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Published on: August 12, 2019
Substituent-Dependent Magnetic Behavior of Discotic Benzo[e][1,2,4]triazinyls
Marcin Jasiński1, Jacek Szczytko2, Damian Pociecha3
1Faculty of Chemistry, University of Łódź , Tamka 12, 91-403 Łódź, Poland.
Abstract:
Discotic mesogens containing the benzo[e][1,2,4]triazinyl radical as the central unit exhibit a Colh phase below 80 °C. Depending on the substituent at the N(1) position, they show different modes of thermal expansion and magnetic behavior, presumably due to differences in molecular organization. Thus, for 1-phenyl (1a) and 1-PhF-m (1b) derivatives, the Colh phase has positive thermal expansion coefficient κ and antiferromagnetic interactions, while for the 1-(3,4,5-(C12H25X)3C6H2) derivatives 1c (X = O) and 1d (X = S), κ is negative and weak ferromagnetic interactions in the crystalline phase are observed for 1c (J/kB = +4.76 K). Compounds 1a and 1c exhibit photoinduced hole transport (μ ≈ 1.3 × 10(-3) cm(2) V(-1) s(-1)) in the Colh phase.
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When atoms or molecules absorb light at the proper frequency, their electrons are excited to higher-energy orbitals. For many main group atoms and molecules, the absorbed photons are in the ultraviolet range of the electromagnetic spectrum, which cannot be detected by the human eye. For coordination compounds, the energy difference between the d orbitals often allows photons in the visible range to be absorbed and emitted, which is seen as colors by the human...

