541 research outputs found

    Tetrahedral Symmetry in Ground- and Low-Lying States of Exotic A ~ 110 Nuclei

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    Recent theoretical calculations predict a possible existence of nuclei with tetrahedral symmetry: more precisely, the mean-field hamiltonians of such nuclei are symmetric with respect to double point-group Td. In this paper, we focus on the neutron-rich Zirconium isotopes as an example and present realistic mean-field calculations which predict tetrahedral ground-state configurations in 108,110Zr and low-lying excited states of tetrahedral symmetry in a number of N > 66 isotopes. The motivations for focusing on these nuclei, as well as a discussion of the possible experimental signatures of tetrahedral symmetry are also presented.Comment: Accepted in Phys. Rev. C - Rapid Communication

    Nuclear break-up of 11Be

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    The break-up of 11Be was studied at 41AMeV using a secondary beam of 11Be from the GANIL facility on a 48Ti target by measuring correlations between the 10Be core, the emitted neutrons and gamma rays. The nuclear break-up leading to the emission of a neutron at large angle in the laboratory frame is identified with the towing mode through its characteristic n-fragment correlation. The experimental spectra are compared with a model where the time dependent Schrodinger equation (TDSE) is solved for the neutron initially in the 11 Be. A good agreement is found between experiment and theory for the shapes of neutron experimental energies and angular distributions. The spectroscopic factor of the 2s orbital is tentatively extracted to be 0.46+-0.15. The neutron emission from the 1p and 1d orbitals is also studied

    Shell Model Study of the Neutron-Rich Nuclei around N=28

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    We describe the properties of the neutron rich nuclei around N=28 in the shell mode framework. The valence space comprises the sdsd shell for protons an the pfpf shell for neutrons without any restriction. Good agreement is found with the available experimental data. The N=28 shell closure, even if eroded due to the large neutron excess, persists. The calculations predict that 40^{40}S and 42^{42}S are deformed with β=0.29\beta=0.29 and β=0.32\beta=0.32 respectively.Comment: 17 pages and 19 figures, LateX, RevTe

    Towards a Multi-Scaled Functional-Structural Model of Apple, Linking Ecophysiology at the Fruit and Branch Scales

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    A multitude of data on eco-physiological processes in apple (Malus x domestica) is available, concerning various aspects of fruit growth and development, fruit quality, or leaf photosynthesis. However, despite the wealth of data and studies many processes leading to (inter-annual and intra-arboreal) heterogeneity in quantity of fruit production as well as fruit quality are still only poorly understood at the branch level Current Functional-Structural Plant Models of apple have targeted canopy architecture, i.e. development of vegetative structures. Here we will present a concept to apply the FSPM paradigm to the simulation of assimilation (source), transport and consumption (sink) of carbon in the context of a static structure representing the limb (fruit-bearing branch)

    Giant resonances in exotic spherical nuclei within the RPA approach with the Gogny force

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    Theoretical results for giant resonances in the three doubly magic exotic nuclei 78^{78}Ni, 100^{100}Sn and 132^{132}Sn are obtained from Hartree-Fock (HF) plus Random Phase Approximation (RPA) calculations using the D1S parametrization of the Gogny two-body effective interaction. Special attention is paid to full consistency between the HF field and the RPA particle-hole residual interaction. The results for the exotic nuclei, on average, appear similar to those of stable ones, especially for quadrupole and octupole states. More exotic systems have to be studied in order to confirm such a trend. The low energy of the monopole resonance in 78^{78}Ni suggests that the compression modulus in this neutron rich nucleus is lower than the one of stable ones.Comment: 16 pages, 10 figure

    Large scale shell model calculations for odd-odd 5862^{58-62}Mn isotopes

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    Large scale shell model calculations have been carried out for odd-odd 5862^{58-62}Mn isotopes in two different model spaces. First set of calculations have been carried out in full fp\it{fp} shell valence space with two recently derived fp\it{fp} shell interactions namely GXPF1A and KB3G treating 40^{40}Ca as core. The second set of calculations have been performed in fpg9/2{fpg_{9/2}} valence space with the fpgfpg interaction treating 48^{48}Ca as core and imposing a truncation by allowing up to a total of six particle excitations from the 0f7/2_{7/2} orbital to the upper fp\it{fp} orbitals for protons and from the upper fp\it{fp} orbitals to the 0g9/2_{9/2} orbital for neutron. For low-lying states in 58^{58}Mn, the KB3G and GXPF1A both predicts good results and for 60^{60}Mn, KB3G is much better than GXPF1A. For negative parity and high-spin positive parity states in both isotopes fpgfpg interaction is required. Experimental data on 62^{62}Mn is sparse and therefore it is not possible to make any definite conclusions. More experimental data on negative parity states is needed to ascertain the importance of 0g9/2_{9/2} and higher orbitals in neutron rich Mn isotopes.Comment: 5 pages, 4 figures, Submitted to Eur. Phys. J.

    How magic is the magic 68Ni nucleus?

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    We calculate the B(E2) strength in 68Ni and other nickel isotopes using several theoretical approaches. We find that in 68Ni the gamma transition to the first 2+ state exhausts only a fraction of the total B(E2) strength, which is mainly collected in excited states around 5 MeV. This effect is sensitive to the energy splitting between the fp shell and the g_{9/2}orbital. We argue that the small experimental B(E2) value is not strong evidence for the double-magic character of 68Ni.Comment: 4 pages, 4 figure

    Spectroscopy of 26^{26}F

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    The structure of the weakly-bound     926^{26}_{\;\;9}F17_{17} odd-odd nucleus, produced from 27,28^{27,28}Na nuclei, has been investigated at GANIL by means of the in-beam γ\gamma-ray spectroscopy technique. A single γ\gamma-line is observed at 657(7) keV in 926^{26}_{9}F which has been ascribed to the decay of the excited J=2+2^+ state to the J=1+^+ ground state. The possible presence of intruder negative parity states in 26^{26}F is also discussed.Comment: 3 pages, 1 figure, accepted for publication in Physical Review
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