Effects of bond-randomness and Dzyaloshinskii–Moriya interactions on the specific heat at low temperatures of a spherical kagomé cluster in {W72V30}

Author:

Motohashi Mikio1,Inoue Kouki1,Morita Katsuhiro1,Fukumoto Yoshiyuki1ORCID,Nakano Hiroki2ORCID

Affiliation:

1. Department of Physics, Faculty of Science and Technology , Tokyo University of Science, Noda, Chiba 278-8510, Japan

2. Graduate School of Science, University of Hyogo , Kamigori, Hyogo 678-1297, Japan

Abstract

Abstract For the spin-1/2 spherical kagomé cluster, as well as for the 2D kagomé lattice, many low-energy singlet excitations have been expected to exist in the energy region below the spin gap, which has been actually confirmed by Kihara et al. in their specific heat measurements up to 10 K in {W72V30}, for which the exchange interaction was estimated as J = 115 K. However, the experimental result of the specific heat cannot be reproduced by the theoretical result in the Heisenberg model. Although the theoretical result has a peak around 2 K, the experimental one does not. To elucidate this difference, we incorporate Dzyaloshinskii–Moriya (DM) interactions and bond-randomness into the model Hamiltonian for {W72V30} and calculate the density of states, entropy, and specific heat at low temperatures by using the Lanczos method. We find that DM interactions do not significantly affect the energy distribution of about 10 singlet states above the ground state, which are involved in the peak structure of the specific heat around 2 K, while even 10% bond-randomness disperses this distribution to collapse the 2 K peak. Kihara et al. also reported experimental specific heats under magnetic fields up to 15 T (= 0.17J), and found that the specific heats show almost no magnetic field dependence, which strongly suggests that the bond-randomness is much stronger than the magnetic fields. For example, our calculated specific heats with 50% randomness reproduce the experimental ones up to about 5 K.

Funder

University of Tokyo

Publisher

Oxford University Press (OUP)

Subject

General Physics and Astronomy

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