2020
DOI: 10.1140/epja/s10050-020-00252-3
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Unstable states in dissociation of relativistic nuclei

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Cited by 17 publications
(51 citation statements)
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“…[26], such α-clustered nuclei can be created in heavy-ion reactions at intermediate energies. They can also be formed in the spectator regions of nuclei in relativistic heavy-ion collisions [27]. The separation of α-clustered and nucleonic states of nuclear matter can be explained [9] by the existence of the potential barrier between these two phases.…”
Section: Introductionmentioning
confidence: 99%
See 1 more Smart Citation
“…[26], such α-clustered nuclei can be created in heavy-ion reactions at intermediate energies. They can also be formed in the spectator regions of nuclei in relativistic heavy-ion collisions [27]. The separation of α-clustered and nucleonic states of nuclear matter can be explained [9] by the existence of the potential barrier between these two phases.…”
Section: Introductionmentioning
confidence: 99%
“…Note that the parameters b = 30.73 MeV −2 and a = 3 • 10 4 used in Ref [15]. violate the constraint(27), which results in an unrealistically large binding energy of α matter W B 214 MeV.…”
mentioning
confidence: 99%
“…Decays of unstable nuclei 8 Be → 2α and 9 B → 2αp, as well as the Hoyle state HS → 3α [1][2][3], can be reconstructed in the events of relativistic nuclei fragmentation in the nuclear track emulsion (NTE). Having extremely low decay energy, the above fragments appear as pairs and triplets with the smallest opening angles.…”
Section: Introductionmentioning
confidence: 99%
“…The analysis of fragmentation of relativistic nuclei in a nuclear track emulsion (NTE) makes it possible to study internally non-relativistic ensembles of H and He nuclei starting with produced in decays of the unstable 8 Be and 9 B nuclei and up to the most complex ones [1][2][3]. NTE layers with a thickness of 200 to 500 µm, longitudinally exposed to the nuclei under study, make it possible to determine with full completeness and resolution of 0.5 µm the angles between the directions of emission of relativistic fragments in the cone sinθ f r = P f r /P 0 , where P f r = 0.2 GeV/c is the characteristic Fermi momentum of nucleons in a projectile nucleus with a momentum per nucleon.…”
Section: Introductionmentioning
confidence: 99%
“…To calculate the invariant masses of 2α-pairs Q 2α and 3α-triplets Q 3α in the approximation of conservation of momentum per nucleon by α-particles of the primary nucleus, only measurements of their emission angles are used. The correspondence between He - 4 He and H -1 H is assumed, since in the case of extremely narrow decays of 8 Be and 9 B, the measured contributions of 3 He and 2 H are small. The initial portions of the event distributions over the variables Q 2α and Q 3α contain peaks corresponding to 8 Be and HS for both 12 C and 16 O.…”
Section: Introductionmentioning
confidence: 99%