Abstract
Possible causes of magnetic oscillations with a low frequency of about 2% of the Brillouin zone, observed in high-temperature superconductors of the YBCO family, are studied. A scenario is proposed in which the observed frequency is proportional to the difference of the bilayer-split closed pockets in the Fermi surface rebuilt due to scattering to charge-density-wave vectors. A method is proposed for experimental determination of which of the four possible scenarios for the rise of these magnetic oscillations is realized in YBCO.
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Notes
Equation (9) presumes that tz(k||) ≈ const. When tz(k||) strongly depends on the direction of the momentum in the plane, Eq. (9) changes but remains an oscillating function of kFc* tan θ [52, 54].
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Funding
The work of P.D. Grigoriev was carried out within state task 0033-2019-0001 “Development of the theory of the condensed state of matter.” The work of T.I. Mogilyuk was supported by the Russian Foundation for Basic Research, grants nos. 19-02-01000, 18-32-00205, 18-02-00280, and 18-02-01022.
This work was supported in part by the Foundation for the Advancement of Theoretical Physics and Mathematics “Basis.”
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Grigoriev, P.D., Mogilyuk, T.I. & Khamzauly, A. On the Nature of Magnetic Oscillations in YBCO High-Temperature Superconductors. Phys. Solid State 61, 1529–1534 (2019). https://doi.org/10.1134/S1063783419090099
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DOI: https://doi.org/10.1134/S1063783419090099