Multinucleon Transfer in Peripheral Collisions of 64Ni on 64Ni at 25 MeV/nucleon

Многосторонний перенос нуклонов в периферических столкновениях 64Ni с 64Ni при энергии 25 МэВ/нуклон
Eirini Kontogianni, G. Souliotis, Chrysi Giannitsa, Konstantinos Gkatzogias, Stergios Koulouris, Eleftheria Travlou, M. Veselský, Sherry J. Yennelo, A. Bonasera
2026-02-24

64NiConstrained Molecular DynamicsDeep-Inelastic Transfer modelmultinucleon transferperipheral collisions
We study the yields, the momentum distributions and the angular distributions of projectile-like fragments from peripheral collisions of 64Ni (25 MeV/nucleon) on 64Ni. The experimental data were obtained in previous works with the BigSol separator system at the Cyclotron Institute of Texas A&M University. Projectile fragments were collected and analyzed at forward angles (1.5-3.0 degrees). The production cross sections, the momentum distributions and the angular distributions of the fragments were systematically studied and compared with the Deep-Inelastic Transfer (DIT) model and the Constrained Molecular Dynamics (CoMD) model followed by the deexcitation model GEMINI. Both models appear to describe the data rather adequately, but possible improvements are necessary. Special attention is given in the possibility to produce neutron-rich rare isotopes of elements at the beginning of the astrophysical r-process. Efforts similar to this work are ongoing to shed light to the reaction mechanisms of peripheral collisions at this energy (25 MeV/nucleon).
1
Both reaction-model approaches describe the measured data reasonably well, although further improvements are needed.
2
Fragments were collected at forward angles of 1.5–3.0 degrees using the BigSol separator at Texas A&M University’s Cyclotron Institute.
3
Production cross sections and kinematic distributions were systematically compared with DIT and CoMD followed by GEMINI deexcitation.
4
Projectile-like fragment yields, momentum distributions, and angular distributions were measured for peripheral 64Ni+64Ni collisions at 25 MeV/nucleon.
5
The study assesses peripheral multinucleon transfer as a possible source of neutron-rich isotopes relevant to the beginning of the astrophysical r-process.

Projectile-like fragments produced in peripheral 64Ni + 64Ni collisions at 25 MeV/nucleon

Production cross sections, momentum distributions, angular distributions, and reaction mechanisms of multinucleon transfer, including the production of neutron-rich isotopes

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2026-02-24
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Eirini Kontogianni
G. Souliotis
Chrysi Giannitsa
Konstantinos Gkatzogias
Stergios Koulouris
Eleftheria Travlou
M. Veselský
Sherry J. Yennelo
A. Bonasera
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