English

A Demonstration of Slowed Electron ${\bf E} \times {\bf B}$ Drift for PTOLEMY

Instrumentation and Detectors 2025-07-11 v6

Abstract

To resolve the effective neutrino mass mβm_\beta with an energy resolution of 50~meV, the PTOLEMY experiment has proposed a novel transverse electromagnetic filtering process. Substantially reducing the kinetic energy of tritium β\beta-decay electrons by counteracting motion from E{\bf E} ×\times B{\bf B} and B\nabla{\rm B} drift, the PTOLEMY filter requires an input of emitted electron kinematic information to generate a tailored, suitable electric field for each candidate. The collaboration proposes to extract these quantities by using antennae to observe the relativistic frequency shift of emitted cyclotron radiation as an electron transits by E{\bf E} ×\times B{\bf B} drift through a uniform magnetic field region preceding the filter. Electrons must be contained within this region long enough such that an adequate integrated radiated power signal is received to accurately estimate these kinematics. This necessitates a controlled, slowed drift speed. This paper presents the experimental design to vary E{\bf E} ×\times B{\bf B} drift speed of carbon-14 β\beta-decay electrons using a custom electrode field cage situated between the pole faces of an electromagnet. Matching our results with high-fidelity simulation, we deduce a capacity to increase particle time of flight by a factor of 5 in the field cage's slow drift region. Limited only by the dimensions of our system, we assert drift speed can be arbitrarily slowed to meet the needs of PTOLEMY's future detector. Actualizing such a system is a crucial milestone in developing the detector, enabling future cyclotron radiation measurements, filter implementation, and source injection.

Keywords

Cite

@article{arxiv.2503.10025,
  title  = {A Demonstration of Slowed Electron ${\bf E} \times {\bf B}$ Drift for PTOLEMY},
  author = {M. Farino and A. Tan and A. Apponi and M. Betti and M. Borghesi and A. Casale and O. Castellano and G. Cavoto and L. Cecchini and E. Celasco and W. Chung and A. G. Cocco and A. Colijn and B. Corcione and N. D'Ambrosio and N. de Groot and S. el Morabit and A. Esposito and M. Faverzani and A. D. Ferella and E. Ferri and L. Ficcadenti and S. Gamba and S. Gariazzo and H. Garrone and F. Gatti and A. Giachero and Y. Iwasaki and A. Kievsky and F. Malnati and G. Mangano and L. E. Marcucci and C. Mariani and J. Mead and G. Menichetti and M. Messina and E. Monticone and M. Naafs and A. Nucciotti and L. Origo and F. Pandolfi and D. Paoloni and C. Pepe and C. Pérez de los Heros and O. Pisanti and F. M. Pofi and A. D. Polosa and I. Rago and M. Rajteri and N. Rossi and A. Ruocco and S. Tayyab and V. Tozzini and C. Tully and I. van Rens and F. Virzi and G. Visser and M. Viviani and U. Zeitler and O. Zheliuk and F. Zimmer},
  journal= {arXiv preprint arXiv:2503.10025},
  year   = {2025}
}

Comments

31 pages, 32 figures