Fermi-surface reconstruction under pressure in the cuprate superconductors YBCO and Nd-LSCO
ORAL
Abstract
It is well established by now that the Fermi surface of hole-doped cuprates such as YBCO [1], Eu-LSCO [2], Nd-LSCO [3] and Hg1201 [4] undergoes a reconstruction caused by the emergence of charge order at low temperature. Here we show how the process of Fermi-surface reconstruction evolves as a function of applied hydrostatic pressure in both YBCO and Nd-LSCO, via measurements of the resistivity and Hall coefficient as a function of temperature and magnetic field. \\[4pt] [1] D. LeBoeuf \textit{et al}., Physical Review B \textbf{83}, 054506 (2011). \\[0pt] [2] F. Lalibert\'{e} \textit{et al}., Nature Communications \textbf{2}, 432 (2011). \\[0pt] [3] R. Daou \textit{et al}., Nature Physics \textbf{5}, 31 (2009). \\[0pt] [4] N. Doiron-Leyraud \textit{et al}., Physical Review X \textbf{3}, 021019 (2013).
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