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Characterization of a plutonium-beryllium neutron source. Appl Radiat Isot 2020; 167:109441. [PMID: 33002762 DOI: 10.1016/j.apradiso.2020.109441] [Citation(s) in RCA: 5] [Impact Index Per Article: 1.3] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 02/18/2020] [Revised: 04/22/2020] [Accepted: 09/21/2020] [Indexed: 11/23/2022]
Abstract
Here we present an investigation of a plutonium-beryllium neutron source available at the Horia Hulubei National Institute of Physics and Nuclear Engineering, Romania, to be used for detector characterization during the implementation of the Extreme Light Infrastructure - Nuclear Physics project. Using several different techniques and instruments, we have measured the isotopic composition for plutonium to be 75% 239Pu and 24% 240Pu, with a minor contribution from other isotopes. Furthermore, we have measured the source activity as of November 20th 2019 to be 2.220(5)×105 neutrons per second with a mean energy of 3.25(17) MeV. We have also measured both the γ-tagged and full neutron energy spectra, and discuss the origin of the observed structure in the neutron energies based on these. All these parameters are of importance both for traceability of nuclear material, radioprotection, and accurate detector characterization.
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Söderström PA, Capponi L, Açıksöz E, Otsuka T, Tsoneva N, Tsunoda Y, Balabanski DL, Pietralla N, Guardo GL, Lattuada D, Lenske H, Matei C, Nichita D, Pappalardo A, Petruse T. Electromagnetic character of the competitive γγ/γ-decay from 137mBa. Nat Commun 2020; 11:3242. [PMID: 32591502 PMCID: PMC7320027 DOI: 10.1038/s41467-020-16787-4] [Citation(s) in RCA: 4] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 12/08/2019] [Accepted: 05/20/2020] [Indexed: 11/09/2022] Open
Abstract
Second-order processes in physics is a research topic focusing attention from several fields worldwide including, for example, non-linear quantum electrodynamics with high-power lasers, neutrinoless double-β decay, and stimulated atomic two-photon transitions. For the electromagnetic nuclear interaction, the observation of the competitive double-γ decay from 137mBa has opened up the nuclear structure field for detailed investigation of second-order processes through the manifestation of off-diagonal nuclear polarisability. Here, we confirm this observation with an 8.7σ significance, and an improved value on the double-photon versus single-photon branching ratio as 2.62 × 10-6(30). Our results, however, contradict the conclusions from the original experiment, where the decay was interpreted to be dominated by a quadrupole-quadrupole component. Here, we find a substantial enhancement in the energy distribution consistent with a dominating octupole-dipole character and a rather small quadrupole-quadrupole component in the decay, hindered due to an evolution of the internal nuclear structure. The implied strongly hindered double-photon branching in 137mBa opens up the possibility of the double-photon branching as a feasible tool for nuclear-structure studies on off-diagonal polarisability in nuclei where this hindrance is not present.
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Affiliation(s)
- P-A Söderström
- Extreme Light Infrastructure-Nuclear Physics (ELI-NP)/Horia Hulubei National Institute for R&D in Physics and Nuclear Engineering, Str. Reactorului 30, 077125, Bucharest-Măgurele, Romania.
| | - L Capponi
- Extreme Light Infrastructure-Nuclear Physics (ELI-NP)/Horia Hulubei National Institute for R&D in Physics and Nuclear Engineering, Str. Reactorului 30, 077125, Bucharest-Măgurele, Romania
| | - E Açıksöz
- Extreme Light Infrastructure-Nuclear Physics (ELI-NP)/Horia Hulubei National Institute for R&D in Physics and Nuclear Engineering, Str. Reactorului 30, 077125, Bucharest-Măgurele, Romania
| | - T Otsuka
- Center for Nuclear Study, University of Tokyo, Hongo, Bunkyo-ku, Tokyo, 113-0033, Japan.,Department of Physics, University of Tokyo, Hongo, Bunkyo-ku, Tokyo, 113-0033, Japan.,RIKEN Nishina Center, 2-1 Hirosawa, Wako, Saitama, 351-0198, Japan
| | - N Tsoneva
- Extreme Light Infrastructure-Nuclear Physics (ELI-NP)/Horia Hulubei National Institute for R&D in Physics and Nuclear Engineering, Str. Reactorului 30, 077125, Bucharest-Măgurele, Romania
| | - Y Tsunoda
- Center for Nuclear Study, University of Tokyo, Hongo, Bunkyo-ku, Tokyo, 113-0033, Japan
| | - D L Balabanski
- Extreme Light Infrastructure-Nuclear Physics (ELI-NP)/Horia Hulubei National Institute for R&D in Physics and Nuclear Engineering, Str. Reactorului 30, 077125, Bucharest-Măgurele, Romania
| | - N Pietralla
- Institut für Kernphysik, Technische Universität Darmstadt, 64289, Darmstadt, Germany
| | - G L Guardo
- Extreme Light Infrastructure-Nuclear Physics (ELI-NP)/Horia Hulubei National Institute for R&D in Physics and Nuclear Engineering, Str. Reactorului 30, 077125, Bucharest-Măgurele, Romania.,Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Sud, 95125, Catania, Italy
| | - D Lattuada
- Extreme Light Infrastructure-Nuclear Physics (ELI-NP)/Horia Hulubei National Institute for R&D in Physics and Nuclear Engineering, Str. Reactorului 30, 077125, Bucharest-Măgurele, Romania.,Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Sud, 95125, Catania, Italy.,Universitá degli Studi di Enna KORE, Viale delle Olimpiadi, 94100, Enna, Italy
| | - H Lenske
- Institut für Theoretische Physik, Universität Gießen, 35392, Gießen, Germany
| | - C Matei
- Extreme Light Infrastructure-Nuclear Physics (ELI-NP)/Horia Hulubei National Institute for R&D in Physics and Nuclear Engineering, Str. Reactorului 30, 077125, Bucharest-Măgurele, Romania
| | - D Nichita
- Extreme Light Infrastructure-Nuclear Physics (ELI-NP)/Horia Hulubei National Institute for R&D in Physics and Nuclear Engineering, Str. Reactorului 30, 077125, Bucharest-Măgurele, Romania.,Politehnica University of Bucharest, Splaiul Independentei 313, 060042, Bucharest, Romania
| | - A Pappalardo
- Extreme Light Infrastructure-Nuclear Physics (ELI-NP)/Horia Hulubei National Institute for R&D in Physics and Nuclear Engineering, Str. Reactorului 30, 077125, Bucharest-Măgurele, Romania
| | - T Petruse
- Extreme Light Infrastructure-Nuclear Physics (ELI-NP)/Horia Hulubei National Institute for R&D in Physics and Nuclear Engineering, Str. Reactorului 30, 077125, Bucharest-Măgurele, Romania.,Politehnica University of Bucharest, Splaiul Independentei 313, 060042, Bucharest, Romania
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Petruse T, Guardo GL, Cognata ML, Lattuada D, Spitalieri C, Balabanski DL, Agiksoz E, Acosta L, Capponi L, Carbone D, Cherubini S, Choudhury D, D’Agata G, Pietro AD, Figuera P, Gulino M, Kilik AI, Commara ML, Lamia L, Matei C, Palmerini S, Pizzone RG, Romano S, Soderstrom PA, Sparta R, Tumino A, Onses SV. Preliminary results for the 19F(ρ,α) 16O reaction cross section measured at INFN-LNS. EPJ WEB OF CONFERENCES 2020. [DOI: 10.1051/epjconf/202022702009] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/14/2022] Open
Abstract
The 19F(ρ,α)16O reaction is an important fluorine destruction chan- nel in the proton-rich outer layers of asymptotic giant branch (AGB) stars and it might also play a role in hydrogen-deficient post-AGB star nucleosynthesis. At present, theoretical models overproduce F abundances in AGB stars with re-spect to the observed values, thus calling for further investigation of the nuclear reaction rates involved in the production and destruction of fluorine. In the last years, new direct and indirect measurements improved significantly the knowl- edge of 19F(ρ,α)16O cross section at deeply sub-Coulomb energies (below 0.8 MeV). However, those data are larger by a factor of 1.4 with respect the previ- ous data reported in the NACRE compilation in the energy region 0.6-0.8 MeV. Using the Large High resolution Array of Silicons for Astrophysics (LHASA), we performed a new direct measurement of the 19F(ρ,α)16O. The goal of this experiment is to reduce the uncertainties in the nuclear reaction rate of the 19F(ρ,α)16O reaction. Here, experimental details, the calibration procedure and angular distributions are presented.
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Guardo GL, Anzalone A, Balabanski D, Chesnevskaya S, Crucillá W, Filipescu D, Gulino M, La Cognata M, Lattuada D, Matei C, Pizzone RG, Rapisarda GG, Romano S, Spitaleri C, Taffara A, Tumino A, Xu Y. Development of the ELISSA array: prototype testing at Laboratori Nazionali del Sud. EPJ WEB OF CONFERENCES 2018. [DOI: 10.1051/epjconf/201818402006] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/15/2022] Open
Abstract
The Extreme Light Infrastructure-Nuclear Physics (ELI-NP) facility, underconstruction in Magurele near Bucharest in Romania, will provide high-intensity andhigh-resolution gamma ray beams that can be used to address hotly debated problems in nuclear astrophysics, such as the accurate measurements of the cross sections of the24Mg(γ,α)20Ne reaction
For this purpose, a silicon strip detector array (named ELISSA) will be realized in acommon effort by ELI-NP and Laboratori Nazionali del Sud (INFN-LNS), in order to measure excitation functions and angular distributions over a wide energy and angular range. A prototype of ELISSA was built and tested at INFN-LNS in Catania (Italy) with the support of ELI-NP. In this occasion, we have carried out experiments with alpha sources and with a 11 MeV 7Li beam that show up a very good energy resolution (better than 1%) and very good position resolution, of the order of 1 mm. Moreover, a threshold of 150 keV can be easily achieved with no cooling.
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Lattuada D, La Cognata M, Anzalone A, Balabanski D, Chesnevskaya S, Costa M, Crucillà V, Guardo G, Gulino M, Matei C, Pizzone R, Romano S, Spitaleri C, Tumino A, Xu Y. A Geant4-based Monte Carlo Tool for Nuclear Astrophysics. EPJ WEB OF CONFERENCES 2018. [DOI: 10.1051/epjconf/2018184020008] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/14/2022] Open
Abstract
Present and future gamma-beam facilities represent a great opportunity to validate and evaluate the cross-sections of many photonuclear reactions at near-threshold energies, whose data mostly come from theoretical calculations. We developed a Monte Carlo (MC) software that makes use of the validatedtracking Geant4 libraries and the n-body event generator of ROOT libraries in order to provide a fast, realiable and complete MC tool to be used for nuclear physics experiments, with a particular focus on photo-nuclear processes. We discuss the results of the MC simulations performed in order to evaluate the effects of the electromagnetic background, the straggling of the emitted particles due to the target thickness and the resolution of the silicon detectors. Finally we present the preliminary results on some nuclear reactions involved in the p-process, which will be studied with ELISSA and the GBS at ELI-NP.
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