Articles Citing

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

A. Mollaebrahimi ^1,2,3,*, C. Walls^4,2, T. Dickel^3,1, T. Miyagi^5,6,7,8, A. Sieverding^9,10, C. Andreoiu¹¹, J. Ash², B. Ashrafkhani^12,2, I. Belosevic² et al.

J. Bergman¹, C. Brown¹³, T. Brunner¹⁴, J. Cardona^4,2, L. Egoriti², G. Gelinas^12,2, G. Gwinner⁴, Z. Hockenbery^14,2, J. D. Holt^2,14, A. Jacobs^15,2, S. Kakkar^4,2, B. Kootte^4,2, J. Lassen², E. M. Lykiardopoulou^15,2, S. Malbrunot-Ettenauer^2,16, G. Martínez-Pinedo^3,5,17, S. F. Paul², W. R. Plaß^3,1, M. P. Reiter¹³, A. Ridley², C. Scheidenberger^3,1,18, R. I. Thompson¹², Y. Wang^15,2, M. E. Wieser¹², and A. A. Kwiatkowski^19,2

¹II. Physikalisches Institut, Justus-Liebig-Universität Gießen, 35392 Gießen, Germany
²TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
³GSI Helmholtzzentrum für Schwerionenforschung GmbH, 64291 Darmstadt, Germany
⁴Department of Physics and Astronomy, University of Manitoba, Winnipeg, Manitoba R3T 2N2, Canada
⁵Institut für Kernphysik (Theoriezentrum), Fachbereich Physik, Technische Universität Darmstadt, Schlossgartenstraße 2, 64289 Darmstadt, Germany
⁶ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung GmbH, 64291 Darmstadt, Germany
⁷Max-Planck-Institut für Kernphysik, Saupfercheckweg 1, 69117 Heidelberg, Germany
⁸Center for Computational Sciences, University of Tsukuba, 1-1-1 Tennodai, Tsukuba 305-8577, Japan
⁹Lawrence Livermore National Laboratory, P.O. Box 808, L-414, Livermore, California 94551, USA
¹⁰Max Planck Institute for Astrophysics, Karl-Schwarzschild-Straße 1, D-85748 Garching, Germany
¹¹Department of Chemistry, Simon Fraser University, Burnaby, British Columbia V5A 1S6, Canada
¹²Department of Physics and Astronomy, University of Calgary, Calgary, Alberta T2G 0J1, Canada
¹³Institute for Particle and Nuclear Physics, University of Edinburgh, Edinburgh EH9 3FD, United Kingdom
¹⁴Department of Physics, McGill University, Montréal, Quebec H3A 2T8, Canada
¹⁵Department of Physics and Astronomy, University of British Columbia, Vancouver, British Columbia V6T 1Z1, Canada
¹⁶Department of Physics, University of Toronto, Toronto, Ontario M5S 1A1, Canada
¹⁷Helmholtz Forschungsakademie Hessen für FAIR (HFHF), GSI Helmholtzzentrum für Schwerionenforschung, Planckstraße 1, 64291 Darmstadt, Germany
¹⁸Helmholtz Forschungsakademie Hessen für FAIR (HFHF), GSI Helmholtzzentrum für Schwerionenforschung, Campus Gießen, 35392 Gießen, Germany
¹⁹Department of Physics and Astronomy, University of Victoria, Victoria, British Columbia V8P 5C2, Canada

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

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Articles Citing

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

r -Process Nucleosynthesis with Ab Initio Nuclear Masses around the N=82 Shell Closure

Partial conservation of seniority in semi-magic nuclei

Integrating ensemble model and interpretable framework to unveil nuclear binding energy

SPIRIT Solver: Accelerating r-process Nucleosynthesis with Sparse Preconditioning

Distribution of Heavy-Element Abundances Generated by Decay from a Quasi-Equilibrium State

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Articles Citing

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

r -Process Nucleosynthesis with Ab Initio Nuclear Masses around the N=82 Shell Closure

Partial conservation of seniority in semi-magic nuclei

Integrating ensemble model and interpretable framework to unveil nuclear binding energy

SPIRIT Solver: Accelerating r-process Nucleosynthesis with Sparse Preconditioning

Distribution of Heavy-Element Abundances Generated by Decay from a Quasi-Equilibrium State

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