Apr 13 – 16, 2026
KIT Campus South
Europe/Berlin timezone

Magnetic Field Simulations for the Next-Generation MMC-Based KATRIN Experiment

Apr 13, 2026, 5:13 PM
2m
Gaede Foyer (KIT Campus South)

Gaede Foyer

KIT Campus South

2nd floor (in front of Gaede-Lecture theater) Physikflachbau Building 30.22 Engesserstraße 7 76131 Karlsruhe
Poster Posters

Speaker

Carlotta Buchner (Karlsruhe Institute of Technology – Institute for Astroparticle Physics (KIT-IAP))

Description

The KATRIN experiment aims to determine the effective mass of the electron antineutrino using kinematics of the electrons from tritium $\beta$ decay. The current upper limit determined by the KATRIN experiment is $m_\nu<0.45\,\mathrm{eV}$ at 90\% confidence level (KATRIN Collaboration et al., Direct neutrino-mass measurement based on 259 days of KATRIN data. Science 388, 180-185 (2025). https://doi.org/10.1126/science.adq9592). A next-generation tritium-based experiment aims to reach sensitivity to the inverted neutrino mass ordering. For this purpose, a novel detector system based on metallic magnetic calorimeters (MMCs) is being proposed as a promising technology. To perform MMC-based spectroscopy of an electron beam, the electrons must be guided windowlessly through the main spectrometer at room temperature to a cryostat at $\mathrm{mK}$, where the $4\,\mathrm{cm^2}$ MMC-based detector will sit. Metallic microcalorimeters (MMCs) are cryogenic quantum sensors that rely on a calorimetric detection principle for single particles. The MMC-based detector is extremely sensitive to changes in the magnetic field in the $\mathrm{mT}$ region and will not work if it is exposed to temperatures exceeding the $\mathrm{mK}$ regime, as it is based on superconductivity. The development of a magnetic chicane with thermal shielding layers is necessary to guide electrons losslessly from the main spectrometer at room temperature and and rather large magnetic fields towards the MMC-based detector at $\mathrm{mK}$ and a low magnetic field on the order of $\mathrm{mT}$. Such a windowless connection between a room temperature region and a $\mathrm{mK}$ region has never been achieved. This highly motivates the design of such a chicane.

This poster will show the first ideas to realise such a magnetic chicane and will focus on the guidance of the electrons through that magnetic chicane using the simulation software Kassiopeia (https://github.com/KATRIN-Experiment/Kassiopeia.git). The software can simulate the movement of charged particles through magnetic and electric fields. Here the guidance of electrons generated by an e-gun and the tritium source used in KATRIN are analysed. These simulations are crucial for the design of the magnetic chicane.

Collaboration or Other Affiliation KATRIN

Author

Carlotta Buchner (Karlsruhe Institute of Technology – Institute for Astroparticle Physics (KIT-IAP))

Presentation materials