Oct 16 – 18, 2024
Karlsruhe Institute of Technology (Campus South)
Europe/Berlin timezone

R&D towards an atomic hydrogen source for future neutrino mass experiments

Oct 16, 2024, 5:31 PM
2m
Physics (Bld. 30.22) + NTI-Hörsaal (Bld. 30.10) (Karlsruhe Institute of Technology (Campus South))

Physics (Bld. 30.22) + NTI-Hörsaal (Bld. 30.10)

Karlsruhe Institute of Technology (Campus South)

Engesserstr. Karlsruhe

Speaker

Caroline Rodenbeck (Karlsruher Institut für Technologie (KIT))

Description

The neutrino mass is one of the still-to-be-solved puzzles of particle physics. Measuring the neutrino mass is possible by performing precision spectroscopy of the tritium beta-decay spectrum at its endpoint. Until now, experiments following this approach use molecular tritium and are therefore limited by the broadening of the molecular final state distribution.

For future experiments aiming for sensitivities as low as the lower boundaries obtained by neutrino oscillation experiments ( 0.05\,eV/c$^2$ in case of inverted ordering, or 0.009\,eV/c$^2$ for normal ordering), atomic tritium sources are essential.

Research on atomic tritium sources is performed at the Johannes Gutenberg University (JGU) in Mainz in the context of the Project 8 experiment and at the Tritium Laboratory Karlsruhe (TLK) of the Karlsruhe Institute of Technology (KIT) in the context of the KATRIN++ program.

Currently, the focus of the JGU group is on developing and characterizing a high-flow atomic source using inactive hydrogen, whereas the focus of the TLK group is on operating a source with tritium for the first time. Subsequently, in a joint venture, these lines of research will be merged to create the Karlsruhe Mainz Atomic Tritium experiment (KAMATE).

The poster will present the current developments for atomic sources at JGU and KIT, and how we combine them into a joint effort to realize an atomic tritium source for future neutrino mass experiments.

Primary authors

Caroline Rodenbeck (Karlsruher Institut für Technologie (KIT)) Dr Larisa Thorne (Johannes Gutenberg University Mainz)

Co-authors

Alec Lindman (Johannes Gutenberg Universität Mainz) Alexander Marsteller (KIT, IAP-TLK) Aya El Boustani (Johannes Gutenberg University Mainz) Beate Bornschein (Karlsruhe Institute of Technology, Institute for Astroparticle Physics) Brunilda Mucogllava (Johannes Gutenberg University Mainz) Christian Matthé (Johannes Gutenberg University Mainz) Daniel Kurz Darius Fenner (Johannes Gutenberg University Mainz) David Hillesheimer (Karlsruhe Institute of Technology) Elias Lütkenhorst (KIT, IAP-TLK) Fabian Piermaier (Johannes Gutenberg University Mainz) Florian Hanß (KIT, IAP-TLK) Florian Priester (KIT) Leonard Hasselmann (IAP) Dr Magnus Schlösser (Tritium Laboratory Karlsruhe - Institute of Astroparticle Physics) Dr Marco Roellig (IAP-TLK) Martin Fertl (Johannes Gutenberg University Mainz) Maxim Astaschov (Johannes Gutenberg University Mainz) Maximilian Hüneborn (Johannes Gutenberg University Mainz) Michael Sturm Dr Robin Größle (KIT) Sebastian Böser (Universität Mainz) Sebastian Koch Stefan Welte (KIT) Dr Thomas Thümmler (KIT-IAP) Tobias Geier (KIT, IAP-TLK)

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