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Topology and Geometry of Spin Origami

Krishanu Roychowdhury, D. Zeb Rocklin, and Michael J. Lawler
Phys. Rev. Lett. 121, 177201 – Published 23 October 2018
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Abstract

Kagome antiferromagnets are known to be highly frustrated and degenerate when they possess simple, isotropic interactions. We consider the entire class of these magnets when their interactions are spatially anisotropic. We do so by identifying a certain class of systems whose degenerate ground states can be mapped onto the folding motions of a generalized “spin origami” two-dimensional mechanical sheet. Some such anisotropic spin systems, including Cs2ZrCu3F12, map onto flat origami sheets, possessing extensive degeneracy similar to isotropic systems. Others, such as Cs2CeCu3F12, can be mapped onto sheets with nonzero Gaussian curvature, leading to more mechanically stable corrugated surfaces. Remarkably, even such distortions do not always lift the entire degeneracy, instead permitting a large but subextensive space of zero-energy modes. We show that for Cs2CeCu3F12, due to an additional point group symmetry associated with the structure, these modes are “Dirac” line nodes with a double degeneracy protected by a topological invariant. The existence of mechanical analogs thus serves to identify and explicate the robust degeneracy of the spin systems.

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  • Received 12 May 2018

DOI:https://doi.org/10.1103/PhysRevLett.121.177201

© 2018 American Physical Society

Physics Subject Headings (PhySH)

Condensed Matter, Materials & Applied PhysicsPolymers & Soft Matter

Authors & Affiliations

Krishanu Roychowdhury1,2, D. Zeb Rocklin1,3, and Michael J. Lawler1,2,4

  • 1Laboratory of Atomic and Solid State Physics, Cornell University, Ithaca, New York 14853, USA
  • 2Kavli Institute for Theoretical Physics, University of California, Santa Barbara, California 93106-4030, USA
  • 3School of Physics, Georgia Institute of Technology, Atlanta, Georgia 30332, USA
  • 4Department of Physics, Binghamton University, Binghamton, New York 13902, USA

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Issue

Vol. 121, Iss. 17 — 26 October 2018

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