Bulletin of the American Physical Society
APS New England Section (NES) Annual Meeting 2025
Friday–Saturday, November 7–8, 2025; Brown University, Providence, Rhode Island
Session A01: Condensed Matter Physics I
12:30 PM–2:30 PM,
Friday, November 7, 2025
Brown University
Room: Pembroke Hall: Room 305
Chair: Lucas Caretta, Brown University
Abstract: A01.00003 : Microscopic Evidence for π-Trihexagonal Charge Density Wave in CsV3Sb5 from NQR and DFT
1:18 PM–1:30 PM
Presenter:
Ginevra Corsale
(Brown University)
Authors:
Ginevra Corsale
(Brown University)
Giuseppe Allodi
(Università degli Studi di Parma)
Ilija K. Nikolov
(Brown University)
ANSHU KATARIA
(Università degli Studi di Parma)
Pietro Bonfa'
(Università degli Studi di Modena e Reggio Emilia)
Samuele Sanna
(Alma Mater Studiorum – Università di Bologna)
Vesna F Mitrovic
(Brown University)
The recently discovered vanadium-based Kagome materials AV3Sb5 (A = Cs, K, Rb) are no exception, exhibiting unconventional superconductivity and a distinctive charge density wave (CDW) order.
Determining the CDW ground state structure remains challenging because of conflicting findings. Ultrafast time-resolved reflectivity measurements suggest a coexistence of a Star of David (SoD) and inverse Star of David (ISD) patterns[1], while 51V nuclear magnetic resonance results detect an SoD pattern [2]. Finally, synchrotron x-ray diffraction measurements detected the 2×2×2 ISD structure, which upon cooling becomes the 2×2×4 structure composed of a three-layer ISD and an SoD layer [3].
In this work, we focus on CsV3Sb5 and track the evolution of the local charge distribution and structural configuration using a combination of nuclear quadrupole resonance (NQR) and density functional theory (DFT).
By examining the temperature evolution of the 121Sb NQR spectrum, we identify the transition to the CDW state. Furthermore, we simulate the NQR spectrum for different CDW patterns and extract all the relative features. A comparison of the theoretical and experimental spectral features reveals that the ISD structure with a π-shift along the c-axis is the most stable distortion pattern.
[1] Q. Den et al. Coherent phonon pairs and rotational symmetry breaking of charge density wave order in the kagome metal CsV3Sb5 . arXiv:2503.07442, 2025.
[2] J. Luo et al. Possible star-of-david pattern charge density wave with additional modulation in the kagome superconductor CsV3Sb5. npj Quantum Materials, vol. 7, Mar. 2022.
[3] L. Kautzsch et al. Structural evolution of the kagome superconductors AV3Sb5 (A = Cs, K, Rb) through charge density wave order. Physical Review Materials, vol. 7, Feb. 2023.
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