applicationContext = Production

KATRIN and TRISTAN: Neutrinos and dark matter

The neutrino is one of the most fascinating particles in the Standard Model of particle physics. Despite important discoveries over the last ten years, a number of questions remain unanswered: How heavy is a neutrino? Is the neutrino its own antiparticle? Does the well-known left-handed neutrino have a right-handed partner? Investigating these unknown neutrino properties is the key to gaining a better understanding of the composition and evolution of the universe, and is the ultimate goal of the KATRIN/TRISTAN Research Group.


View of the KATRIN experiment
View of the KATRIN experiment (Photo: KIT)

The Karlsruhe Tritium Neutrino experiment (KATRIN) is a large-scale experiment that is currently being commissioned at Karlsruhe Institute of Technology (KIT) whose aim is the direct determination of the neutrino mass. An international research collaboration comprising around 150 members from 17 institutes in six different countries is involved in this experiment. 

The KATRIN experiment comprises an ultrahigh-intensity source of heavy hydrogen (tritium) and a high-precision spectrometer. One electron and one neutrino are emitted during the radioactive decay of the tritium atoms in the source. The energy released in this decay is randomly divided between the two particles. However, the electron can never possess all of the decay energy, as the neutrino lays claim to at least the energy that corresponds to its mass (E = mc2).

By determining the maximum energy of the electron, it is then possible to derive the mass of the neutrino. The KATRIN spectrometer is used to measure the energy of the electron produced when the tritium decays. KATRIN will be commissioned by the end of this year, and aims to determine the neutrino mass with a sensitivity of 200 millielectronvolts over the next few years. 

Our Research Group will concentrate on the upcoming data analysis and on developing a novel detector system for KATRIN, known as TRISTAN.


A TRISTAN detector module
A TRISTAN detector module (Photo: T. Bode)

Owing to its excellent source and spectrometer properties, the KATRIN experiment enables us to not only determine the neutrino mass, but also to search for a new variant of the particle: The right-handed partner of the neutrino, the so-called sterile neutrino. 

The existence of sterile neutrinos has been predicted in numerous theories, but has thus far not been confirmed experimentally. Sterile neutrinos in the mass range of a few kiloelectronvolts are suitable candidates for dark matter. 

In order to search for dark matter, KATRIN has to be equipped with a new detector and read-out system: TRISTAN (Tritium Beta Decay to Search for Sterile Neutrinos).

Our Group is heading the development of this novel silicon multi-pixel detector system. This work is being undertaken together with the Halbleiterlabor (HLL) of the Max Planck Society, Lawrence Berkeley National Laboratory, Oak Ridge National Laboratory, CEA Saclay, and Karlsruhe Institute of Technology.

In July 2016, the French COCOTE (Compact Compton Telescope) project was already using a prototype of the silicon detector, which was launched into the stratosphere attached to a balloon.

More information on the KATRIN/TRISTAN group

News releases


Aude Glaenzer and Paul Ripoche, two master students in their first year at the famous École normale supérieure de Paris-Saclay, spent four months as interns at the Max-Planck-Institute for Physics. They worked with Dr. Susanne Mertens’ KATRIN/TRISTAN group. Before they left, we asked them a couple...

Read more

Important milestone for new neutrino experiment

KATRIN detector catches sight of its first electrons

The KATRIN experiment recently celebrated its “first light”. The Karlsruhe Institute of Technology has announced that the detector has registered, for the first time, electrons that have initially flown through the 70-meter-long beamline. As the most precise measuring scale in the world, KATRIN’s...

Read more

Experimental neutrino physics – this is the main topic of a new Research Group at the Max Planck Institute for Physics. The Group will is led by Susanne Mertens, who has previously worked on the KATRIN and the Majorana experiments at the Karlsruhe Institute for Technology and Lawrence Berkeley...

Read more

Group members

name function extension www

Bode, Tobias

Scientist 401

Broussard, Leah

Scientist 373

Brunst, Tim

PhD Student 401

Edzards, Frank

PhD Student 205

Fuchs, Dominik

Student 373

Ha Minh, Martin

Student 373

Houdy, Thibaut

Scientist 560

Israel Morales Guzman, Pablo

Student 373

Karl, Christian Robert

Student 205

Keller, Stefan

Student 560

Lasserre, Thierry

Scientist 582

Mertens, Susanne, Dr.

Scientist 590

Pollithy, Anna

PhD Student 583

Roccati, Federico

Student 560

Schlueter, Lisa

Student 560

Schätz, Cornelius

Student 401

Siegmann, Daniel

Student 590

Slezak, Martin

Scientist 583

Steven, Madlen

Student 373

Willers, Michael

Scientist 401

External members

Dr. Thierry Lasserre, ICEA, France
Dr. Julieta Gruzko, UW, USA
Dr. Alexey Lokhov, RAS, Russia

Key publications

Commissioning of the vacuum system of the KATRIN Main Spectrometer
KATRIN Collaboration
Journal of Instrumentation, Volume 11, April 2016

A White Paper on keV Sterile Neutrino Dark Matter
M. Drewes, T. Lasserre, A. Merle, S. Mertens
submitted to Journal of Cosmology and Astroparticle Physics (JCAP) (2016)

Sensitivity of Next-Generation Tritium Beta-Decay Experiments for keV-Scale Sterile Neutrinos
S. Mertens, T. Lasserre, S. Groh, G. Drexlin, F. Glück, A. Huber, A. W. P. Poon, M. Steidl, N. Steinbrink, C. Weinheimer
Journal of Cosmology and Astroparticle Physics (JCAP) 1502 (2015) 02, 020

Wavelet approach to search for sterile neutrinos in tritium beta- decay spectra
S. Mertens, K. Dolde, M. Korzeczek, F. Glück, S. Groh, R. D. Martin, A. W. P. Poon, M. Steidl
Physical Review D 91 (2015) 4, 042005

Current Direct Neutrino Mass Experiments
G. Drexlin, V. Hannen, S. Mertens, C. Weinheimer
Advances in High Energy Physics, Volume 2013 (2013)