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https://hdl.handle.net/10356/179639
Title: | Midgap states induced by Zeeman field and p-wave superconductor pairing | Authors: | Jin, Yuanjun Yue, Xingyu Xu, Yong Yu, Xiang-Long Chang, Guoqing |
Keywords: | Physics | Issue Date: | 2024 | Source: | Jin, Y., Yue, X., Xu, Y., Yu, X. & Chang, G. (2024). Midgap states induced by Zeeman field and p-wave superconductor pairing. Physical Review B, 109(24), L241101-. https://dx.doi.org/10.1103/PhysRevB.109.L241101 | Project: | NRF-NRFF13-2021-0010 M23M6c0100 MOET2EP50222-0014 NTU SUG |
Journal: | Physical Review B | Abstract: | The one-dimensional Su-Schrieffer-Heeger (SSH) model is central to band topology in condensed matter physics, which allows us to understand and design distinct topological states. In this work we find another mechanism to analogize the SSH model in a spinful system, realizing an obstructed atomic insulator by introducing intrinsic spin-orbit coupling and in-plane Zeeman field. In our model the midgap states originate from a quantized hidden polarization with invariant index Z2 (0; 01) due to the local inversion symmetry breaking. When the global inversion symmetry is broken, a charge pumping is designed by tuning the polarization. Moreover, by introducing the p+ip superconductor pairing potential, a topological phase dubbed obstructed superconductor (OSC) is identified. This new state is characterized by invariant index Z2 (0; 01) and nonchiral midgap states. More interestingly, these nonchiral edge states result in a chiral-like nonlocal conductance, which is different from the traditional chiral topological superconductor. Our findings not only find another strategy to achieve a spinful SSH model but also predict the existence of OSC, providing a promising avenue for further exploration of its transport properties. | URI: | https://hdl.handle.net/10356/179639 | ISSN: | 2469-9950 | DOI: | 10.1103/PhysRevB.109.L241101 | Schools: | School of Physical and Mathematical Sciences | Rights: | © 2024 American Physical Society. All rights reserved. This article may be downloaded for personal use only. Any other use requires prior permission of the copyright holder. The Version of Record is available online at http://doi.org/10.1103/PhysRevB.109.L241101 | Fulltext Permission: | open | Fulltext Availability: | With Fulltext |
Appears in Collections: | SPMS Journal Articles |
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PhysRevB.109.L241101.pdf | 1.08 MB | Adobe PDF | View/Open |
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