2020
DOI: 10.1007/s00601-020-1545-5
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The Hoyle Family: The Search for Alpha-Condensate States in Light Nuclei

Abstract: Our present understanding of the structure of the Hoyle state in 12 C and other near-threshold states in α-conjugate nuclei is reviewed in the framework of the α-condensate model. The 12 C Hoyle state, in particular, is a candidate for α-condensation, due to its large radius and α-cluster structure. The predicted features of nuclear α-particle condensates are reviewed along with a discussion of their experimental indicators, with a focus on precision break-up measurements. Two experiments are discussed in deta… Show more

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Cited by 9 publications
(13 citation statements)
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References 65 publications
(135 reference statements)
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“…Breit-Wigner) of resonance line-shapes [17]. A non-zero branching ratio was also predicted in previous studies [3,4] although the ability to determine these as direct-looking rather than pileup on an event-by-event basis was not possible.…”
mentioning
confidence: 55%
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“…Breit-Wigner) of resonance line-shapes [17]. A non-zero branching ratio was also predicted in previous studies [3,4] although the ability to determine these as direct-looking rather than pileup on an event-by-event basis was not possible.…”
mentioning
confidence: 55%
“…This preferentially populates the center of the Dalitz plot where all the α-particles have similar energies. It is therefore practically identical to the DDE (Direct Decay Energy-sharing) model where the α-particles have identical energies, smeared only by the uncertainty principle [3,5]. The experimental data, shown in Fig.…”
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confidence: 59%
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“…The HS state is the second excitation of the 12 C nucleus (review [2]) at 378 keV above the 3α threshold. The isolation of HS at the beginning of the 12 C excitation spectrum and the width Γ(HS) = 9.3 ± 0.9 eV make it a 3α analogue of 8 Be.…”
Section: Introductionmentioning
confidence: 99%
“…The HS state is the second excitation of the 12 C nucleus (review [2]) at 378 keV above the 3α threshold. The isolation of HS at the beginning of the 12 C excitation spectrum and the width Γ(HS) = 9.3 ± 0.9 eV make it a 3α analogue of 8 Be. Synthesis of 12 C in the medium of red giants is possible through the merger 3α → α 8 Be → 12 C(0 + 2 ) → 12 C (+2γ or e + e − with a probability of about 10 −4 ).…”
Section: Introductionmentioning
confidence: 99%