Abstract
In order to discuss the spin-gap formation in a multiorbital system, we analyze an -orbital Hubbard model on a geometrically frustrated zigzag chain by using a density-matrix renormalization group method. Due to the appearance of a ferro-orbital arrangement, the system is regarded as a one-orbital system, while the degree of spin frustration is controlled by the spatial anisotropy of the orbital. In the region of strong spin frustration, we observe a finite energy gap between ground and first-excited states, which should be called a spin-orbital gap. The physical meaning is clarified by an effective Heisenberg spin model including the correct effect of the orbital arrangement influenced by the spin excitation.
- Received 23 July 2006
DOI:https://doi.org/10.1103/PhysRevB.75.014410
©2007 American Physical Society