Possible breaking of the Pauli limit in Sn1-xInxTe/III-V heterostructures
ORAL
Abstract
Sn1-xInxTe has been synthesized and studied as a candidate topological superconductor. In recent years, scientists start to explore its thin film form. Up to now, the superconducting behavior in Sn1-xInxTe seems to follow traditional BCS theory.
Here we report transport studies of Sn1-xInxTe/(Ga,In)(As,Sb), grown by molecular beam epitaxy. Band bending between two layers causes a depletion region at the interface. By varying the composition of (Ga,In)(As,Sb), we are able to tune the strength of band bending and modify the superconducting properties of Sn1-xInxTe. Interestingly, we have observed a breaking of the Pauli limit in Sn0.7In0.3Te/Ga0.52In0.48Sb heterostructure. Meanwhile, Pauli limit is preserved in Sn0.7In0.3Te layers grown on wide-gap BaF2 substrate, where no band bending occurs. The result indicates the existence of unconventional superconductivity emerging on Sn1-xInxTe in the 2D limit. Our work has also shown a possible way of engineering the superconducting properties by band bending.
Here we report transport studies of Sn1-xInxTe/(Ga,In)(As,Sb), grown by molecular beam epitaxy. Band bending between two layers causes a depletion region at the interface. By varying the composition of (Ga,In)(As,Sb), we are able to tune the strength of band bending and modify the superconducting properties of Sn1-xInxTe. Interestingly, we have observed a breaking of the Pauli limit in Sn0.7In0.3Te/Ga0.52In0.48Sb heterostructure. Meanwhile, Pauli limit is preserved in Sn0.7In0.3Te layers grown on wide-gap BaF2 substrate, where no band bending occurs. The result indicates the existence of unconventional superconductivity emerging on Sn1-xInxTe in the 2D limit. Our work has also shown a possible way of engineering the superconducting properties by band bending.
* Research supported by DMR-1905277, and partly by CRDF.
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Presenters
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Jiashu Wang
Department of Physics and Astronomy, University of Notre Dame, University of Notre Dame
Authors
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Jiashu Wang
Department of Physics and Astronomy, University of Notre Dame, University of Notre Dame
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Logan S Riney
University of Notre Dame
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Hao Li
Purdue University
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Leonid P Rokhinson
Purdue University
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Xinyu Liu
Department of Physics and Astronomy, University of Notre Dame, University of Notre Dame
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Badih A Assaf
Department of Physics and Astronomy, University of Notre Dame, University of Notre Dame