Nickelate superconductivity without doping at 100 GPa in PrNiO2
ORAL
Abstract
The discovery of superconductivity in infinite layer nickelates [1] has raised the hope for a better understanding of superconductivity in strongly correlated systems. Dynamical vertex approximation (DΓA) successfully predicted [2] the experimental phase diagram [3]. When applying a pressure of 12 GP, the superconducting critical temperature (Tc) of PrNiO2 further increases to over 30 K [4].
Here we show in DΓA calculations [5] that even higher Tc's are possible if the ratio bandwidth-to-interaction is increased [5]. One way to achieve this is pressure, were we find (i) good agreement with [4], (ii) a further increase of Tc at higher pressures, and (iii) that superconductivity is possible even without doping in PrNiO2 at a pressure slightly above 100 GPa. The last is due to the self-doping effect of the electron pockets. Another promising route we [5] identified to increase the bandwidth and Tc is to move from 3d nickelates to 4d palladates.
[1] D. Li et al., Nature 573, 624 (2019).
[2] M. Kitatani et al., npj Quantum Materials 5, 59 (2020).
[3] K. Lee et al. arXiv:2203.02580
[4] N. N. Wang et al, Nature Communications 13, 4367 (2022).
[5] M. Kitatani et al., Phys. Rev. Lett. 130, 166002 (2023).
Here we show in DΓA calculations [5] that even higher Tc's are possible if the ratio bandwidth-to-interaction is increased [5]. One way to achieve this is pressure, were we find (i) good agreement with [4], (ii) a further increase of Tc at higher pressures, and (iii) that superconductivity is possible even without doping in PrNiO2 at a pressure slightly above 100 GPa. The last is due to the self-doping effect of the electron pockets. Another promising route we [5] identified to increase the bandwidth and Tc is to move from 3d nickelates to 4d palladates.
[1] D. Li et al., Nature 573, 624 (2019).
[2] M. Kitatani et al., npj Quantum Materials 5, 59 (2020).
[3] K. Lee et al. arXiv:2203.02580
[4] N. N. Wang et al, Nature Communications 13, 4367 (2022).
[5] M. Kitatani et al., Phys. Rev. Lett. 130, 166002 (2023).
* This work has been supported throught he Austrian Science funds (FWF) project ID 5398.
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Publication: M. Kitatani et al., Phys. Rev. Lett. 130, 166002 (2023).
S. di Cataldo et al., in preparation.
Presenters
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Karsten Held
TU Wien, TU Vienna
Authors
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Karsten Held
TU Wien, TU Vienna
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Simone Di Cataldo
TU Wien
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Liang Si
Northwestern University, China
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Motoharu Kitatani
Hyogo University