Sachdev-Ye-Kitaev type physics in the strained Kitaev honeycomb model

Publication date

2021-05-13

Authors

Fremling, M.H.O.ISNI 0000000448666039
Fritz, L.ISNI 0000000419304792

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Document Type

/dk/atira/pure/researchoutput/researchoutputtypes/workingpaper/preprint
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Abstract

In this work, we investigate whether the Kitaev honeycomb model can serve as a starting point to realize the intriguing physics of the Sachdev-Ye-Kitaev (SYK) model. The starting point is to strain the system, which leads to flat bands reminiscent of Landau levels, thereby quenching the kinetic energy. The presence of weak residual perturbations, such as Heisenberg interactions and the $\gamma$-term, creates effective interactions between the Majorana modes when projected into the flux-free sector. We assume the resulting interactions to be effectively random. This leads to a bipartite Sachdev-Ye-Kitaev model (b-SYK) with very similar properties as the SYK model. We also hypothesize under which conditions one would expect the standard SYK model in such a setup.

Keywords

cond-mat.str-el

Citation

Fremling, M & Fritz, L 2021 'Sachdev-Ye-Kitaev type physics in the strained Kitaev honeycomb model' arXiv, pp. 1-14. https://doi.org/10.48550/arXiv.2105.06119