Free energy barrier and thermal-quantum behavior of sliding bilayer graphene
Jean Paul Nery, Lorenzo Monacelli, Francesco Mauri
TL;DR
The study addresses how thermal and quantum fluctuations renormalize the free-energy barrier governing sliding between graphene layers. It employs the stochastic self-consistent harmonic approximation (SSCHA), augmented by an interpolation technique, to compute temperature-dependent free energies at both the equilibrium and saddle-point configurations, including unstable states. The results show the barrier drops from $V_{\mathrm{SP}}=1.24$ meV/atom (fixed nuclei) to about $0.80$ meV/atom at $T=100$ K (≈$35\%$ reduction), remains near this value up to ~500 K, and further decreases to ~ $0.64$ meV/atom at $T=1000$ K, with quantum effects negligible above ~100 K and interlayer shear modes driving the reduction. This leads to a corrected maximum shear stress of $0.13$ GPa in agreement with experiments, demonstrating that thermal effects must be included in free-energy barrier calculations and providing a general framework for studying thermally activated sliding in other macroscopic layered systems.
Abstract
In multilayer graphene, the stacking order of the layers plays a crucial role in the electronic properties and the manifestation of superconductivity. By applying shear stress, it is possible to induce sliding between different layers, altering the stacking order. Here, focusing on bilayer graphene, we analyze how ionic fluctuations alter the free energy barrier between different stacking equilibria. We calculate the free energy barrier through the state-of-the-art self-consistent harmonic approximation, which can be evaluated at unstable configurations. We find that above 100 K there is a large reduction of the barrier of more than 30% due to thermal vibrations, which significantly improves the agreement between previous first-principles theoretical work and experiments in a single graphite crystal. As the temperature increases, the barrier remains nearly constant up to around 500 K, with a more pronounced decrease only at higher temperatures. Our approach is general and paves the way for systematically accounting for thermal effects in free energy barriers of other macroscopic systems.
