Effects of the Next-Nearest-Neighbor Hopping on the Low-Dimensional Hubbard Model: Ferromagnetism, Antiferromagnetism, and Superconductivity
Luhang Yang, Adrian E. Feiguin, Thomas P. Devereaux, Elbio Dagotto
TL;DR
This work surveys numerical studies of the Hubbard model with next-nearest-neighbor hopping ($t_2$) in one and two dimensions, focusing on how $t_2$ reshapes magnetism and superconductivity. By formulating the $t_1-t_2-U$ and related $t_1-t_2-J_1-J_2$ models and employing methods such as DMRG, QMC, tensor networks, and exact diagonalization, the authors map out phase diagrams featuring AFM, FM, SC, CDW, and PDW across dopings. A key finding is that NNN hopping can stabilize superconductivity on the electron-doped side in 2D and induce FM and PDW phenomena in 1D and near van Hove regions, though the presence of a SC dome on the hole-doped side remains contested. Altogether, the study highlights the critical role of band topology and longer-range hopping in shaping correlated phases and informs ongoing debates about cuprate-like superconductivity and related materials.
Abstract
The Hubbard model has attracted considerable interest due to its prototypical role in describing strongly interacting electronic systems, such as high-critical-temperature superconductors as well as many novel quantum materials. By introducing next-nearest-neighbor (NNN) hoppings to the Hubbard model, the phase diagram becomes richer, and fascinating phenomena arise in both, one-dimensional chains and square lattices, such as: antiferromagnetism (AFM), ferromagnetism (FM), superconductivity (SC), as well as charge orders, among others. Moreover, NNN hoppings play a fundamental role in understanding effects of doping on magnetism and pairing orders in strongly interacting regimes. In this article, we review the recent progress in understanding the different competing phases of this model in one and two dimensions from a computational perspective. We comment on the pressing technical challenges, illustrate the controversial results concerning the emergence of the SC phase, and conclude with our perspectives on future explorations.
