Three-body effects in the Hoyle-state decay
arXiv:1712.05251 · doi:10.1016/j.physletb.2018.02.031
Abstract
We use a sequential -matrix model to describe the breakup of the Hoyle state into three particles via the ground state of . It is shown that even in a sequential picture, features resembling a direct breakup branch appear in the phase-space distribution of the particles. We construct a toy model to describe the Coulomb interaction in the three-body final state and its effects on the decay spectrum are investigated. The framework is also used to predict the phase-space distribution of the particles emitted in a direct breakup of the Hoyle state and the possibility of interference between a direct and sequential branch is discussed. Our numerical results are compared to the current upper limit on the direct decay branch determined in recent experiments.
References in corpus (9)
- Evidence for -particle condensation in nuclei from the Hoyle state deexcitation
- High precision probe of the fully sequential decay width of the Hoyle state in C
- Quantum three-body calculation of the nonresonant triple-αreaction rate at low temperatures
- Decay and structure of the Hoyle state
- Three-body calculations of triple-alpha reaction
- Direct and sequential radiative three-body reaction rates at low temperatures
- Anatomy of three-body decay I. Schematic models
- R-Matrix description of particle energy spectra produced by low-energy T+T reactions
- Complete kinematical study of the 3 breakup of the 16.11 MeV state in C