First-principles investigation of isolated band formation in half-metallic TixGa1xP(x=0.31250.25)

P. Palacios, J. J. Fernández, K. Sánchez, J. C. Conesa, and P. Wahnón
Phys. Rev. B 73, 085206 – Published 22 February 2006

Abstract

Several alloy semiconductors containing a transition metal atom of the type MGa4X3 with X=As or P and M=Sc or Ti have been found previously to present an isolated partially filled intermediate band within the usual band gap of the host semiconductors and have been proposed as highly efficient photovoltaic materials. In this paper, we carry out an ab initio investigation of band structures and electronic properties for the more chemically stable TixGa1xP compound as a candidate for isolated intermediate band formation. We have calculated the electronic structures using self-consistent density functional theory method in both local density approximation and generalized gradient approximation (GGA) approaches and compared the GGA results with those obtained with the exact exchange method that we have implemented in the code SIESTA. Using spin-polarized localized wave functions to represent the valence electrons states and nonlocal pseudopotentials for the core electrons, we have also studied in detail the TixGa1xP compounds at different dilution levels of the Ti transition metal atom (x=3.125%,6.25%,12.5%,25.0%) and for two (cubic and tetragonal) different crystal cells. Results at the different dilutions show in all cases a fully spin-polarized structure and, except for the case of immediate Ti neighbors, indicate a rather small spin coupling between Ti atoms and confirm the presence of the isolated narrow partially filled intermediate band for this compound. They also show the higher suitability of isotropic crystal structures for obtaining in these materials the intermediate band with the desired small band width.

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  • Received 5 August 2005

DOI:https://doi.org/10.1103/PhysRevB.73.085206

©2006 American Physical Society

Authors & Affiliations

P. Palacios1, J. J. Fernández1, K. Sánchez1, J. C. Conesa2, and P. Wahnón1

  • 1Instituto de Energía Solar, ETSI Telecomunicación, Universidad Politécnica de Madrid, 28040 Madrid, Spain
  • 2Instituto de Catálisis and Petroleoquímica, CSIC, Marie Curie 2, Cantoblanco, 28049 Madrid, Spain

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Vol. 73, Iss. 8 — 15 February 2006

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