https://doi.org/10.1140/epjd/e2017-80048-3
Topical Review
A review of recent progress in understanding the spontelectric state of matter*
1 ISA, Department of Physics and Astronomy, Aarhus University, 8000 Aarhus C, Denmark
2 Sincrotrone Trieste, S.C.p.A. di Interesse Nazionale, 34149 Basovizza, Trieste, Italy
3 Institute of Chemical Sciences, Heriot-Watt University, Riccarton, EH14 4 AS Edinburgh, UK
4 Laboratoire Interuniversitaire des Systèmes Atmosphériques (LISA), CNRS UMR 7583, Université Paris-Est Créteil, UniversitéParis Diderot, Faculté des Sciences et Technologie, 61 avenue du Général de Gaulle, 94010 Créteil Cedex, France
a
e-mail: dfield@phys.au.dk
Received: 23 January 2017
Received in final form: 31 March 2017
Published online: 20 June 2017
The spontelectric state of matter is exemplified by the presence of static, spontaneous electric fields extending throughout thin films of dipolar solids. The spontelectric state was discovered using a low energy electron beam technique, using the ASTRID storage ring at Aarhus University. Following a resume of the characteristics and of a model for the spontelectric effect, a description is given of the counter-intuitive behaviour of fields in films of methyl formate as a function of deposition temperature, T. It is found that films for T ≤ 77.5 K show the expected decrease in the field with increasing T but, for T ≥ 77.5 K, an increase in the field for higher T is revealed. Analysis of these results illustrates the non-linear and non-local characteristics of the spontelectric state. Recently it has been shown that Reflection-Absorption Infrared Spectroscopy (RAIRS) provides a new and independent technique for the detection of the spontelectric effect, through the observation of vibrational Stark shifts in spectra of films. Stark shifts for nitrous oxide are demonstrated to be in harmony with electric fields measured using the electron beam technique. The method is then applied to carbon monoxide, showing that this material displays the spontelectric effect between deposition temperatures of 20 K and 26 K.
© EDP Sciences, Società Italiana di Fisica, Springer-Verlag 2017
