2019
DOI: 10.1103/physrevc.99.054610
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Full disassembly of excited Mg24 into six α particles

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Cited by 11 publications
(23 citation statements)
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“…In summary, the reaction mechanism of the 12 C( 16 O, 28 Si ) channel was studied at three beam energies of 160, 280, and 400 MeV. This experiment was performed to search for α-gas states in 12 C, 16 O, 20 Ne, 24 Mg and 28 Si. No such states were found for systems heavier than 12 C. In the case of heavier isotopes, there were various reasons discussed in this work in detail which could have obscured the observation of those states.…”
Section: Discussionmentioning
confidence: 99%
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“…In summary, the reaction mechanism of the 12 C( 16 O, 28 Si ) channel was studied at three beam energies of 160, 280, and 400 MeV. This experiment was performed to search for α-gas states in 12 C, 16 O, 20 Ne, 24 Mg and 28 Si. No such states were found for systems heavier than 12 C. In the case of heavier isotopes, there were various reasons discussed in this work in detail which could have obscured the observation of those states.…”
Section: Discussionmentioning
confidence: 99%
“…This system is analogous to a Bose-Einstein Condensate which has been well studied in atomic systems [17,18]. This work has been furthered in the nuclear realm by several experiments involving high-multiplicity particle decays [19][20][21] and experiments to observe an α-gas via "Coulomb explosion" of 40 Ca appear possible from a theoretical perspective [22]. Such an exotic state of matter is therefore postulated to describe the well-studied light N-α clustered states ( 8 Be(g.s) and 12 C(0 + 2 )) and is known as an α-condensate.…”
Section: Introductionmentioning
confidence: 98%
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“…In this paper one demonstrates, by means of the AMD simulation coupled with statistical models, that the charge equilibration process measured via isospin transport ratio is indeed affected by perturbations introduced by the dynamical and sta- tistical emissions from the fragments after their separation. In particular, the statistical emission (described by Gemini++ code) tends to introduce non-linear spurious distortions at low excitation energies (where structure effects are well known to affect the particle emission [67][68][69]), i.e. for large impact parameters, while the distortion becomes smoother and linear with increasing excitation.…”
Section: Neutron-proton Equilibrationmentioning
confidence: 99%
“…The investigation of the causes behind the nonlinearity at low E * /A is out of the goal of this paper. A possible contribution could be due to structure effects, since is well known that they affect the particle emission at low excitation energy [42][43][44]. In this sense, the isoscaling analysis [4,5] could be more suited as it divides out many structure effects to the first order.…”
Section: Statistical De-excitation Effectsmentioning
confidence: 99%