ERIK MCLEAN / UNSPLASH

Physikalisches Kolloquium

Friday, 24. January 2025 5:00 pm  Ultrafast Dynamics in Hybrid Semiconductors for Energy Applications

Prof. Dr. Felix Deschler, Institute of Physical Chemistry, University of Heidelberg

Addressing the climate challenge requires functional materials that enable energy generation, storage, and conversion from renewable sources, forming the foundation for a sustainable energy infrastructure. My group focuses on advancing functional materials to enable novel energy technologies, including next-generation lighting, energy storage, and information systems. We leverage high-resolution ultrafast spectroscopy to investigate the dynamics of local optoelectronic and structural processes at femtosecond timescales. This approach not only advances material functionality but also provides new insights into fundamental phenomena critical for energy applications.

In this talk, I will discuss how we use advanced spectroscopic techniques to explore the ultrafast dynamics of photoexcited electronic states, spin populations, and atomic structure in hybrid perovskite semiconductors. Our research elucidates the origins of the exceptional optoelectronic properties of these materials, which have positioned them at the forefront of solution-processable semiconductors. I will present results on spatio-temporal imaging of excitations via ultrafast transient microscopy, as well as spin dynamics using ultrafast Faraday rotation microscopy. Additionally, I will highlight recent findings on chiral hybrid perovskites for manipulating spin-orbit interactions, and dynamics of opto-ionic excited state reservoirs with implications for neuromorphic computing. Finally, I will extend the discussion to further material systems, such as bismuth vanadate photocatalysts and organic semiconductors, demonstrating the broad applicability of our approach for investigating material dynamics.

Astronomy colloquium

Tuesday, 7. January 2025 4:30 pm  The origin of interstellar dust: from local supernovae to the high-redshift Universe

Professor Ilse De Looze, University of Ghent The interstellar medium of galaxies from the local to high-redshift Universe is pervaded with dust. Yet, the dominant dust formation and evolution mechanisms remain poorly constrained. Stellar sources such as asymptotic giant branch stars and supernovae are known dust producers, but the efficient dust destruction by supernova shocks could impose the need for an additional dust production source accounting for dust grains forming in situ in the ISM.   In this talk, I will review recent observational and numerical efforts that scrutinise the efficiency of supernova dust formation and destruction processes, and other dust production sources. I will also give an extensive overview of new exciting JWST observations of nearby supernovae, including the detection of a puzzling newly identified dusty structure that dominates the mid-infrared emission in the central regions of Cassiopeia A.  Thanks to the combined strengths of JWST and ALMA, we start probing the rise of metals and dust in the early Universe, where supernovae are thought to play an important role. Modelling the chemical build-up of metals and dust in these first galaxies, and in galaxies in the nearby Universe, gives us a unique perspective on the contributions of different dust sources and sinks, and on the baryonic cycling of dusty material in and out of galaxies. I will conclude my talk with a summary of exciting new observational inferences of dust across cosmic time. Those unable to attend the colloquium in person are invited to participate online through Zoom (Meeting ID: 942 0262 2849, passcode 792771) using the link: https://eu02web.zoom-x.de/j/94202622849?pwd=dGlPQXBiUytzY1M2UE5oUDRhbzNOZz09 During her visit to Heidelberg, Professor de Looze will be available for meetings by arrangement with her host, Kathryn Kreckel(Kathryn.kreckel@uni-heidelberg.de).

Center for Quantum Dynamics Colloquium

Wednesday, 22. January 2025 4:30 pm  tba

Prof. Hélène Perrin , Laboratoire de Physique des Lasers, CNRS, Université Paris Nord