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Featured researches published by F. Browne.


Physical Review Letters | 2015

Extension of the N = 40 Island of Inversion towards N =50: Spectroscopy of 66Cr,70,72Fe

C. Santamaria; C. Louchart; A. Obertelli; V. Werner; P. Doornenbal; F. Nowacki; G. Authelet; H. Baba; D. Calvet; F. Château; A. Corsi; A. Delbart; J.-M. Gheller; A. Gillibert; T. Isobe; V. Lapoux; Michio M. Matsushita; S. Momiyama; Tohru Motobayashi; M. Niikura; H. Otsu; C. Péron; Alan Peyaud; E. C. Pollacco; J.-Y. Roussé; H. Sakurai; M. Sasano; Y. Shiga; Satoshi Takeuchi; R. Taniuchi

We report on the measurement of the first 2(+) and 4(+) states of (66)Cr and (70,72)Fe via in-beam γ-ray spectroscopy. The nuclei of interest were produced by (p,2p) reactions at incident energies of 260  MeV/nucleon. The experiment was performed at the Radioactive Isotope Beam Factory, RIKEN, using the DALI 2γ-ray detector array and the novel MINOS device, a thick liquid hydrogen target combined with a vertex tracker. A low-energy plateau of 2(1)(+) and 4(1)(+) energies as a function of the neutron number was observed for N≥38 and N≥40 for even-even Cr and Fe isotopes, respectively. State-of-the-art shell model calculations with a modified Lenzi-Nowacki-Poves-Sieja (LNPS) interaction in the pfg(9/2)d(5/2) valence space reproduce the observations. Interpretation within the shell model shows an extension of the island of inversion at N=40 for more neutron-rich isotopes towards N=50.


Physical Review Letters | 2017

94β -Decay Half-Lives of Neutron-Rich Cs55 to Ho67 : Experimental Feedback and Evaluation of the r -Process Rare-Earth Peak Formation

J. Wu; S. Nishimura; G. Lorusso; Peter Möller; E. Ideguchi; P. H. Regan; G. S. Simpson; P.-A. Söderström; P. M. Walker; Hiroshi Watanabe; Z. Y. Xu; H. Baba; F. Browne; R. Daido; P. Doornenbal; Y. F. Fang; G. Gey; T. Isobe; P. Lee; J. J. Liu; Z. Li; Z. Korkulu; Z. Patel; V. H. Phong; S. Rice; H. Sakurai; Laura C. Sinclair; T. Sumikama; M. Tanaka; A. Yagi

The β-decay half-lives of 94 neutron-rich nuclei ^{144-151}Cs, ^{146-154}Ba, ^{148-156}La, ^{150-158}Ce, ^{153-160}Pr, ^{156-162}Nd, ^{159-163}Pm, ^{160-166}Sm, ^{161-168}Eu, ^{165-170}Gd, ^{166-172}Tb, ^{169-173}Dy, ^{172-175}Ho, and two isomeric states ^{174m}Er, ^{172m}Dy were measured at the Radioactive Isotope Beam Factory, providing a new experimental basis to test theoretical models. Strikingly large drops of β-decay half-lives are observed at neutron-number N=97 for _{58}Ce, _{59}Pr, _{60}Nd, and _{62}Sm, and N=105 for _{63}Eu, _{64}Gd, _{65}Tb, and _{66}Dy. Features in the data mirror the interplay between pairing effects and microscopic structure. r-process network calculations performed for a range of mass models and astrophysical conditions show that the 57 half-lives measured for the first time play an important role in shaping the abundance pattern of rare-earth elements in the solar system.


Physical Review Letters | 2017

Shape Evolution in Neutron-rich Krypton Isotopes beyond N = 60 : First spectroscopy of 98;100Kr

F Flavigny; P. Doornenbal; A. Obertelli; J-P Delaroche; M Girod; J Libert; Tomás R. Rodríguez; G. Authelet; H. Baba; D. Calvet; F Chateau; S. Chen; A. Corsi; A. Delbart; J.-M. Gheller; A. Giganon; A. Gillibert; Lapoux; T Motobayashi; M. Niikura; N. Paul; J.-Y. Roussé; H Sakura; C. Santamaria; D Steppenbeck; R. Taniuchi; T Uesaka; T. Ando; T. Arici; A. Blazhev

We report on the first γ-ray spectroscopy of low-lying states in neutron-rich ^{98,100}Kr isotopes obtained from ^{99,101}Rb(p,2p) reactions at ∼220  MeV/nucleon. A reduction of the 2_{1}^{+} state energies beyond N=60 demonstrates a significant increase of deformation, shifted in neutron number compared to the sharper transition observed in strontium and zirconium isotopes. State-of-the-art beyond-mean-field calculations using the Gogny D1S interaction predict level energies in good agreement with experimental results. The identification of a low-lying (0_{2}^{+}, 2_{2}^{+}) state in ^{98}Kr provides the first experimental evidence of a competing configuration at low energy in neutron-rich krypton isotopes consistent with the oblate-prolate shape coexistence picture suggested by theory.


ORIGIN OF MATTER AND EVOLUTION OF GALAXIES 2013: Proceedings of the 12th International Symposium on Origin of Matter and Evolution of Galaxies (OMEG12) | 2014

β-decay of neutron-rich Z∼60 nuclei and the origin of rare earth elements

Jinguang Wu; S. Nishimura; G. Lorusso; Z.Y. Xu; H. Baba; F. Browne; R. Daido; P. Doornenbal; Y.F. Fang; E. Ideguchi; T. Isobe; Z. Li; Z. Patel; S. Rice; G. S. Simpson; L. Sinclair; P.-A. Söderström; T. Sumikama; Hiroshi Watanabe; A. Yagi; R. Yokoyama; N. Aoi; F. L. Bello Garrote; G. Benzoni; G. Gey; A. Gottardo; H. Nishibata; A. Odahara; H. Sakurai; M. Tanaka

A large fraction of the rare-earth elements observed in the solar system is produced in the astrophysical rapid neutron capture process (r-process). However, current stellar models cannot completely explain the relative abundance of these elements partially because of nuclear physics uncertainties. To address this problem, a β-decay spectroscopy experiment was performed at RI Beam Factory (RIBF) at RIKEN, aimed at studying a wide range of very neutron-rich nuclei with Z∼60 that are progenitors of the rare-earth elements with mass number A∼460. The experiment provides a test of nuclear models as well as experimental inputs for r-process calculations. This contribution presents the experimental setup and some preliminary results of the experiment.


Physical Review C | 2017

Nuclear structure and β -decay schemes for Te nuclides beyond N=82

B. Moon; C.-B. Moon; P.-A. Söderström; A. Odahara; R. Lozeva; B. Hong; F. Browne; H. S. Jung; P. Lee; C. S. Lee; A. Yagi; Cenxi Yuan; S. Nishimura; P. Doornenbal; G. Lorusso; T. Sumikama; Hiroshi Watanabe; I. Kojouharov; T. Isobe; H. Baba; H. Sakurai; R. Daido; Y. Fang; H. Nishibata; Z. Patel; S. Rice; L. Sinclair; Jinguang Wu; Z.Y. Xu; R. Yokoyama

We study for the first time the internal structure of 140Te through the beta-delayed gamma-ray spectroscopy of 140Sb. The very neutron-rich 140Sb, Z = 51 and N = 89, ions were produced by the in-flight fission of 238U beam on a 9Be target at 345 MeV per nucleon at the Radioactive Ion Beam Factory, RIKEN. The half-life and spin-parity of 140Sb are reported as 124(30) ms and (4-), respectively. In addition to the excited states of 140Te produced by the beta-decay branch, the beta-delayed one-neutron and two-neutron emission branches were also established. By identifying the first 2+ and 4+ excited states of 140Te, we found that Te isotopes persist their vibrator character with E(4+)/E(2+) = 2. We discuss the distinctive features manifest in this region, such as valence neutron symmetry and asymmetry, revealed in pairs of isotopes with the same neutron holes and particles with respect to N = 82.


Physical Review Letters | 2016

New Isotopes and Proton Emitters Crossing the Drip Line in the Vicinity of

I. Celikovic; M. Lewitowicz; R. Gernhäuser; R. Krücken; S. Nishimura; H. Sakurai; D. S. Ahn; H. Baba; B. Blank; A. Blazhev; P. Boutachkov; F. Browne; P. Doornenbal; T. Faestermann; Y. Fang; N. Fukuda; J. Giovinazzo; N. Goel; M. Górska; S. Ilieva; N. Inabe; T. Isobe; A. Jungclaus; D. Kameda; Y.-K. Kim; Y. k. Kwon; I. Kojouharov; T. Kubo; N. Kurz; G. Lorusso

Several new isotopes, ^{96}In, ^{94}Cd, ^{92}Ag, and ^{90}Pd, have been identified at the RIKEN Nishina Center. The study of proton drip-line nuclei in the vicinity of ^{100}Sn led to the discovery of new proton emitters ^{93}Ag and ^{89}Rh with half-lives in the submicrosecond range. The systematics of the half-lives of odd-Z nuclei with T_{z}=-1/2 toward ^{99}Sn shows a stabilizing effect of the Z=50 shell closure. Production cross sections for nuclei in the vicinity of ^{100}Sn measured at different energies and target thicknesses were compared to the cross sections calculated by epax taking into account contributions of secondary reactions in the primary target.


Acta Physica Polonica B | 2015

^{100}

F. Browne; A. M. Bruce; T. Sumikama; I. Nishizuka; S. Nishimura; P. Doornenbal; G. Lorusso; Z. Patel; S. Rice; L. Sinclair; P.-A. Söderström; Hiroshi Watanabe; Jinguang Wu; Z.Y. Xu; H. Baba; N. Chiga; Raymond J. Carroll; R. Daido; F. Didierjean; Y. Fang; G. Gey; E. Ideguchi; N. Inabe; T. Isobe; D. Kameda; I. Kojouharov; N. Kurz; T. Kubo; S. Lalkovski; Z. Li

F. Browne et al.; 4 pags.; 2 figs.; Presented at the Zakopane Conference on Nuclear Physics “Extremes of the Nuclear Landscape”, Zakopane, Poland, August 31–September 7, 2014; PACS numbers: 21.10.Re, 21.10.Tg, 23.20.Js, 27.60.+j


ORIGIN OF MATTER AND EVOLUTION OF GALAXIES 2013: Proceedings of the 12th International Symposium on Origin of Matter and Evolution of Galaxies (OMEG12) | 2014

Sn

G. Lorusso; S. Nishimura; H. Baba; F. Browne; R. Daido; P. Doornenbal; F. Yifan; G. Gey; T. Isobe; H. S. Jung; Z. H. Li; D. Lubos; K. Moschner; H. Nishibata; Z. Patel; S. Rice; L. Sinclair; P.-A. Söderström; T. Sumikama; J. Taprogge; Zs. Vajta; Z.Y. Xu; Hiroshi Watanabe; Jinguang Wu; A. Yagi; K. Yoshinaga

EURICA is a project at the RIKEN Nishina Center aimed at studying a wide range of exotic nuclei through β-decay measurements and high-resolution γ-ray spectroscopy. During its first two years of operation, about 80 days of beam time have been dedicated to the project allowing the exploration of several very exotic regions of the nuclear chart, which include key nuclei such as 78Ni, 100Sn, 110Zr, 128Pd, and 138Sn. Data analysis of the EURICA experiments is currently ongoing.


XI Latin American Symposium on Nuclear Physics and Applications | 2016

GAMMA-RAY SPECTROSCOPY IN THE VICINITY OF 108 Zr

P.-A. Söderström; P. Doornenbal; G. Lorusso; S. Nishimura; J. Wu; Zhengyu Xu; H. Baba; G. Benzoni; F. Browne; G. Gey; T. Isobe; A. Jungclaus; G Kiss; I. Kojouharov; N. Kurz; D Lubos; K. Moschner; Z. Patel; V. H Phong; S. Rice; H. Sakurai; H. Schaffner; G. Simpson; Laura C. Sinclair; T. Sumikama; J. Taprogge; Zs Vajta; Hiroshi Watanabe; A. Yagi

β- and isomer-decay spectroscopy are sensitive probes of nuclear structure, and are often the only techniques capable of providing data for exotic nuclei that are produced with very low rates. Decay properties of exotic nuclei are also essential to model astrophysical events responsible for the evolution of the universe such as the rp- and r-processes. The EURICA project (EUROBALL RIKEN Cluster Array) has been launched in 2012 with the goal of performing spectroscopy of very exotic nuclei. Since 2012, five experimental campaigns have been successfully completed using fragmentation of 124Xe beam and in-flight-fission of 238U beam. In these proceedings we will introduce the experimental setup and highlight some key recent results around 78Ni, 132Sn, and 110Zn published during 2014 and 2015.


Physics Letters B | 2018

β-decay spectroscopy at RIBF: The EURICA project

A. I. Morales; G. Benzoni; H. Watanabe; G. de Angelis; S. Nishimura; L. Coraggio; A. Gargano; N. Itaco; T. Otsuka; Y. Tsunoda; P. Van Isacker; F. Browne; R. Daido; P. Doornenbal; Y. Fang; G. Lorusso; Z. Patel; S. Rice; L. Sinclair; P.-A. Söderström; T. Sumikama; J. J. Valiente-Dobón; J. Wu; Z.Y. Xu; A. Yagi; R. Yokoyama; H. Baba; R. Avigo; F. L. Bello Garrote; Nives Blasi

Abstract The low-lying structures of the midshell ν g 9 / 2 Ni isotopes 72Ni and 74Ni have been investigated at the RIBF facility in RIKEN within the EURICA collaboration. Previously unobserved low-lying states were accessed for the first time following β decay of the mother nuclei 72Co and 74Co. As a result, we provide a complete picture in terms of the seniority scheme up to the first ( 8 + ) levels for both nuclei. The experimental results are compared to shell-model calculations in order to define to what extent the seniority quantum number is preserved in the first neutron g 9 / 2 shell. We find that the disappearance of the seniority isomerism in the ( 8 1 + ) states can be explained by a lowering of the seniority-four ( 6 + ) levels as predicted years ago. For 74Ni, the internal de-excitation pattern of the newly observed ( 6 2 + ) state supports a restoration of the normal seniority ordering up to spin J = 4 . This property, unexplained by the shell-model calculations, is in agreement with a dominance of the single-particle spherical regime near 78Ni.

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P. Doornenbal

GSI Helmholtz Centre for Heavy Ion Research

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G. Lorusso

Michigan State University

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G. Gey

Joseph Fourier University

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Z. Y. Xu

University of Hong Kong

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