My research within the group focuses on cosmic relic neutrinos and the possibility of a direct detection using neutrino capture on tritium. The precision data collected by the KATRIN experiment enable us to explore the relic neutrino parameter space with a projected sensitivity of approximately η < 10¹⁰.^[1]

Moreover, I am interested in exploring new ideas for next-generation neutrino experiments that can determine the neutrino mass with unprecedented sensitivity.

In the past, my work focused on analyzing KATRIN neutrino mass data using both frequentist and Bayesian methods, resulting in an upper limit of m_ν < 0.45 eV (90% CL).^[2]

[1] KATRIN Collaboration. Phys. Rev. Lett. 129, 011806 (2022).

[2] KATRIN Collaboration. Science 388, 180-185 (2025).