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新型可升华自旋交叉分子Fe{[Me2Pyrz]3BH}2薄膜中的热滞现象及转变温度变化

Hysteresis and change of transition temperature in thin films of Fe{[Me2Pyrz]3BH}2, a new sublimable spin-crossover molecule.

作者信息

Davesne V, Gruber M, Studniarek M, Doh W H, Zafeiratos S, Joly L, Sirotti F, Silly M G, Gaspar A B, Real J A, Schmerber G, Bowen M, Weber W, Boukari S, Da Costa V, Arabski J, Wulfhekel W, Beaurepaire E

机构信息

Institut de Physique et de Chimie des Matériaux de Strasbourg, UMR 7504 CNRS, Université de Strasbourg, 23 rue du Loess, 67034 Cedex 2 Strasbourg, France.

Institut de Chimie et Procédés pour l'Energie, l'Environnement et la Santé, UMR 7515 CNRS, Université de Strasbourg, 25 rue Becquerel, 67087 Cedex 2 Strasbourg, France.

出版信息

J Chem Phys. 2015 May 21;142(19):194702. doi: 10.1063/1.4921309.

Abstract

Thin films of the spin-crossover (SCO) molecule Fe{[Me2Pyrz]3BH}2 (Fe-pyrz) were sublimed on Si/SiO2 and quartz substrates, and their properties investigated by X-ray absorption and photoemission spectroscopies, optical absorption, atomic force microscopy, and superconducting quantum interference device. Contrary to the previously studied Fe(phen)2(NCS)2, the films are not smooth but granular. The thin films qualitatively retain the typical SCO properties of the powder sample (SCO, thermal hysteresis, soft X-ray induced excited spin-state trapping, and light induced excited spin-state trapping) but present intriguing variations even in micrometer-thick films: the transition temperature decreases when the thickness is decreased, and the hysteresis is affected. We explain this behavior in the light of recent studies focusing on the role of surface energy in the thermodynamics of the spin transition in nano-structures. In the high-spin state at room temperature, the films have a large optical gap (∼5 eV), decreasing at thickness below 50 nm, possibly due to film morphology.

摘要

自旋交叉(SCO)分子Fe{[Me2Pyrz]3BH}2(Fe-pyrz)的薄膜被升华到Si/SiO2和石英衬底上,并通过X射线吸收和光电子能谱、光吸收、原子力显微镜和超导量子干涉装置对其性质进行了研究。与之前研究的Fe(phen)2(NCS)2不同,这些薄膜不是光滑的,而是颗粒状的。这些薄膜定性地保留了粉末样品的典型SCO性质(SCO、热滞回、软X射线诱导的激发自旋态捕获和光诱导的激发自旋态捕获),但即使在微米厚的薄膜中也呈现出有趣的变化:当厚度减小时,转变温度降低,并且滞回受到影响。我们根据最近关注表面能在纳米结构自旋转变热力学中作用的研究来解释这种行为。在室温下的高自旋态中,薄膜具有较大的光学带隙(约5 eV),在厚度低于50 nm时减小,这可能归因于薄膜形态。

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