Karl Franzens University Graz | Graz University of Technology |
All (2002-Present) SS23 WS23 SS24 WS24 SS25 WS25 SS26
Tuesday 03 March 2026 | |
| 16:15 - 17:15 |
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Tuesday 10 March 2026 | |
| 16:15 - 17:15 |
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Tuesday 17 March 2026 | |
| 16:15 - 17:15 |
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Tuesday 24 March 2026 | |
| 16:15 - 17:15 |
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Tuesday 14 April 2026 TUG HS P2 | |
| 16:15 - 17:15 |
Correlations and dynamical screening with ab initio GW+EDMFT In this talk I will introduce the core ideas of ab initio GW+EDMFT, and review the first multi-tier implementations that made the method promising for a broad set of correlated materials (metals[1], Mott insulators[2], and semiconductors[3]). I will briefly mention how the ...more |
Tuesday 21 April 2026 | |
| 16:15 - 17:15 |
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Tuesday 28 April 2026 | |
| 16:15 - 17:15 |
Experimental modelling of “single-atom” catalysts: What defines molecular adsorption on single-metal sites? “Single-atom” catalysis (SAC) presents a recent frontier in catalysis research, promising to lower our dependence on precious metals and improve the economic viability of carbon-neutral technologies. Countless SACs were reported over the past decade, but rational design remai ...more |
Tuesday 05 May 2026 TUG HS P2 | |
| 16:15 - 17:15 |
Control and detection of broken time-reversal symmetry and Berry curvature with nonlinear optics TMDs are an ideal platform to study the interplay between space-inversion and time-reversal symmetries, which can be independently engineered by tuning the number of layers (space-inversion) and via excitation with circularly polarized light (time-reversal). In this talk, I will ...more |
Tuesday 12 May 2026 KFU - HS 05.01 | |
| 16:15 - 17:15 |
Near-field Raman Spectroscopy - via Apertures and Tips to Nanometer Resolution |
Tuesday 19 May 2026 | |
| 16:15 - 17:15 |
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Tuesday 02 June 2026 TUG HS P2 | |
| 16:15 - 17:15 |
TBA |
Tuesday 09 June 2026 KFU | |
| 16:15 - 17:15 |
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Tuesday 16 June 2026 TUG HS P2 | |
| 16:15 - 17:15 |
TBA |
Tuesday 23 June 2026 | |
| 16:15 - 17:15 |
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Tuesday 30 June 2026 TUG HS P2 | |
| 16:15 - 17:15 |
Magnetic Buoyancy – Learning from Satellite Observations of Magnetosphere Magnetic buoyancy has been known to play a role in the solar atmosphere, where it brings slender flux tubes with reduced density up through much of the convective zone. Magnetic buoyancy does operate in planetary magnetospheres, where field line curvature takes the role of gravit ...more |