We present the main features of the spin-orbital superexchange which describes the magnetic and optical properties of the Mott insulators with orbital degrees of freedom. In contrast to the SU(2) symmetry of spin superexchange, the orbital part of the superexchange obeys the lower cubic symmetry of the lattice and is intrinsically frustrated. This intrinsic frustration and spin-orbital entanglement induce enhanced quantum fluctuations, and we point out a few situations where this leads to disordered states. Strong coupling between the spin and orbital degrees of freedom is discussed on the example of the RVO 3 perovskites, with R standing for rare-earth ion, La,. . .,Lu. We explain the observed evolution of the orbital T OO and Néel T N1 transition temperature in the RVO 3 series with decreasing ionic radius r R . A few open problems and the current directions of research in the field of spin-orbital physics are pointed out.
Orbital versus spin superexchangeIn recent years the physical properties of Mott (or charge transfer) insulators are in the focus of interest in the condensed matter theory [1]. In order to develop theoretical understanding of complex phenomena in doped correlated insulators, including high temperature superconductivity in the cuprates and the colossal magnetoresistance (CMR) in the manganites, it is necessary to describe first the undoped materials, such as La 2 CuO 4 and LaMnO 3 . In both cases the local Coulomb interactions (Hubbard U ) is large and suppresses charge fluctuations, leading to low-energy effective Hamiltonians with superexchange interactions which stabilize antiferromagnetic (AF) spin order at low temperature [2,3]. However, these two compounds are qualitatively quite different. On the one hand, the degeneracy of partly filled e g orbitals is lifted in La 2 CuO 4 by the tetragonal distortions of CuO 6 octahedra, resulting in two-dimensional (2D) AF superexchange of S = 1/2 holes in x 2 − y 2 orbitals of Cu 2+ ions. On the other hand, in LaMnO 3 e g orbital degeneracy plays a fundamental role and, together with the Jahn-Teller (JT) distortions, is required to understand the origin of the anisotropic A-type AF (A-AF) order [4]. As realized already three decades ago [2], in this latter case the orbital degrees of freedom, which are described by the components |x ≡(1) of pseudospin τ = 1/2 and contribute explicitly to the structure of the superexchange. Thus they have to be included on equal footing with ionic spins in a spinorbital superexchange model. In the last two decades several new concepts were developed, such as enhanced quantum fluctuations due to orbital degrees of freedom which participate in joint spin-orbital excitations [5], and spin-orbital entanglement which occurs in cases when spin and orbital operators cannot be decoupled from each other [6]. The actual physical problems in this emerging and rapidly developing field were reviewed in the Focus Issue Orbital Physics in New Journal of Physics [7] a few years ago. Here we want to focus on a few representative r...