Machine-learning Guided Search for Phonon-mediated Superconductivity in Boron and Carbon Compounds
Niraj K. Nepal, Lin-Lin Wang
TL;DR
This work develops a workflow that couples high-throughput DFPT calculations of electron-phonon coupling with machine-learning guided searches to identify boron/carbon–based superconductors at ambient pressure. Crucially, it includes compounds with imaginary phonon modes (dynamical instability) in the training data, using stabilization strategies to extract EPC properties and Tc estimates. The study compares CGCNN and ALIGNN, finding ALIGNN generally superior when unstable data are included, and reports promising Tc predictions for metastable materials such as Ca$_5$B$_3$N$_6$ and TaNbC$_2$, highlighting the role of soft, stabilized phonons in enhancing superconductivity. The methodology provides a robust screening tool for metastable phases and suggests that metastable boron/carbon compounds near the convex hull can host sizable Tc, with implications for discovering new phonon-mediated superconductors at ambient conditions.
Abstract
We present a workflow that iteratively combines \textit{ab-initio} calculations with a machine-learning (ML) guided search for superconducting compounds with both dynamical stability and instability from imaginary phonon modes, the latter of which have been largely overlooked in previous studies. Electron-phonon coupling (EPC) properties and critical temperature (T$_c$) of 417 boron, carbon, and borocarbide compounds have been calculated with density functional perturbation theory (DFPT) and isotropic Eliashberg approximation. Our study addresses T$_c$ convergence of Brillouin zone sampling with an ansatz test, stabilizing imaginary phonon modes for significant EPC contributions and comparing performance of two ML models especially when including compounds of dynamical instability. We predict a few promising superconducting compounds with formation energy just above the ground state convex hull, such as Ca$_5$B$_3$N$_6$ (35 K), TaNbC$_2$ (28.4 K), Nb$_3$B$_3$C (16.4 K), Y$_2$B$_3$C$_2$ (4.0 K), Pd$_3$CaB (7.0 K), MoRuB$_2$ (15.6 K), RuVB$_2$ (15.0 K), RuSc$_3$C$_4$ (6.6 K) among others.
