English

Characterization of field cage and cathode for low radioactivity operation with the CYGNO experiment

Instrumentation and Detectors 2026-04-29 v2 Instrumentation and Methods for Astrophysics High Energy Physics - Experiment

Abstract

Dark matter, which is considered to account for approximately the 27% of the Universe's energy-mass content, remains an open issue in modern particle physics along with its composition. The CYGNO Experiment aims to exploit an innovative approach applied to the direct detection search of low energy nuclear recoils possibly induced by cold particle-like dark matter candidates. CYGNO employs a directional detector based on a Time Projection Chamber (TPC) filled with a He:CF4_{4} gas mixture and equipped with an optical readout. Currently, the CYGNO Collaboration is constructing the detector demonstrator, CYGNO-04, in Hall F at Laboratori Nazionali del Gran Sasso (LNGS). This 0.4 m3^3 detector has the goal of proving the scalability of the technology and assessing the physics and radiopurity capabilities. Given the low radioactivity requirements, especially in internal components such as field cage and cathode, the reduction of material while keeping the correct electrical behavior is paramount. In this paper, we present the validation of several internal components, mainly focusing on the field cage material and support structure. The tests included geometrical asymmetries in the electric field response, collection efficiency as well as measurement of known physical quantities. A preferred configuration is found with a structure based on Nylon material which supports a PET or Kapton sheet with copper strips deposited on.

Keywords

Cite

@article{arxiv.2510.23229,
  title  = {Characterization of field cage and cathode for low radioactivity operation with the CYGNO experiment},
  author = {F. D. Amaro and R. Antonietti and E. Baracchini and L. Benussi and S. Bianco and A. Biondi and C. Capoccia and M. Caponero and L. G. M. de Carvalho and G. Cavoto and I. A. Costa and A. Croce and M. D'Astolfo and G. D'Imperio and E. Danè and G. Dho and E. Di Marco and J. M. F. dos Santos and D. Fiorina and F. Iacoangeli and Z. Islam and E. Kemp and H. P. Lima and G. Maccarrone and R. D. P. Mano and D. J. G. Marques and G. Mazzitelli and A. G. McLean and P. Meloni and A. Messina and C. M. B. Monteiro and R. A. Nobrega and I. F. Pains and E. Paoletti and L. Passamonti and F. Petrucci and S. Piacentini and D. Piccolo and D. Pierluigi and D. Pinci and A. Prajapati and F. Renga and F. Rosatelli and A. Russo and G. Saviano and P. A. O. C. Silva and N. J. Spooner and R. Tesauro and S. Tomassini and S. Torelli and D. Tozzi},
  journal= {arXiv preprint arXiv:2510.23229},
  year   = {2026}
}