Pressure induced evolution of anisotropic superconductivity and Fermi surface nesting in a ternary boride
Subhajit Pramanick, Sudip Chakraborty, A. Taraphder
TL;DR
This work uses Migdal-Eliashberg theory implemented in EPW to characterize anisotropic, phonon-mediated superconductivity in Ta(MoB)_2, showing a single-gap superconducting state dominated by Mo-d states coupling to in-plane Mo vibrations with Tc ≈ 19.3 K at ambient pressure. The material remains dynamically stable under hydrostatic pressure up to 76.69 GPa, but its electronic structure and phonon spectrum evolve such that Tc initially decreases (P ≤ 59.71 GPa) due to a reduced N_F and stiffened phonons, followed by a Lifshitz transition at 76.69 GPa that sharpens Fermi surface nesting and abruptly increases Tc, yielding a V-shaped Tc(P) response. The absence of strong CDW signatures is linked to weak nesting and lack of phonon softening, while the Lifshitz transition provides a mechanism for pressure-induced enhancement of superconductivity. Overall, the paper highlights how Fermi surface topology and nesting interplay with EPC under pressure to govern superconductivity in a metastable ternary boride, with predictions amenable to high-pressure experiments.
Abstract
Using Migdal-Eliashberg theory implemented in Electron Phonon Wannier (EPW) code, we have investigated anisotropic superconductivity in a ternary boride $\mathrm{Ta(MoB)_2}$. It is a single-gap, anisotropic, phonon-mediated superconductor having a critical temperature $\mathrm{T_c}\sim \, 19.3$ K. A dominant contribution to superconductivity arises from the robust coupling between electronic states, primarily created by the $\mathrm{d_{xy}}$,$\mathrm{d_{x^2 - y^2}}$ orbitals of Mo atoms and the in-plane vibrations of Mo atoms. A weak Fermi surface nesting and a small electron-phonon coupling cannot induce charge density wave-like instabilities, as evidenced by the lack of a significant peak in the real part of the total Lindhard susceptibility and the absence of phonon softening. Furthermore, we have studied its electronic and superconducting properties under hydrostatic pressure up to 76.69 GPa, owing to its low bulk modulus and metastability. The persistent reduction in the density of states at the Fermi level, Fermi surface nesting and the stiffening of phonon modes lead to a diminution of superconductivity under pressure up to 59.71 GPa. At 76.69 GPa, a modification in the topology of the Fermi surface, namely a Lifshitz transition, occurs resulting in a sudden enhancement of nesting. This enhanced nesting, in turn, induces an abrupt stabilisation of superconductivity at 76.69 GPa, resulting in a V-shaped response to pressure.
