When Charge Order Meets Superconductivity: Insights from Transition-Metal Dichalcogenides

25 Mar 2026, 13:30
30m
Albano 3: 4204 - SU Conference Room (56 seats) (Albano Building 3)

Albano 3: 4204 - SU Conference Room (56 seats)

Albano Building 3

AlbaNova Univ. Center Hannes Alfvéns väg 12 SE-106 91 Stockholm Sweden
56

Speaker

Yasmine Sassa (Royal Institute of Technology, KTH)

Description

Quantum materials have emerged as a rich platform to explore novel electronic phases that arise from strong interactions between electrons and the lattice. Among these systems, transition-metal dichalcogenides have attracted particular interest because they host both charge-density-wave order and superconductivity, two collective phenomena that often coexist and compete.
In this talk I will present our recent experimental efforts to investigate the microscopic origin of charge order and its relation to superconductivity in layered dichalcogenides. Using a combination of muon spin rotation (μSR), inelastic x-ray scattering (IXS), and angle-resolved photoemission spectroscopy (ARPES), we probe both the lattice dynamics and the superconducting ground state in these materials.
First, I will discuss our studies of the charge-density-wave transition in 2H-TaS₂. Momentum-resolved phonon measurements reveal a strongly localized Kohn anomaly associated with the charge order, while ARPES measurements show the opening of a sizeable electronic gap at the transition. Together these results highlight the central role of electron–phonon coupling and lattice dynamics in driving the ordered state. I will then present μSR measurements of the superconducting phase of 2H-TaS₂, demonstrating that the superconductivity is consistent with a conventional nodeless BCS-like state.
Finally, I will show how superconductivity evolves when charge order is suppressed in 1T-TiSe₂ under pressure. Our μSR measurements reveal a two-gap superconducting state, where the superfluid density is strongly enhanced near a Lifshitz transition associated with changes in the Fermi surface.

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