Frontiers in Physics (May 2024)
Background discrimination with a Micromegas detector prototype and veto system for BabyIAXO
- K. Altenmüller,
- J. F. Castel,
- S. Cebrián,
- T. Dafni,
- D. Díez-Ibañez,
- A. Ezquerro,
- E. Ferrer-Ribas,
- J. Galan,
- J. Galindo,
- J. Galindo,
- J. A. García,
- A. Giganon,
- C. Goblin,
- I. G. Irastorza,
- C. Loiseau,
- G. Luzón,
- X. F. Navick,
- C. Margalejo,
- H. Mirallas,
- L. Obis,
- A. Ortiz de Solórzano,
- T. Papaevangelou,
- O. Pérez,
- A. Quintana,
- A. Quintana,
- J. Ruz,
- J. K. Vogel,
- J. K. Vogel
Affiliations
- K. Altenmüller
- Center for Astroparticles and High Energy Physics (CAPA), Universidad de Zaragoza, Zaragoza, Spain
- J. F. Castel
- Center for Astroparticles and High Energy Physics (CAPA), Universidad de Zaragoza, Zaragoza, Spain
- S. Cebrián
- Center for Astroparticles and High Energy Physics (CAPA), Universidad de Zaragoza, Zaragoza, Spain
- T. Dafni
- Center for Astroparticles and High Energy Physics (CAPA), Universidad de Zaragoza, Zaragoza, Spain
- D. Díez-Ibañez
- Center for Astroparticles and High Energy Physics (CAPA), Universidad de Zaragoza, Zaragoza, Spain
- A. Ezquerro
- Center for Astroparticles and High Energy Physics (CAPA), Universidad de Zaragoza, Zaragoza, Spain
- E. Ferrer-Ribas
- Université Paris-Saclay, CEA, IRFU, Gif-sur-Yvette, France
- J. Galan
- Center for Astroparticles and High Energy Physics (CAPA), Universidad de Zaragoza, Zaragoza, Spain
- J. Galindo
- Center for Astroparticles and High Energy Physics (CAPA), Universidad de Zaragoza, Zaragoza, Spain
- J. Galindo
- Instituto Tecnológico de Aragón (ITA), Zaragoza, Spain
- J. A. García
- Center for Astroparticles and High Energy Physics (CAPA), Universidad de Zaragoza, Zaragoza, Spain
- A. Giganon
- Université Paris-Saclay, CEA, IRFU, Gif-sur-Yvette, France
- C. Goblin
- Université Paris-Saclay, CEA, IRFU, Gif-sur-Yvette, France
- I. G. Irastorza
- Center for Astroparticles and High Energy Physics (CAPA), Universidad de Zaragoza, Zaragoza, Spain
- C. Loiseau
- Université Paris-Saclay, CEA, IRFU, Gif-sur-Yvette, France
- G. Luzón
- Center for Astroparticles and High Energy Physics (CAPA), Universidad de Zaragoza, Zaragoza, Spain
- X. F. Navick
- Université Paris-Saclay, CEA, IRFU, Gif-sur-Yvette, France
- C. Margalejo
- Center for Astroparticles and High Energy Physics (CAPA), Universidad de Zaragoza, Zaragoza, Spain
- H. Mirallas
- Center for Astroparticles and High Energy Physics (CAPA), Universidad de Zaragoza, Zaragoza, Spain
- L. Obis
- Center for Astroparticles and High Energy Physics (CAPA), Universidad de Zaragoza, Zaragoza, Spain
- A. Ortiz de Solórzano
- Center for Astroparticles and High Energy Physics (CAPA), Universidad de Zaragoza, Zaragoza, Spain
- T. Papaevangelou
- Université Paris-Saclay, CEA, IRFU, Gif-sur-Yvette, France
- O. Pérez
- Center for Astroparticles and High Energy Physics (CAPA), Universidad de Zaragoza, Zaragoza, Spain
- A. Quintana
- Center for Astroparticles and High Energy Physics (CAPA), Universidad de Zaragoza, Zaragoza, Spain
- A. Quintana
- Université Paris-Saclay, CEA, IRFU, Gif-sur-Yvette, France
- J. Ruz
- Center for Astroparticles and High Energy Physics (CAPA), Universidad de Zaragoza, Zaragoza, Spain
- J. K. Vogel
- Center for Astroparticles and High Energy Physics (CAPA), Universidad de Zaragoza, Zaragoza, Spain
- J. K. Vogel
- LLNL Lawrence Livermore National Laboratory, Livermore, CA, United States
- DOI
- https://doi.org/10.3389/fphy.2024.1384415
- Journal volume & issue
-
Vol. 12
Abstract
In this paper we present measurements performed with a Micromegas X-ray detector setup. The detector is a prototype in the context of the BabyIAXO helioscope, which is under construction to search for an emission of the hypothetical axion particle from the Sun. An important component of such a helioscope is a low background X-ray detector with a high efficiency in the 1–10 keV energy range. The goal of the measurement was to study techniques for background discrimination. In addition to common techniques we used a multi-layer veto system designed to tag cosmic-ray induced neutron background. Over an effective time of 52 days, a background level of 8.6 × 10−7 counts keV−1 cm−2 s−1 was reached in a laboratory at above ground level. This is the lowest background level achieved at surface level. In this paper we present the experimental setup, show simulations of the neutron-induced background, and demonstrate the process to identify background signals in the data. Finally, prospects to reach lower background levels down to 10–7 counts keV−1 cm−2 s−1 are discussed.
Keywords
- axions
- rare event search
- TPC (time projection chamber)
- background discrimination
- x-ray detector
- ultra low background