DOI: 10.1140/epjc/s10052-026-15912-9 ISSN: 1434-6052

New limits on the Pauli forbidden transitions in $$^{12}\textrm{C}$$ nuclei obtained with the complete Borexino dataset

, D. Basilico, G. Bellini, J. Benziger, R. Biondi, B. Caccianiga, A. Caminata, A. Chepurnov, D. D’Angelo, A. Derbin, A. Di Giacinto, V. Di Marcello, X. F. Ding, A. Di Ludovico, L. Di Noto, I. Drachnev, D. Franco, C. Galbiati, C. Ghiano, M. Giammarchi, A. Goretti, M. Gromov, D. Guffanti, A. Ianni, A. Ianni, A. Jany, V. Kobychev, G. Korga, S. Kumaran, M. Laubenstein, E. Litvinovich, P. Lombardi, I. Lomskaya, L. Ludhova, I. Machulin, J. Martyn, E. Meroni, L. Miramonti, M. Misiaszek, V. Muratova, L. Oberauer, V. Orekhov, F. Ortica, M. Pallavicini, L. Pelicci, Ö. Penek, L. Pietrofaccia, N. Pilipenko, A. Pocar, G. Raikov, M. T. Ranalli, G. Ranucci, A. Razeto, A. Re, N. Rossi, S. Schönert, D. Semenov, G. Settanta, M. Skorokhvatov, A. Singhal, O. Smirnov, A. Sotnikov, R. Tartaglia, G. Testera, E. Unzhakov, A. Vishneva, R. B. Vogelaar, F. von Feilitzsch, M. Wojcik, M. Wurm, S. Zavatarelli, K. Zuber, G. Zuzel

Abstract

The Pauli exclusion principle (PEP) was tested for nucleons in

$$^{12}{C}$$ 12 C
nuclei using the Borexino dataset from 2007 to 2021. The approach consists of searching for
$$\gamma $$ γ
-quanta, neutrons, protons, as well as electrons and positrons emitted in non-Paulian transitions of nucleons from the
$$1P_{3/2}$$ 1 P 3 / 2
shell to the filled
$$1S_{1/2}$$ 1 S 1 / 2
shell. Due to the uniquely low background level, the large mass, and long measurement time of the Borexino detector, the most stringent experimental constraints to date on the lifetime of the
$$\mathrm {^{12}C}$$ 12 C
nucleus with respect to PEP-forbidden transitions were obtained:
$$\tau ({^{12}\textrm{C}}\rightarrow {^{12}\widetilde{\textrm{C}}}+\gamma ) \ge {1.1\times 10^{32}}$$ τ ( 12 C 12 C ~ + γ ) 1.1 × 10 32
y,
$$\tau ({^{12}\textrm{C}}\rightarrow {^{11}\widetilde{\textrm{B}}}+ p) \ge {1.0\times 10^{31}}$$ τ ( 12 C 11 B ~ + p ) 1.0 × 10 31
y,
$$\tau ({^{12}\textrm{C}}\rightarrow {^{11}\widetilde{\textrm{C}}}+ n) \ge 2.0 \times 10^{31}$$ τ ( 12 C 11 C ~ + n ) 2.0 × 10 31
y,
$$\tau ({^{12}\textrm{C}}\rightarrow {^{12}\widetilde{\textrm{N}}}+ e^- + \overline{\nu }_e) \ge 6.4 \times 10^{30}$$ τ ( 12 C 12 N ~ + e - + ν ¯ e ) 6.4 × 10 30
y and
$$\tau ({^{12}\textrm{C}}\rightarrow {^{12}\widetilde{\textrm{B}}}+ e^+ + \nu _e) \ge 6.6 \times 10^{30}$$ τ ( 12 C 12 B ~ + e + + ν e ) 6.6 × 10 30
y (90% C.L.). The upper limits on the relative strengths for the non-Paulian electromagnetic, strong, and weak transitions have been obtained:
$$\delta ^2_{\gamma }\le 1.0\times 10^{-57}$$ δ γ 2 1.0 × 10 - 57
,
$$\delta ^2_{N}\le 7.0\times 10^{-61}$$ δ N 2 7.0 × 10 - 61
and
$$\delta ^2_{\beta }\le 9.6\times 10^{-36}$$ δ β 2 9.6 × 10 - 36
, all at 90% C.L.

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