic structure of mercury-based high- TCcompounds: H@aKan-ICu,%+2 (n= L&3) C.O. Rodriguez IFLYSIB, Grupo Fisica de1 S&do, C.C. 565, La Plata (1900). Argentina N.E. Christensen and E.L. Peltzer y Blanch Institute of Physics and Astronomy, Aarhus University, DIM000 Aarhus, C, Denmark Received 14 July 1993 A fist principles determination of the electronic structure of the tetragonal mercury-based compounds containing one Hg plane, HgBarCuO, (Hgl201), HgBa2CaCua06 (Hgl212) and HgBaaCarCusOs (Hgl223), has been made within the local-density approximation using the full potential linear muffin tin orbital method. The band structures exhibit overall features similar to those of other cuprate superconductors with a marked peculiarity: an antibonding band coming mostly from the hybridization of Hg - p andd and apicaloxygen (02) -p states whichlies slightly above the Fermilevel for Hgl201 and below it for Hgl212 andHg1223, but whose exact position depends on the relative z-position of apical 02 atoms within the unit cell. This detail is important to establish the degree of self-doping in these compounds. 1. Introduction The report by Putilin et al. [ 1] of superconductivity at 94 K in HgBazCu04+, stimulated considerable interest in Hg-based systems. The crystal structure of Hgl20 1 is multi-layered, each unit containing one copper oxide layer. Experience with analogous copper oxide compounds based on thallium or bismuth showed that the transition temperature increased as the number of copper oxide layers n in the unit cell increased from n= 1 to 3. A similar effect was expected for the mercury family with more than one copper oxide layer. &hilling et al. [2] reported magnetic and resistivity measurements confirming a maximum critical temperature of 133 K in a material containing HgBazCazCu908+,, HgBazCaCuzOs+,., and an ordered superstructure composed of a sequence of the unit cells of these two phases. The highest-T, superconducting phase has not yet been identified. In this paper we present a fist principles determination of the electronic structure for the stoichiometric structures for the three members of the family Hg1201, Hg1212 and Hg1223 within the local 0921-4534/93/$06.00 density approximation (LDA) using the full potential linear muffin tin orbital (FP-LMTO) method [ 3 1. Structural properties and a detailed study of the electronic structure of Hgl201 have already been reported [ 4 1, and this serves as a basis for the analysis in the present study. One can compare the behavior of the mercury family HgBaZCan_-ICunOZn+Z to that of TlzBazCa,_ 1C~n02n+4,n= 1, 2, 3 (notice that, as pointed out in ref. [51,the formal valence of two T13+02- layers is the same as that of a single Hg2+ layer). The major difference lies in the oxygen stoichiometry of the HgO, and TlO,_, layers, respectively (x=0 for the studied stoichiometric compounds). From theoretical predictions in such Tlbased materials [ 6-8 ] a Tl-0 derived band dips below the Fermi energy (&) for the entire series making the behavior of all these materials self-doped. The minimum of the “dopand” band is 0.14, 0.20 and 0.25 eV below EF,for the one-, two-, and three-layer materials, respectively. A similar behavior cannot be ruled out for the Hg family, since a hybridization of Hg-states with the apical oxygens and Ba may develop, so as to make this Hg-0 derived band cross or stay close to Ep The structural and internal struc- 0 1993 Elsevier Science Publishers B.V. All rights reserved. CO. Rodriguez et al. /Electronic structureo/HgBa2Ca,_ ICun02n+l tural parameters of Hgl201 are well established [ 1,9]. In this case, the Hg-0 derived band lies slightly above EF (0.13 and 0.09 eV at X and R, respectively ) . The precise character of this band, where it is close to EF, is Hg( p,)-02 (p,), whereas it is mainly Hg( dZ2)-02(p,) in the rest of the Brillouin zone. A structural model was set up for Hg12 12 and Hg1223, based on the relative positions of atoms in the infinite-layered compound CaCuO, [ lo] and those of Hg 120 1 [ 1,9], scaled according to the experimentally known lattice parameters. This allowed a systematic study of the band structure to be made and in particular made it possible to determine the position of the Hg-0 derived band for the three members of the Hg family, and its dependence on the z-position of apical 02 atoms. Using our model structures for Hg1212 and Hg1223, the band minimum lies below EF at the X point by an amount of 0.09 and 0.10 eV, respectively. The values at the R point are very similar. We have also used for Hg1223 the known structure of the analogue, T1Ba2CazCujOg compound [ 111 substituting the TlO plane by Hg, resealing for the experimental c and a lattice parameters and found the Hg-0 band crossing below EF at 0.146 eV. We have, however, studied the variations of that particular band for small changes of the 02 z-position, and found minor modifications of the dipping relative to EF. This means that variations from our model structure of the 02-Hg distance will not modify the qualitative picture of the band structure presented in this paper for Hg1212 and Hg1223. The question as to the degree of the self-doping for the two- and threelayered compounds can only be answered when the actual crystal structures are known. 13 eluded explicitly for 15 6, inside the MT spheres. The charge density in the interstitial region is obtained by matching a linear combination of atom-centered Hankel functions with II 6 and for two different rc2 values (formal envelope kinetic energy [ 12 ] ) , to the values and slopes of the density on the sphere. The “tails” with I> 6 of the Hankel functions extend into the spheres. The final density is then continuous and smooth and includes angular momentum terms with 1 up to infinity. Poisson’s equation can then be solved analytically for the interstitial region and by numerical integration inside the spheres. For the contribution from the interstitial potential to the matrix elements, the product of two Hankel functions is fitted in the interstitial region by a linear combination of Hankel functions as for the charge density [ 13 1. The basis functions are defined using a triple+ set. The choice of kinetic energies IC’,associated with the envelope Hankel functions is not critical and we have taken them to be -0.25, - 1.0 and -3.0 Ry. The core electrons are allowed to relax; the core charge density is recalculated at each iteration in the self-consistency loop. All calculations were done within the LDA using the Barth-Hedin parametrization of the exchange-correlation energy and potential [ 141. The basis set included 19 1, 256 and 276 LMTO’s per cell for the one-, two- and threelayer compounds, respectively. To obtain the desired precision it was necessary to use 84 points plus linear tetrahedral interpolation in the irreducible Brillouin zone of the tetragonal structure. The calculations were carried out in two panels including the following orbitals as semicore: Cu (3s and 3p), Ba (Ss), Hg (5~). 3. Results 2. Method of calculation We’ have used the FP-LMTO technique which makes no shape approximation for the charge density or for the potential [ 31. Space is divided into non-overlapping atomic spheres and an interstitial region (muffin-tin (MT) geometry). The basis consists of MT orbitals, which are Hankel functions outside the MT spheres, augmented inside by numerical solution of Schrijdinger’s equation [ 12 1. Spherical harmonic components of the charge density are in- The tetragonal structures of Hg 120 1, Hg 12 12 and Hg1223 contain (parallel to the xy plane) n=l, 2 and 3 CuOZ planes, respectively, and n - 1 Ca atoms are located above the centres of Cu02 squares. These sandwiches are bounded by a pair of BaO planes. Oxygen atoms in the Ba planes will be called 02. Hg ions then separate these basic layered sheets. 02 is directly on top of Cu and the position of Hg is directly above 02. The lattice parameters are: az3.8797, 3.93, 3.93 A and ~~9.5087, 12.7, 16.1 8, for Hg1201, Hg1212 and Hg1223, respectively. The C.O. Rodriguez et al. /Electronic structure of HgBa2Ca,,_ IC~nOZn+2 14 position of the atoms for Hg12 12 and Hg 1223, based on our model structures are given in ref. [ 15 1. The band structure of Hg1201 for the experimental lattice constant is shown in fig. 1. Figures 2 and 3 correspond to the band structures of Hg1212 and Hg1223. The dispersion in the z direction can be seen by comparing left and right parts of figs. l-3 which are joined by the T-Z line. The left part shows the bands at k,=O in different directions between the high symmetry point r, M and X. The right part depicts the corresponding symmetry points with kpn/c: Z, Fig. 3. Band structure for Hg1223. -6 r M X r z A R 2 Fig. 1. Band structure for Hg1201. The symmetry points are r=(O,O,O),M=(l, 1,O)r/aandX=(l,O,O)n/a,Z=(0,0, 1)x/c, A= (1, 1, a/c)rr/a and R= (1, 0, a/c)x/a, (a, care the tetragonal lattice constants). r z “,x I 0 I 7 0 x E!? 3 -2 -4 -6 4 : / --ny ~ ~ -IOl- M X rZ I ~ A Fig. 2. Band structure for Hg1212. R R Fig. 4. Intersection of the LDA Fermi surface of Hg12 12 with the upper half of the Brillouin zone boundaries. The dashed line shows the Fermi surface in the nearest-neighbor two-dimensional tightbinding model for half-tilling. 4 5 I Z Fig. 5. Same as tig. 4 but for Hg1223. CO. Rodriguez et al. /Electronic structure of HgBa,Ca._ IC%&+J A, R. Figures 4 and 5 show the Fermi surface (FS) cross-sections of Hg12 12 and Hg1223 in the symmetry planes (the “box” laid out). Again, the dispersion in the z direction can be observed by the difference of crossings in the two squares. The band structure is highly two-dimensional. Our band structures agree for Hg1201 and Hg1223 with recent calculations by Singh [ 5,17 ] using the full potential linear augmented plane wave (FP-LAPW). The FS of Hg 120 1 has only one sheet denoted by (I as shown in fig. 2 of ref. [ 41, but for the case of the two and three layer compound three and four sheets appear, denoted by ul, u2, b and a,, a,, u3 and b, respectively. The a, (n= 1, 2 or 3) FS-sheets come from linear combinations of the n Cu02-derived bands characteristic of the cuprate superconductors. Each CuO, band can be understood as the antibonding pdo band from a simple tight-binding model, in the nearestneighbor approximation, which includes 0 1 (p,), Cu(dx2_,,2 ), 01 (p,,). The corresponding two-dimensional FS for the case of half filling is a square, with saddle points (van Hove singularities) at the points k=X and Y exactly at the Fermi level and would have “perfect nesting”. Both of these features disappear when next-nearest neighbor hopping between 01 (p,) and (p,) are included together with a weak hybridization of these orbitals with Cu (s) and 01 (s). The shape of the FS is more like a square turned 45” with respect to that of the simplest tightbinding model. This is very similar to what happens in YBa2Cu30, (YBCO) (see ref. [ 16 ] ). In the case of Hg1201 the saddle points in the u sheet lie far at 0.52 and 0.37 eV below EF, at X and R respectively, but get closer to EF in the other two compounds due to the interaction between the planes, which also causes the interaction with the Hg-0 derived band to increase. For the case of Hg1201 a band sets very close to E,:O. 13 and 0.09 eV at points X and R, respectively. It is also highly two-dimensional. This band is mainly derived from the Hg-apical 02 interaction, and this hybridization is such as to make this band lie close to the Fermi level. The position of this band changes and even crosses EF in both Hg12 12 and Hg1223 for our proposed structural models. This brings out the b FS-sheet in figs. 4 and 5. A finer analysis of the character of this band for Hg1223 shows that from M to X and from X to XT/ 2 is Hg(p,)-02(p,)-Ol(p,) and Ba(d,*). The 15 character changes in the region I to M, XI-/2 to F, where the states are predominantly Hg (d,z)-02 (p,). Similar behaviors have the corresponding states with k,= n/c due to the highly two-dimensional character of these states. The corresponding band for Hgl201 and Hg 12 12 shows very similar behavior. Since the precise atomic coordinates are not yet known for the two- and threelayered compound, we have studied the position of the Hg-0 derived band as 02 atoms were moved closer to and away from the Hg plane. As already mentioned the dipping was slightly modified. The deformation potential is such that changes in the zposition of 02 from our model atomic positions cannot make the minimum of this band lie on top of EF. 4. Conclusions We have presented a detailed study of the electronic structure of Hg1201, Hg1212 and Hg1223 within the LDA using the FP-LMTO method. A description of the character of the states close to and at the FS was given. We have seen that due to the small dependence of the position of the Hg-0 derived band with the z-position of the 02 atoms, only the question to the degree of self-doping in Hg1212 and Hg1223 will remain open until the precise structure is known. Acknowledgements We have benefited from the interaction with W.E. Pickett and D.J. Sir@. This work was supported by Consejo National de Investigaciones Cientificas y Ttcnicas de la Republica Argentina, by the Commission of the European Communities, Contracts no. S/CIl*-913141 and CIl*-CT92-0086 and by the Danish Research Council under grant No. 11-96851SE. References [ l] S.N. Putilin, E.V. Antipov, 0. Chmaissen and M. Marezio, Nature (London) 362 (1993) 226. [2] A. Schilling, M. Cantoni, J.D. Guo and H.R. Ott, Nature (London) 363 (1993) 56. 16 C. 0. Rodriguezet al. /Electronic structureof HgBaJCa._D.O2,,+2 [3] M. Methfessel, Phys. Rev. B 38 (1988) 1537. [4] C.O. Rodriguez, Phys. Rev. B, submitted. [ 5] D.J. Singh, Phys. Rev. B, submitted. [ 61 J. Yu, S. Massida and A.J. Freeman, Physica C I52 ( 1988) 273. [7] D.R. Hamann and L.F. Matheiss, Phys. Rev. B 38 (1988) 5138. [8] D.J. Singh and W.E. Pickett, Physica C 203 (1992) 193. [9] J.L. Wagner,P.G. Radaelli,D.G. Hinks, J.D. Jorgensen, J.F. Mitchell, B. Dabrowski, G.S. Knapp and M.A. Beno, Physica C210(1993)447. [lo] T. Siegrist, S.M. Zahurak, D.W. Murphy and R.S. Roth, Nature (London) 334 (1992) 231. [ 111 T. Hetrlein, H. Burzlaff, H.H. Otto, T. Zetterer and K.F. Renk, Natutwissenschaften 76 ( 1989) 170. [ 121 O.K. Andersen, Phys. Rev. B 12 (1975) 3060. [ 131 M. Methfessel, C.O. Rodriguez and O.K. Andersen, Phys. Rev. B 40 ( 1989) 200. [ 141 U. von Barth and L. Hedin, J. Phys. C 5 ( 1972) 1629. [ 151The atomic z-coordinates are z(Ca)=O, r(Cu)=0.1245, z(O1)=0.1245, z(Ba) =0.2763, 2(02)=0.3453, z(Hg)=0.5 for Hg1212 and z(Cul)=O, z(Oll)=O, z(Cu)=O.1993, z(O1)=0.1993, z(O2)=0.3771, z(Ba)=0.3271, z(Hg)=0.5 for Hg1223, in units of the corresponding c lattice parameter. [ 161 C.O. Rodriguez, A.I. Liechtenstein, 0. Jepsen, I. Mazin and O.K. Andersen, J. Comp. Phys., to be published. [ 171 D.J. Singh, Physica C 212 (1993) 228.
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