Ground State Decay of the Three-Proton Emitter $^{17}$Na Reveals Isospin Symmetry Breaking
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arXiv
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| Natura: | Preprint |
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2026
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| author | Xu, X. -D. Mukha, I. Xu, Z. C. Wang, S. M. Zhang, K. Y. Acosta, L. Casarejos, E. Cortina-Gil, D. Espino, J. M. Fomichev, A. Geissel, H. Gómez-Camacho, J. Grigorenko, L. V. Kiselev, O. Korsheninnikov, A. A. Kurz, N. Litvinov, Yu. A. Martel, I. Nociforo, C. Pfützner, M. Rodríguez-Tajes, C. Scheidenberger, C. Stanoiu, M. Sümmerer, K. Weick, H. Woods, P. J. Zhukov, M. V. |
| author_facet | Xu, X. -D. Mukha, I. Xu, Z. C. Wang, S. M. Zhang, K. Y. Acosta, L. Casarejos, E. Cortina-Gil, D. Espino, J. M. Fomichev, A. Geissel, H. Gómez-Camacho, J. Grigorenko, L. V. Kiselev, O. Korsheninnikov, A. A. Kurz, N. Litvinov, Yu. A. Martel, I. Nociforo, C. Pfützner, M. Rodríguez-Tajes, C. Scheidenberger, C. Stanoiu, M. Sümmerer, K. Weick, H. Woods, P. J. Zhukov, M. V. |
| contents | The spectrum of the exotic three-proton (3p) emitter $^{17}$Na has been studied by detecting all in-flight decay products. Derived from the measured angular correlations $^{14}$O+p+p+p, a resonant peak has been discovered at the 3p-decay energy of 2.24($^{+0.17}_{-0.25}$) MeV, which likely corresponds to the $^{17}$Na ground state. This decay energy value is significantly smaller than the previous experimental upper limit. Our measured $^{14}$O-p correlations stemming from the ground state decay have been quantitatively described by a sequential 1p-2p emission from a $^{17}$Na resonance via the intermediate $^{16}$Ne ground state, which allowed to derive the upper limit of $^{17}$Na ground-state width of 0.6 MeV. A dramatic systematic decrease in the mirror energy differences of mirror nuclei pairs has been observed at almost all 3p emitters with known proton separation energy (such as $^{31}$K, $^{20}$Al, and $^{17}$Na), in sharp contrast to the behavior in less exotic nuclei. Such a lowering effect indicates a general trend in evolution of nuclear structure for light to medium mass nuclei beyond the proton drip line, which is often associated with strong isospin symmetry breaking. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2604_08229 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | Ground State Decay of the Three-Proton Emitter $^{17}$Na Reveals Isospin Symmetry Breaking Xu, X. -D. Mukha, I. Xu, Z. C. Wang, S. M. Zhang, K. Y. Acosta, L. Casarejos, E. Cortina-Gil, D. Espino, J. M. Fomichev, A. Geissel, H. Gómez-Camacho, J. Grigorenko, L. V. Kiselev, O. Korsheninnikov, A. A. Kurz, N. Litvinov, Yu. A. Martel, I. Nociforo, C. Pfützner, M. Rodríguez-Tajes, C. Scheidenberger, C. Stanoiu, M. Sümmerer, K. Weick, H. Woods, P. J. Zhukov, M. V. Nuclear Experiment The spectrum of the exotic three-proton (3p) emitter $^{17}$Na has been studied by detecting all in-flight decay products. Derived from the measured angular correlations $^{14}$O+p+p+p, a resonant peak has been discovered at the 3p-decay energy of 2.24($^{+0.17}_{-0.25}$) MeV, which likely corresponds to the $^{17}$Na ground state. This decay energy value is significantly smaller than the previous experimental upper limit. Our measured $^{14}$O-p correlations stemming from the ground state decay have been quantitatively described by a sequential 1p-2p emission from a $^{17}$Na resonance via the intermediate $^{16}$Ne ground state, which allowed to derive the upper limit of $^{17}$Na ground-state width of 0.6 MeV. A dramatic systematic decrease in the mirror energy differences of mirror nuclei pairs has been observed at almost all 3p emitters with known proton separation energy (such as $^{31}$K, $^{20}$Al, and $^{17}$Na), in sharp contrast to the behavior in less exotic nuclei. Such a lowering effect indicates a general trend in evolution of nuclear structure for light to medium mass nuclei beyond the proton drip line, which is often associated with strong isospin symmetry breaking. |
| title | Ground State Decay of the Three-Proton Emitter $^{17}$Na Reveals Isospin Symmetry Breaking |
| topic | Nuclear Experiment |
| url | https://arxiv.org/abs/2604.08229 |