ERIK MCLEAN / UNSPLASH

Physikalisches Kolloquium

Freitag, 16. Januar 2026 17:00 Uhr  Unveiling the early stages of planet formation

Dr. Myriam Benisty, Max-Planck-Institut für Astronomie, Heidelberg Unveiling the early stages of planet formation Dr. Myriam Benisty Max-Planck-Institut für Astronomie, Heidelberg Recent observations have revealed a surprising diversity in planetary systems, but the processes that shape them are still not fully understood. Key questions remain about how and when planets form, how they interact with their surrounding environment - the protoplanetary disk, birthplace of planets - and how these interactions affect both the planets and the disk. Protoplanetary disks evolve and dissipate as planets form, implying strong feedback between disk dynamics and planet formation. These interactions leave observable signatures in the disk structure, which are now routinely detected with high-resolution telescopes. In this talk, I will introduce the major open questions in planet formation and present recent observational results that shed light on the processes that lead to the formation of planets.

Teilchenkolloquium

Probing the Quark-Gluon Plasma with the sPHENIX experiment at RHIC

Prof. Dr. Stefan Bathe , Baruch College, CUNY, and EMMI Visiting Professor Heidelberg

Astronomisches Kolloquium

Dienstag, 20. Januar 2026 16:30 Uhr  Exoplanets, cool stars, and their interactions

Katja Poppenhäger, Leibniz-Institut für Astrophysik Potsdam (AIP) The vast majority of known exoplanets orbits their host stars at quite close distances, compared to what we are used to from our own solar system. This proximity lets exoplanets and their host stars interact in significant ways through gravitational, magnetic, and radiation fields. The various flavours of those so-called Star-Planet Interactions manifest themselves as rotational and magnetic anomalies of the host stars' behavior, as well as in some cases as dramatic atmospheric evaporation of the exoplanets. Planet-induced alterations of stellar behaviour are hard to detect observationally, since cool stars display a number of stochastic magnetic phenomena of their own, which need to be distinguished from planetary effects. However, cleverly designed experiments and a wealth of space-based and ground-based data have allowed the field to make a lot of progress over the past decade. I will show exciting new results for observations of Star-Planet Interactions in this talk, and give an outlook on the possibilities for the field in the near future. To arrange a visit with the speaker during the visit, please contact their host: Joachim Wambsganss

Zentrum für Quantendynamik Kolloquium

Mittwoch, 21. Januar 2026 16:30 Uhr  Creating and Exploring Bose-Einstein Condensates of Dipolar Molecules

Prof. Sebastian Will, Department of Physics, Columbia University of New York Creating and Exploring Bose-Einstein Condensates of Dipolar Molecules Sebastian Will, Columbia University, Department of Physics, New York, NY, USA Recently, we have realized the first BEC of dipolar molecules [1]. We evaporatively cool a gas of sodium-cesium molecules to below 10 nanokelvin, deep in the quantum degenerate regime. The BECs live for several seconds. This dramatic improvement over previous molecular cooling efforts is enabled by collisional shielding via microwave dressing, suppressing inelastic losses by four orders of magnitude [2]. Microwave dressing also provides an exceptional level of tunability of dipole-dipole interactions, opening the door to novel phases of matter in molecular quantum liquids. Most recently, we have observed self-bound droplets in a gas of strongly dipolar molecules [3]. In this talk, I will describe our experimental approach, discuss recent results, and give an outlook on novel opportunities enabled by molecular BECs for many-body quantum physics, quantum simulation, and quantum computing. I will also briefly highlight our broader efforts in quantum, including recent advances on single atom trapping in metasurface optical tweezer arrays [4]. Figure: Formation of self-bound droplets in a BEC of dipolar NaCs molecules References: [1] Bigagli, Yuan, Zhang, et al., Observation of Bose-Einstein condensation of dipolar molecules, Nature 631, 289-293 (2024) [2] Yuan, Zhang, et al., Extreme loss suppression and wide tunability of dipolar interactions in an ultracold molecular gas, arXiv:2505.08773 (2025) [3] Zhang, Yuan, et al., Observation of self-bound droplets of ultracold dipolar molecules, arXiv:2507.15208 (2025) [4] Holman, Xu, et al., Trapping of single atoms in metasurface optical tweezer arrays, arXiv:2411.05321 (2024) (in print) Bio: Sebastian Will is an Associate Professor of Physics at Columbia University. His research focuses on ultracold atoms and molecules for applications in fundamental science, quantum simulation, quantum computing, and quantum networking. He is a recipient of the Columbia RISE Award, the NSF Career Award, and a Sloan Fellowship. His research is supported by the NSF, AFOSR, ARO, ONR, DOE, and the Gordon and Betty Moore Foundation.