6533b822fe1ef96bd127ccae
RESEARCH PRODUCT
Commissioning of the BRIKEN beta-delayed neutron detector for the study of exotic neutron-rich nuclei
Shigeru KubonoA. RiegoShunji NishimuraG. LorussoG. CortesK. P. RykaczewskiC. Domingo-pardoShintaro GoL. J. Harkness-brennanPhilip WoodsZsolt PodolyakN. FukudaJames SimpsonA. EstradeF. MontesS. BaeH. TakedaD. S. AhnRobert GrzywaczN. NepalA. Tolosa-delgadoJ. HaGabor KissJ. L. TainR. Caballero FolchB. RubioMaya TakechiV. H. PhongT. IsobeJ. AgramuntD. KahlB. MoonAriel Tarifeño-saldiviaM. LabicheP. J. Coleman-smithIris DillmannN. T. BrewerO. HallHiroyoshi SakuraiA.i. MoralesJj LiuJenny LeeV. F. E. PucknellH. SuzukiP. A. SöderströmI.h. LazarusS.l. ThomasRobert PageY. ShimizuToshiyuki SumikamaP. H. ReganP. H. ReganAlejandro AlgoraAlejandro AlgoraC. J. GriffinM. KogimtzisThomas DavinsonD. W. StracenerK. MatsuiK. MiernikK. MiernikB.c. RascoH. BabaF. CalviñoY. Saitosubject
AstrofísicaNeutron emissionQC1-999Astrophysics::High Energy Astrophysical PhenomenaNeutron detectorNuclear TheoryElectronNeutronAstrophysics01 natural sciencesNuclear physics0103 physical sciencesNeutron detectionNeutron010306 general physicsNuclear ExperimentDelayed neutronsPhysics:Energies::Energia nuclear [Àrees temàtiques de la UPC]Neutrons:Física [Àrees temàtiques de la UPC]010308 nuclear & particles physicsPhysicsNuclear structureDetectorNeutron captureDelayed neutronRadioactive decaydescription
Beta-delayed neutron emission (Beta-n) is a form of radioactive decay in which an electron, an anti-neutrino and one or more neutrons are emitted. This process arises if the energy window of the decay Q_Beta is greater than the neutron separation energy S n of the daughter. The probability in each decay of emitting neutrons is called the Pn value. This form of decay plays a key role in the synthesis of chemical elements in the Universe via the rapid neutron capture process, or r-process. The r-process proceeds far from the valley of nuclear stability, and leads to very neutron-rich nuclei that then decay to the line of stability. Most of these nuclei are ßn emitters. The initial abundance distribution is shaped by the decay half-life T1/2, but the neutron emission affects the final abundances in two ways: on the one hand it shifts the decay path to lower masses and on the other hand it provides a source of neutrons for late captures that will shift it in the opposite way. Thus, a good knowledge of Pn and T1/2 values of the nuclei between the line of stability and the r-process path is needed for a correct understanding of the observed abundances. Besides the astrophysical interest, the measurement of new Pn values and half-lives is also useful for refining nuclear structure models, constraining parameters of the models and testing ß-strength functions [3]. Our current understanding of the process of ß-delayed multiple neutron emission, as well as the competition between different open channels (gamma, one-neutron, two-neutron, etc), is incomplete because of the scarcity of experimental data. With these ideas in mind, the BRIKEN (Beta-delayed-neutron-measurements at RIKEN) collaboration was established, with the aim of greatly improving the quantity and quality of data the decays of very neutron-rich nuclei close to the r-process path.
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2017-01-01 |