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Precision Mass Measurements Reveal Low Neutron Pairing in Tin beyond N=82 and Its Impact on Stellar Nucleosynthesis

A. Mollaebrahimi1,2,3,*, C. Walls4,2, T. Dickel3,1, T. Miyagi5,6,7,8, A. Sieverding9,10, C. Andreoiu11, J. Ash2, B. Ashrafkhani12,2, I. Belosevic2 et al.

J. Bergman1, C. Brown13, T. Brunner14, J. Cardona4,2, L. Egoriti2, G. Gelinas12,2, G. Gwinner4, Z. Hockenbery14,2, J. D. Holt2,14, A. Jacobs15,2, S. Kakkar4,2, B. Kootte4,2, J. Lassen2, E. M. Lykiardopoulou15,2, S. Malbrunot-Ettenauer2,16, G. Martínez-Pinedo3,5,17, S. F. Paul2, W. R. Plaß3,1, M. P. Reiter13, A. Ridley2, C. Scheidenberger3,1,18, R. I. Thompson12, Y. Wang15,2, M. E. Wieser12, and A. A. Kwiatkowski19,2

  • *Contact author: A.mollaebrahimi@GSI.de

Chong Qi

Eur. Phys. J. A 62 15 (2026)

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Universe 11 323 (2025)

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