Atomistic Description of Spin Crossover Under Pressure and its Giant Barocaloric Effect

Abstract

The pressure-dependent evolution of the Spin Crossover (SCO) transition has garnered significant interest due to its connection to the giant barocaloric effect (BCE) near room temperature. Pressure alters both the molecular and solid-state structures of SCO materials, affecting the relative stability of low- and high-spin states and, consequently, the transition temperature (T_(1/2)). Crucially, the shape of the T₁/₂ vs. pressure curve dictates the magnitude of the BCE, making its accurate characterization essential for identifying high-performance materials. In this work, we investigate the nonlinear T_(1/2) vs. pressure behavior of the prototypical SCO complex [FeL₂][BF₄]₂ [L = 2,6-di(pyrazol-1-yl)pyridine] using solid-state PBE+U computations. Our results unveil the mechanisms by which pressure influences its SCO transition, including the onset of a phase transition, as well as the key role of low-frequency phonons in the BCE. Furthermore, we establish a computational protocol for accurately modeling the BCE in SCO crystals, providing a powerful tool for the rapid and efficient discovery of new materials with enhanced barocaloric performance.

Supplementary files

Article information

Article type
Paper
Submitted
07 Jul 2025
Accepted
20 Aug 2025
First published
21 Aug 2025
This article is Open Access
Creative Commons BY-NC license

J. Mater. Chem. C, 2025, Accepted Manuscript

Atomistic Description of Spin Crossover Under Pressure and its Giant Barocaloric Effect

S. Vela, J. Ribas-Ariño, S. Vallone, A. M. dos Santos, M. Halcrow and K. Sandeman, J. Mater. Chem. C, 2025, Accepted Manuscript , DOI: 10.1039/D5TC02560E

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