Spin dynamics and an orbital-antiphase pairing symmetry in iron-based superconductors
Abstract
The symmetry of the wave function describing the Cooper pairs is one of the most fundamental quantities in a superconductor but its measurement in the iron-based superconductors has proved to be very difficult. The complex multi-band nature of these materials makes the interplay of superconductivity with spin and orbital dynamics very intriguing, leading to very material dependent magnetic excitations, and pairing symmetries. Here we use first-principles many-body method, including ab initio determined two-particle vertex function, to study the spin dynamics and superconducting pairing symmetry in a large number of iron-based superconductors. In iron compounds with high transition temperature, we find both the dispersive high-energy spin excitations, and very strong low energy commensurate or nearly commensurate spin response, suggesting that these low energy spin excitations play the dominate role in cooper pairing. We find three closely competing types of pairing symmetries, which take a very simple form in the space of active iron orbitals, and differ only in the relative quantum mechanical phase of the , and orbital contributions. The extensively discussed s symmetry appears when contributions from all orbitals have equal sign, while the opposite sign in and orbitals leads to the wave symmetry. A novel orbital antiphase symmetry emerges when orbital has opposite sign to and orbitals. We propose that this orbital-antiphase pairing symmetry explains the puzzling variation of the experimentally observed superconducting gaps on all the Fermi surfaces of LiFeAs. This novel symmetry of the order parameter may be realized in other iron superconductors.
Keywords
Cite
@article{arxiv.1311.1188,
title = {Spin dynamics and an orbital-antiphase pairing symmetry in iron-based superconductors},
author = {Z. P. Yin and K. Haule and G. Kotliar},
journal= {arXiv preprint arXiv:1311.1188},
year = {2015}
}
Comments
6 pages plus 7-page supplementary information