Search results for "Neutron-rich"

showing 8 items of 18 documents

The NEXT Project: Towards Production and Investigation of Neutron-Rich Heavy Nuclides

2022

The heaviest actinide elements are only accessible in accelerator-based experiments on a one-atom-at-a-time level. Usually, fusion–evaporation reactions are applied to reach these elements. However, access to the neutron-rich isotopes is limited. An alternative reaction mechanism to fusion–evaporation is multinucleon transfer, which features higher cross-sections. The main drawback of this technique is the wide angular distribution of the transfer products, which makes it challenging to catch and prepare them for precision measurements. To overcome this obstacle, we are building the NEXT experiment: a solenoid magnet is used to separate the different transfer products and to focus those of …

massaspektrometriaNuclear and High Energy Physicsneutron-rich nucleisolenoid separatorNEXT; neutron-rich nuclei; mutlinucleon transfer; solenoid separator; mass spectrometertutkimuslaitteetspektrometritmass spectrometermutlinucleon transferNEXTydinfysiikkaCondensed Matter PhysicsAtomic and Molecular Physics and OpticsAtoms; Volume 10; Issue 2; Pages: 59
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First decay study of the very neutron-rich isotope 93Br

2001

The decay of the mass-separated, very neutron-rich isotope 93 Br has been studied by γ spectroscopy. A level scheme of its daughter 93 Kr has been constructed. Level energies, γ-ray branching ratios, and multipolarities suggest spins and parities which are in accord with a smooth systematics of the N = 57 isotones for Z <~ 4 0 , suggesting the N = 56 subshell closure still to be effective in Kr isotopes. So far, there is no indication of a progressive onset of deformation in neutron-rich Kr isotopes. peerReviewed

neutron-rich isotopesNuclear Experiment
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First evidence of multiple β-delayed neutron emission for isotopes with a > 100

2017

The β-delayed neutron emission probability, Pn, of very neutron-rich nuclei allows us to achieve a better understanding of the nuclear structure above the neutron separation energy, Sn. The emission of neutrons can become the dominant decay process in neutron-rich astrophysical phenomena such as the rapid neutron capture process (r-process). There are around 600 accessible isotopes for which β-delayed one-neutron emission (β1n) is energetically allowed, but the branching ratio has only been determined for about one third of them. β1n decays have been experimentally measured up to the mass A ∼ 150, plus a single measurement of 210Tl. Concerning two-neutron emitters (β2n), ∼ 300 isotopes are …

neutron-rich nucleiAstrophysics::High Energy Astrophysical PhenomenaNuclear Theorynuclear structureNuclear Experimentbeta-delayed neutron emission
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High-sensitivity study of levels in 30Al following β decay of 30Mg

2016

γ -ray and fast-timing spectroscopy were used to study levels in 30Al populated following the β− decay of 30Mg. Five new transitions and three new levels were located in 30Al. A search was made to identify the third 1+ state expected at an excitation energy of ∼2.5 MeV. Two new levels were found, at 3163.9 and 3362.5 keV, that are firm candidates for this state. Using the advanced time-delayed (ATD) βγγ (t) method we have measured the lifetime of the 243.8-keV state to be T1/2 = 15(4) ps, which implies that the 243.8-keV transition is mainly of M1 character. Its fast B(M1; 2+ → 3+) value of 0.10(3) W.u. is in very good agreement with the USD shell-model prediction of 0.090 W.u. The 1801.5-k…

neutron-rich nucleibeta decayalumiinimagnesiumexcited statesPhysical Review C
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97/37 Rb 60 : The Cornerstone of the Region of Deformation around A∼100

2015

Excited states of the neutron-rich nuclei 97,99Rb were populated for the first time using the multistep Coulomb excitation of radioactive beams. Comparisons of the results with particle-rotor model calculations provide clear identification for the ground-state rotational band of 97Rb as being built on the πg9/2 [431] 3/2+ Nilsson-model configuration. The ground-state excitation spectra of the Rb isotopes show a marked distinction between single-particle-like structures below N=60 and rotational bands above. The present study defines the limits of the deformed region around A∼100 and indicates that the deformation of 97Rb is essentially the same as that observed well inside the deformed regi…

rubidiumneutron-rich nucleiCoulomb excitation
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97/37 Rb 60 : The Cornerstone of the Region of Deformation around A∼100

2015

rubidiumta114neutron-rich nucleiCoulomb excitationPhysical Review Letters
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High-sensitivity study of levels in 30Al following β decay of 30Mg

2016

ta114neutron-rich nucleiAluminiumMagnesiumbeta decayexcited statesPhysical Review C
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Production of a 15C radioactive ion beam based on 18O(n, α)

2019

In the context of the SPIRAL2 radioactive beam facility the production rate of the neutron-rich 15C nucleus by 18O(n,α) has been investigated. In a water target of 20 cm3, enriched in 18O and placed behind the neutron converter, a rate of a few 1010 nuclei per second can be reached with 1mA of 40MeV deuterons. A 18O(n,α) cross-section based on the activation method is proposed. It is intermediate between the highest and lowest evaluations available to date. peerReviewed

tutkimuslaitteetydinfysiikkaion beam productionneutron-rich carbon isotopes
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