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Cotunneling signatures of Spin-Electric coupling in frustrated triangularmolecular magnets
Linnéuniversitetet, Fakulteten för teknik (FTK), Institutionen för fysik och elektroteknik (IFE). Lund University. (condensed matter physics)ORCID-id: 0000-0001-8162-6993
Linnéuniversitetet, Fakulteten för teknik (FTK), Institutionen för fysik och elektroteknik (IFE). Lund Univ,. (condensed matter physics)ORCID-id: 0000-0003-4489-7561
2014 (engelsk)Inngår i: Physical Review B. Condensed Matter and Materials Physics, ISSN 1098-0121, E-ISSN 1550-235X, Vol. 89, nr 23, s. Article ID: 235435-Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

The ground state of frustrated (antiferromagnetic) triangular molecular magnets is characterized by two total-spin S = 1/2 doublets with opposite chirality. According to a group theory analysis [M. Trif et al., Phys. Rev. Lett. 101, 217201 (2008)] an external electric field can efficiently couple these two chiral spin states, even when the spin-orbit interaction (SOI) is absent. The strength of this coupling, d, is determined by an off-diagonal matrix element of the dipole operator, which can be calculated by ab-initio methods [M. F. Islam et al., Phys. Rev. B 82, 155446 (2010)]. In this work we propose that Coulomb-blockade transport experiments in the cotunneling regime can provide a direct way to determine the spin-electric coupling strength. Indeed, an electric field generates a d-dependent splitting of the ground state manifold, which can be detected in the inelastic cotunneling conductance. Our theoretical analysis is supported by master-equation calculations of quantum transport in the cotunneling regime. We employ a Hubbard-model approach to elucidate the relationship between the Hubbard parameters t and U, and the spin-electric coupling constant d. This allows us to predict the regime in which the coupling constant d can be extracted from experiment.

 

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2014. Vol. 89, nr 23, s. Article ID: 235435-
HSV kategori
Forskningsprogram
Fysik, Kondenserade materians fysik
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URN: urn:nbn:se:lnu:diva-34400DOI: 10.1103/PhysRevB.89.235435ISI: 000339049700004Scopus ID: 2-s2.0-84903732948OAI: oai:DiVA.org:lnu-34400DiVA, id: diva2:719722
Tilgjengelig fra: 2014-05-26 Laget: 2014-05-26 Sist oppdatert: 2023-08-09bibliografisk kontrollert

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