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Microscopic nature of the charge-density wave in the kagome superconductor RbV3Sb5

Jonathan Frassineti, Pietro Bonfà, Giuseppe Allodi, Erick Garcia, Rong Cong, Brenden R. Ortiz, Stephen D. Wilson, Roberto De Renzi, Vesna F. Mitrović, Samuele Sanna

DOI 10.1103/PhysRevResearch.5.L012017 · Physical Review Research

T1

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Abstract

The recently discovered vanadium-based Kagome metals AV3Sb5 (A = K, Rb, Cs) undergo a unique phase transition into charge-density wave (CDW) order which precedes both unconventional superconductivity and time-reversal symmetry breaking. Therefore the essential first step in building a full understanding of the role of CDW in establishing these unconventional phases is to unveil the symmetries and the microscopic nature of the charge-ordered phase. Here, we determine the exact structure of the 2×2×2 superlattice that develops below the charge-density wave ordering temperature (TCDW) in RbV3Sb5. We present a comprehensive set of V51, Rb87, and Sb121 nuclear magnetic resonance (NMR) measurements and density functional theory simulations of NMR observables to provide a unique site-selective view into the local nature of the charge-ordered phase. The combination of these experimental results with simulations provides compelling evidence that the CDW structure prevailing below 103 K in RbV3Sb5 is the so-called inverse Star of David pattern, π-shifted along the c axis. These findings put severe constraints on the topology of these Kagome compounds and thus provide essential guidance for the development of an appropriate theoretical framework for predicting properties of exotic electronic orders arising within the CDW phase.

Source-reported materials — not catalogue approval

FormulaReported Tc (K)Pressure (GPa)Type
RbV3Sb5

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2.5Pressure not reportedunknown
KV3Sb5

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Source-occurrence policy only; no material identity or catalogue acceptance is inferred from the formula.

2.5Pressure not reportedunknown
CsV3Sb5

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2.5Pressure not reportedunknown

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