Fusion reactions with the one-neutron halo nucleus 15C
M. Alcorta, K. E. Rehm, B. B. Back, S. Bedoor, P. F. Bertone, C. M., Deibel, B. DiGiovine, H. Esbensen, J. P. Greene, C. R. Hoffmann, C. L. Jiang,, J. C. Lighthall, S. T. Marley, R. C. Pardo, M. Paul, A. M. Rogers, C. Ugalde,, A. H. Wuosmaa

TL;DR
This study investigates fusion reactions involving the one-neutron halo nucleus 15C, revealing significant sub-barrier fusion enhancement compared to non-halo isotopes, highlighting the influence of halo structure on nuclear fusion processes.
Contribution
First experimental measurement of fusion-fission cross sections for 15C + 232Th near the Coulomb barrier, demonstrating halo effects on fusion enhancement.
Findings
Fusion yield for 15C is 2-5 times higher at sub-barrier energies.
Cross sections for 14C align with trends for 12,13C.
Halo structure influences fusion probability at near-barrier energies.
Abstract
The structure of 15C, with an s1/2 neutron weakly bound to a closed-neutron shell nucleus 14C, makes it a prime candidate for a one-neutron halo nucleus. We have for the first time studied the cross section for the fusion-fission reaction 15C + 232Th at energies in the vicinity of the Coulomb barrier and compared it to the yield of the neighboring 14C + 232Th system measured in the same experiment. At sub-barrier energies, an enhancement of the fusion yield by factors of 2-5 was observed for 15C, while the cross sections for 14C match the trends measured for 12,13C.
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