- Open Access
- Access by Xinjiang University
Sensitivity of MAGIX@MESA to BSM effects via Bethe-Heitler pair production
Phys. Rev. D 114, 035034 – Published 24 August, 2026
DOI: https://doi.org/10.1103/bgx7-19gt
Abstract
We explore the sensitivity of the upcoming MAGIX experiment at the MESA facility to light Beyond the Standard Model (BSM) mediators in the few to hundred MeV mass range. Utilizing high-intensity electron beams of 55 MeV and 105 MeV on a heavy target, we investigate the production of scalar, pseudoscalar, vector, and axial vector mediators via the Bethe-Heitler process. By optimizing the asymmetric kinematic acceptance of the double-spectrometer setup to enhance the signal over background ratio, we demonstrate that MAGIX can probe mediator-electron couplings down to , offering a competitive probe of the dark sector in the sub-GeV mass range.
Physics Subject Headings (PhySH)
Article Text
References (32)
- G. Bertone, D. Hooper, and J. Silk, Phys. Rep. 405, 279 (2005).
- N. Aghanim et al. (Planck Collaboration), Astron. Astrophys. 641, A6 (2020); 652, C4(E) (2021).
- A. J. Krasznahorkay et al., Phys. Rev. Lett. 116, 042501 (2016).
- A. J. Krasznahorkay, M. Csatlós, L. Csige, J. Gulyás, A. Krasznahorkay, B. M. Nyakó, I. Rajta, J. Timár, I. Vajda, and N. J. Sas, Phys. Rev. C 104, 044003 (2021).
- F. Bossi et al. (PADME Collaboration), J. High Energy Phys. 11 (2025) 007.
- B. Holdom, Phys. Lett. 166B, 196 (1986).
- M. Pospelov, A. Ritz, and M. B. Voloshin, Phys. Lett. B 662, 53 (2008).
- A. Ringwald, Phys. Dark Universe 1, 116 (2012).
- K. Baker et al., Ann. Phys. (Berlin) 525, A93 (2013).
- M. Bauer, M. Neubert, and A. Thamm, J. High Energy Phys. 12 (2017) 044.
- S. Knapen, T. Lin, and K. M. Zurek, Phys. Rev. D 96, 115021 (2017).
- M. Fabbrichesi, E. Gabrielli, and G. Lanfranchi, The Dark Photon, SpringerBriefs in Physics (Springer, Cham, 2020).
- J. Jaeckel and A. Ringwald, Annu. Rev. Nucl. Part. Sci. 60, 405 (2010).
- A. Accardi et al., Eur. Phys. J. A 57, 261 (2021).
- S. Schlimme et al., EPJ Web Conf. 303, 06002 (2024).
- D. Becker et al., Eur. Phys. J. A 54, 208 (2018).
- M. Christmann et al. (MAGIX Collaboration), Proc. Sci. EPS-HEP2021 (2022) 129.
- B. S. Schlimme et al. (A1 Collaboration and MAGIX Collaboration), Nucl. Instrum. Methods Phys. Res., Sect. A 1013, 165668 (2021).
- H. Merkel et al. (A1 Collaboration), Phys. Rev. Lett. 106, 251802 (2011).
- H. Merkel et al., Phys. Rev. Lett. 112, 221802 (2014).
- M. Heller, N. Keil, and M. Vanderhaeghen, Phys. Rev. D 104, 073007 (2021).
- W. A. McKinley and H. Feshbach, Phys. Rev. 74, 1759 (1948).
- X. Fan, T. G. Myers, B. A. D. Sukra, and G. Gabrielse, Phys. Rev. Lett. 130, 071801 (2023).
- A. Pustyntsev and M. Vanderhaeghen, Phys. Rev. D 112, 095001 (2025).
- J. P. Lees et al. (BABAR Collaboration), Phys. Rev. Lett. 113, 201801 (2014).
- J. R. Batley et al. (NA48/2 Collaboration), Phys. Lett. B 746, 178 (2015).
- D. Banerjee et al. (NA64 Collaboration), Phys. Rev. D 101, 071101 (2020).
- T. Ferber, Acta Phys. Pol. B 46, 2285 (2015).
- P. Ilten, J. Thaler, M. Williams, and W. Xue, Phys. Rev. D 92, 115017 (2015).
- A. Pustyntsev, M. S. Ramasamy, and M. Vanderhaeghen, Phys. Rev. D 113, 075032 (2026).
- S. Egli et al. (SINDRUM Collaboration), Phys. Lett. B 222, 533 (1989).
- L. Di Luzio, P. Paradisi, and N. Selimovic, Nucl. Phys. B1021, 117177 (2025).