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On formation of the 12C(0+2) and 12C(3-) states in relativistic dissociation of light nuclei

2024/11/27 by A. Zaitsev, Zaitsev, A. A., P. I. Zarubin +1
Physics and Astronomy · #Astro and Planetary Science #Atomic and Molecular Physics #FOS: Physical sciences #Nuclear Experiment (nucl-ex) #Nuclear Theory (nucl-th) #Nuclear physics research studies

paper · pdf · doi:10.48550/arxiv.2411.18394

openalex publication_date 2024/11/27 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

The formation of the excited states 12C(0+2) and 12C(3-) is investigated in the dissociation of 12C → 3α and 16O → 4α at the energy of 3.65 GeV per nucleon in the nuclear emulsion. The identification becomes possible by reconstructing the invariant mass from measurements of emission angles in the approximation of conservation of momentum per nucleon of the parent nucleus. The contribution of the decays 12C(0+2) and 12C(3-) to the dissociation 12C → 3α is 11 and 19%, and in 16O → 4α it is - 20 and 30%, correspondingly.

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