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Rosseland Lecture 2026: The dark matter puzzle

Each spring, near the date of Svein Rosseland's birthday, the Institute of Theoretical Astrophysics invites everyone to a guest lecture as a remembrance for the great astrophysicist Svein Rosseland (1894-1985), founder of our institute.

 A field of galaxies in space, dominated by an enormous, bright-white elliptical galaxy that is the core of a massive galaxy cluster. Many other elliptical galaxies can be seen around it. Also around it are short, curved, glowing red lines, which are images of distant background galaxies magnified and warped by gravitational lensing. A couple of foreground stars appear large and bright with long spikes around them.

James Webb Space Telescope's image of the central galaxy cluster Abell S1063. This behemoth collection of galaxies, lying 4.5 billion light-years from Earth in the constellation Grus (the Crane), dominates the scene. Looking more closely, this dense collection of heavy galaxies is surrounded by red streaks of light: these warped arcs are in fact faint galaxies from the Universe’s distant past. They are visible due to brightening and magnification as a result of gravitational lensing from the combined mass of the galaxy cluster. It can only be explained if the cluster is dominated by an enormous amount of invisible mass: dark matter.

Photo: ESA/Webb, NASA & CSA, H. Atek, M. Zamani (ESA/Webb)

The dark matter puzzle

The problem of missing mass in the Universe, at the scale of galaxies, large-scale structures, and its global content, is a multi-faceted enigma. In the cold dark matter scenario, one of the main candidates for the exotic particles, is the neutralino, the most stable of the super-symmetric particles. However, supersymmetry does not appear as expected in the Large Hadron Collider experiments at CERN. 

Many other models have blossomed in recent years, I will describe some alternatives such as axions, sterile neutrinos, or modified gravity.

The Rosseland Lecturer 2026

This year’s Rosseland Lecture will be held by Professor Françoise Combes, Emeritus Professor at Collège de France, chair of “Galaxies and cosmology”, and president of the French Academy of Sciences for 2025-2026.

portrait photo of a woman with dark, short hair and glasses
Professor Françoise Combes. © Frédérique PLAS / CNRS

Combes works at the Paris Observatory on the formation and evolution of galaxies, their dynamics and their co-evolution with supermassive black holes, as well as on models of dark matter. 

She has received several awards, including the CNRS Gold Medal (2020), the international L'Oreal-Unesco award for Women in Science (2021), and the Gothenburg Lise Meitner Award from the Gothenburg Physics Centre (2017).

Combes was elected member of the European Academy (2009) and international member of the National Academy of Sciences (USA, 2023).


The Rosseland Lecture 2026 will be held on Friday the 8th of May at 15:15 in the Science Library in Vilhelm Bjerknes’ hus at Blindern, University of Oslo.

Coffee and cakes will be served from 14:45. Welcome!

The Rosseland Lecture

The Rosseland Lecture is held annually by the Institute of Theoretical Astrophysics, University of Oslo, in memory of Norway’s foremost astrophysicist, and founder of our institute, Professor Svein Rosseland (1894 – 1985). The Rosseland Lecturers are internationally renowned, outstanding astrophysicists. The Rosseland Lectures hold a semi-popular level and are open for all.

The lecture will be streamed on YouTube channel of the Science Library.

Tags: Cosmology, Astrophysics, Rosseland Lecture, Dark Matter
Published Feb. 24, 2026 5:09 PM - Last modified Apr. 30, 2026 4:15 PM