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

Research output: Contribution to journalArticlepeer-review

20 Scopus citations

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.

Original languageEnglish
Article numberL012017
JournalPhysical Review Research
Volume5
Issue number1
DOIs
StatePublished - Jan 2023
Externally publishedYes

Funding

Work at Brown was supported in part by the US National Science Foundation (NSF) Grant No. DMR-1905532 and funds from Brown and the University of Bologna. S.D.W. and B.R.O. gratefully acknowledge support via the UC Santa Barbara NSF Quantum Foundry funded via the Q-AMASE-i program under award DMR-1906325. G.A., P.B., and R.D.R. acknowledge support from the University of Parma, under Bando Attrezzature 2020, HyReSpect-4 project. P.B. and R.D.R. acknowledge funding from the SUPER (Supercomputing Unified Platform - Emilia-Romagna) regional project, the National Recovery and Resilience Plan (NRRP), Mission 04 Component 2 Investment 1.5 NextGenerationEU, Call for tender No. 3277, 30/12/2021 Award 0001052, 23/06/2022 computing power form STFC's SCARF cluster and CINECA (ISCRA-C Grant No. HP10CZHPHI).

FundersFunder number
CINECAHP10CZHPHI
National Recovery and Resilience Plan0001052, 3277
UC Santa Barbara NSFDMR-1906325
National Science FoundationDMR-1905532
Science and Technology Facilities Council
Università degli Studi di Parma
Università di Bologna

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