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.