Hostname: page-component-76fb5796d-25wd4 Total loading time: 0 Render date: 2024-04-25T08:02:23.980Z Has data issue: false hasContentIssue false

Structural Aspects of Magnetic Coupling in CaCu3Mn4O12 and CaCu3Ti4P12

Published online by Cambridge University Press:  01 February 2011

M. D. Johannes
Affiliation:
Department of Physics, University of California, Dacis CA 95616
W. E. Pickett
Affiliation:
Department of Physics, University of California, Dacis CA 95616
R. Weht
Affiliation:
Departamento de a Física, CNEA, Avda. General Paz y Constituyentes, 1650 - San Martín Argentina
Get access

Abstract

Two perovskite-derived materials, CaCu3Mn4O12, have drawn much recent interest due to their magnetoresistive, dielectric, and mafnetoelectronic characteristics. Here we present initial theoretical insights into each of these points, based on first principles, density functional based calculations. Our results predict CCMO to have a spin-asymmetric energy gap, which leads to distinct temperature- and magnetic field-dependent changes in properties, and helps to account for its observed negative magnetoresistivity. We have studied CCTO primarily to gain insight into the exchange coupling in both these compounds, where the conventional superexchange coupling vanishes by symmetry for both nearest and next nearest Cu-Cu neighbors, a consequence of the structure. In CCTO, it is necessary to go 5th Cu-Cu neighbors to obstain a (superexchange) coupling that can provide the coupling necessary to give three dimensional order. Non-superexchange mechanisms may be necessary to describe the magnetic coupling in this structural clss.

Type
Research Article
Copyright
Copyright © Materials Research Society 2002

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

[1] The term “quadrupled perovskite structure” has also been used for a different (layered and oxygen deficient) class of oxide defect compounds; see for example Mansourian-Hadaci, N. et al., J.Solid State chem. 155, 216 (2000). Our description and figures will make clear the class we are discussing.Google Scholar
[2] Chenacas, J. Joubert, J. C. Marezio, M. and Bochu, B. J. Solid State Chem. 14, 25 (1975); J. C. Joubert et al., Ferrites, Proceedings of the Third Intl. Conf. on Ferrites, Kyoto 1980 (Reidel, Dordrecht, Netherlands, 1982), P.400.Google Scholar
[3] Collomb, A. et al., J. Magn. Magn. Mat. 7, 1 (1978).Google Scholar
[4] Lacroix, C. J. Phys. C 13, 5125 (1980).Google Scholar
[5] Subramanian, M.A. et al., J. Solid State Chem. 151, 323 (2000); A.P. Ramirez et al., Solid State Commun. 115 217 (2000)Google Scholar
[6] Homes, C.C. (unpublished work)Google Scholar
[7] Subramanian, M.A. (unpublished work)Google Scholar
[8] Zeng, Z. et al., J Solid State Chem. 147, 185 (1999).Google Scholar
[9] Sinclair, D.C. et al., Appl. Phys. Lett. 80, 2153 (2002).Google Scholar
[10] Homes, C.C. et al., Science 293, 673 (2001)Google Scholar
[11] He, L. et al., cond-mat /0110166Google Scholar
[12] Collomb, A. Samaras, D. Bochu, B. and Joubert, J. C. Phys. Stat. Solidi (a) 41, 459 (1977).Google Scholar
[13] Koitsch, A. et al., Phys. Rev. B 65, 052406 (2002).Google Scholar
[14] Kim, Y.J. et al., Solid State Commun. 121, 625 (2002)Google Scholar
[15] WIEN97, see Blaha, P. Schwarz, K. and Luitz, J. Vienna University of Technology, 1997, improved and updated version of the original copyrighted WIEN code, which was published by Blaha, P. Schwarz, K. Sorantin, P. and Trickey, S. B. Comput. Commun. 59, 399 (1990);Google Scholar
[16] Perdew, J.P, Y. Wang PRB, 45, 13244 (1992).Google Scholar
[17] Schwarz, K. and Mohn, P. J.Phys. F 14, L129 (1984).Google Scholar
[18] Bochu, B. et al., J. Magn. Magn. Mat. 15-18, 1319 (1980).Google Scholar
[19] Weht, R. and Pickett, W. E. Phys. Rev. B 65, 014415 (2001).Google Scholar
[20] Ziese, M. Rep. Prog. Phys. 65, 143 (2002).Google Scholar
[21] Hellberg, C.S. et al., J. Phys. Soc. Japan 68, 3489 (1999)Google Scholar
[22] Weht, R. and Pickett, W.E. Phys. Rev. Lett. 80, 2502 (1988)Google Scholar
[23] Rosner, H. et al., Phys. Rev. Lett. 88, 186405 (2002).Google Scholar
[24] Feldkemper, S. et al., Phys. Rev. B 52, 313 (1995)Google Scholar
[25] Slater, J.C. Koster, G.F. Phys. Rev. 94 844 (1954).Google Scholar