English

Probing Long-Range Forces in Neutrino Oscillations at the ESSnuSB Experiment

High Energy Physics - Phenomenology 2025-07-22 v3 High Energy Physics - Experiment

Abstract

Neutrino oscillations constitute an excellent tool to probe physics beyond the Standard Model. In this paper, we investigate the potential of the ESSnuSB experiment to constrain the effects of flavour-dependent long-range forces (LRFs) in neutrino oscillations, which may arise due to the extension of the Standard Model gauge group by introducing new U(1)U(1) symmetries. Focusing on three specific U(1)U(1) symmetries -- LeLμL_e - L_\mu, LeLτL_e - L_\tau, and LμLτL_\mu - L_\tau, we demonstrate that ESSnuSB offers a favourable environment to search for LRF effects. Our analyses reveal that ESSnuSB can set 90%90\% confidence level bounds of Veμ<2.99×1014eVV_{e\mu} < 2.99 \times 10^{-14} \, \text{eV}, Veτ<2.05×1014eVV_{e\tau} < 2.05 \times 10^{-14} \, \text{eV}, and Vμτ<1.81×1014eVV_{\mu\tau} < 1.81 \times 10^{-14} \, \text{eV}, which are competitive to the upcoming Deep Underground Neutrino Experiment (DUNE). It is also observed that reducing the systematic uncertainties from 5%5\% to 2%2\% improves the ESSnuSB limits on VαβV_{\alpha\beta}. Interestingly, we find limited correlations between LRF parameters and the less constrained lepton mixing parameters θ23\theta_{23} and δCP\delta_{\text{CP}}, preserving the robustness of ESSnuSB's sensitivity to CP violation. Even under extreme LRF potentials (Vαβ1013eVV_{\alpha\beta} \gg 10^{-13} \, \text{eV}), the CP-violation sensitivity and δCP\delta_{\text{CP}} precision remain largely unaffected. These results establish ESSnuSB as a competitive experimental setup for probing LRF effects, complementing constraints from other neutrino sources and offering critical insights into the physics of long-range forces.

Keywords

Cite

@article{arxiv.2504.10480,
  title  = {Probing Long-Range Forces in Neutrino Oscillations at the ESSnuSB Experiment},
  author = {ESSnuSB and : and J. Aguilar and M. Anastasopoulos and D. Barčot and E. Baussan and A. K. Bhattacharyya and A. Bignami and M. Blennow and M. Bogomilov and B. Bolling and E. Bouquerel and F. Bramati and A. Branca and G. Brunetti and I. Bustinduy and C. J. Carlile and J. Cederkall and T. W. Choi and S. Choubey and P. Christiansen and M. Collins and E. Cristaldo Morales and P. Cupiał and D. D'Ago and H. Danared and J. P. A. M. de André and M. Dracos and I. Efthymiopoulos and T. Ekelöf and M. Eshraqi and G. Fanourakis and A. Farricker and E. Fasoula and T. Fukuda and N. Gazis and Th. Geralis and M. Ghosh and A. Giarnetti and G. Gokbulut and A. Gupta and C. Hagner and L. Halić and M. Hooft and K. E. Iversen and N. Jachowicz and M. Jakkapu and M. Jenssen and R. Johansson and E. Kasimi and A. Kayis Topaksu and B. Kildetoft and B. Kliček and K. Kordas and B. Kovač and A. Leisos and M. Lindroos and A. Longhin and C. Maiano and D. Majumdar and S. Marangoni and S. Marciano and J. G. Marcos and C. Marrelli and D. Meloni and M. Mezzetto and N. Milas and J. L. Muñoz and K. Niewczas and M. Oglakci and T. Ohlsson and M. Olvegård and M. Pari and D. Patrzalek and G. Petkov and Ch. Petridou and P. Poussot and A. Psallidas and F. Pupilli and D. Saiang and D. Sampsonidis and A. Scanu and C. Schwab and F. Sordo and G. Stavropoulos and M. Stipčević and R. Tarkeshian and F. Terranova and T. Tolba and E. Trachanas and R. Tsenov and A. Tsirigotis and S. E. Tzamarias and M. Vanderpoorten and G. Vankova-Kirilova and N. Vassilopoulos and S. Vihonen and J. Wurtz and V. Zeter and O. Zormpa},
  journal= {arXiv preprint arXiv:2504.10480},
  year   = {2025}
}

Comments

31 pages, 13 figures, 3 tables, Version accepted for publication in JHEP