Investigating the predicted breathing-mode excitation of the Hoyle state
arXiv:2201.10396 · doi:10.1016/j.physletb.2022.136928
Abstract
Knowledge of the low-lying monopole strength in the Hoyle state in particular is crucial for our understanding of both the astrophysically important reaction and of -particle clustering. Multiple theoretical models have predicted a breathing mode of the Hoyle State at MeV, corresponding to a radial in-phase oscillation of the underlying clusters. The and reactions were employed to populate states in C in order to search for this predicted breathing mode. A self-consistent, simultaneous analysis of the inclusive spectra with R-matrix lineshapes, together with angular distributions of charged-particle decay, yielded clear evidence for excess monopole strength at MeV which is highly collective. Reproduction of the experimentally observed inclusive yields using a fit, with consistent population ratios for the various broad states, required an additional source of monopole strength. The interpretation of this additional monopole resonance as the breathing-mode excitation of the Hoyle state would provide evidence supporting a symmetry for the Hoyle state itself. The excess monopole strength may complicate analysis of the properties of the Hoyle state, modifying the temperature dependence of the rate at and ultimately, the predicted nucleosynthesis in explosive stars.
8 pages, 5 figures
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Cited by in corpus (5)
- Emergent geometry and duality in the carbon nucleus
- Cluster structures of the states of with the 3 four-body orthogonality condition model
- Understanding the total width of the state in
- Low-energy C continuum states in three- model
- Examination of the -cluster breaking in the four bands of C with the variation of multiple bases of the antisymmetrized molecular dynamics