Sub-barrier fusion of neutron-rich nuclei and its astrophysical consequences

V. I. Zagrebaev, V. V. Samarin, and Walter Greiner
Phys. Rev. C 75, 035809 – Published 27 March 2007

Abstract

Near-barrier fusion of neutron-rich nuclei was studied within the semiempirical channel coupling model for intermediate neutron rearrangement and within the time-dependent three-body Schrödinger equation. The possibility of neutron transfer with positive Q values considerably increases the barrier penetrability. A huge enhancement of deep sub-barrier fusion probability was found for light neutron-rich weakly bound nuclei (such as He6). This may be quite important for astrophysical primordial and supernova nucleosynthesis.

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  • Received 15 December 2006

DOI:https://doi.org/10.1103/PhysRevC.75.035809

©2007 American Physical Society

Authors & Affiliations

V. I. Zagrebaev and V. V. Samarin

  • Flerov Laboratory of Nuclear Reactions, JINR, Dubna, Moscow Region, Russia

Walter Greiner

  • Frankfurt Institute for Advanced Studies, J. W. Goethe-Universität, Frankfurt, Germany

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Issue

Vol. 75, Iss. 3 — March 2007

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