ERIK MCLEAN / UNSPLASH

Physikalisches Kolloquium

Friday, 14. November 2025 5:00 pm  News from Wendelstein 7-X: Towards Clean Energy from Fusion

Prof. Dr. Thomas Klinger , Max-Planck-Institut für Plasmaphysik, Garching High performance steady state fusion plasmas in the superconducting stellarator device Wendelstein 7-X T. Klinger, Greifswald/Germany Max-Planck Institute for Plasma Physics, Wendelsteinstrasse 1, 117489 Greifswald The stable generation of high-temperature and low-density hydrogen plasmas (ion and electron temperature in the range 10-20 keV resp. 100-200 million degree Kelvin) is the basis for the use of nuclear fusion to generate heat and electric power. The most promising path is to use strong, toroidally shaped, twisted magnetic fields to confine the electrically charged plasma particles in order to avoid heat losses to the cold, solid wall elements. Two magnetic confinement concepts have proven being most suitable: (a) the tokamak and (b) the stellarator. The stellarator creates the magnetic field by external coils only, the tokamak by combining the externally created field with the magnetic field generated by a strong current in the plasma. “Wendelstein 7-X” is the most advanced large superconducting stellarator that operates at the Max Planck Institute in Greifswald. With 30 m3 plasma volume, 3 T magnetic field on axis, and 10 MW micro wave plasma heating power, hydrogen plasmas are generated that allow one to establish a technical and scientific basis for the extrapolation to a future fusion power plant. It is a unique feature of Wendelstein 7-X to be able to operate high-power hydrogen plasmas under steady-state conditions, more specifically for 1800 s (note that the world standard is now in the 10 s ballpark). Furthermore, Wendelstein 7-X has recently proven to be at par with tokamak plasma performance for long discharges. This talk provides a brief review of the principles of nuclear fusion and discusses the key physics subjects of optimized stellarators. We summarize the most important findings of the previous performance operation campaigns and put them into the international context of fusion research. An outlook is given towards fusion power as a building block of future energy supply of the world. [1] National Geographic, November Issue 2025 https://www.nationalgeographic.com/science/article/stars-nuclear-fusion-energy [1] T. Klinger et al., Nuclear Fusion 2019, 59(11) 112004 [2] A. Dinklage et al., Nature Physics 2018, 14(8) 855

Particle Colloquium

Briefing Book for the European Strategy

Prof. Dr. Monica Dunford, Kirchhoff Institut für Physik

Astronomy colloquium

Tuesday, 4. November 2025 4:30 pm  Weighing the Universe with the Lightest Elements

Max Pettini, Institute of Astronomy, University of Cambridge In the era of `Precision Cosmology' remarkable advances have been made in the determination of cosmological parameters from the Cosmic Microwave Background and Big Bang Nucleosynthesis, with spectacular concordance between these two pillars of the Standard Cosmological Model. While much exposure has been given to the impressive results from the WMAP and Planck missions, perhaps less attention has been paid to the equally striking advances made in the last ten years in the measurements of the abundances of the light elements forged in the first few minutes of our Universe history. In this talk I shall focus in particular on the determination of the primordial abundance of deuterium, in an overview that spans almost 80 years, from the first seeds of the idea sown in the 1940s to the most recent results and forward look to the era of Extremely Large Telescopes and next generation Wide Field Surveys of the sky. To arrange a visit with the speaker during the visit, please contact their host: Eduardo Banados

Center for Quantum Dynamics Colloquium

Wednesday, 12. November 2025 4:30 pm  tba

Dr. Rob Smith, Department of Physics, University of Oxford