1,576 research outputs found

    Lifetimes of 26Al and 34Cl in an astrophysical plasma

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    We study here the onset of thermal equilibrium affecting the lifetimes of 26Al and 34Cl nuclei within a hot astrophysical photon gas. The 26Al isotope is of prime interest for gamma ray astronomy with the observation of its delayed (t_1\2=0.74 My) 1.809MeV gamma-ray line. Its nucleosynthesis is complicated by the presence of a short lived (t_1\2=6.34s) spin isomer. A similar configuration is found in 34Cl where the decay of its isomer (34mCl, t_1\2=32m) is followed by delayed gamma-ray emission with characteristic energies. The lifetimes of such nuclei are reduced at high temperature by the thermal population of shorter lived levels. However, thermal equilibrium within 26Al and 34Cl levels is delayed by the presence of the isomer. We study here the transition to thermal equilibrium where branching ratios for radiative transitions are needed in order to calculate lifetimes. Since some of these very small branching ratios are not known experimentally, we use results of shell model calculations.Comment: 11 pages, 5 figures, Latex, accepted for publication in Phys. Rev.

    Nilsson-SU3 selfconsistency in heavy N=Z nuclei

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    It is argued that there exist natural shell model spaces optimally adapted to the operation of two variants of Elliott' SU3 symmetry that provide accurate predictions of quadrupole moments of deformed states. A selfconsistent Nilsson-like calculation describes the competition between the realistic quadrupole force and the central field, indicating a {\em remarkable stability of the quadruplole moments}---which remain close to their quasi and pseudo SU3 values---as the single particle splittings increase. A detailed study of the N=ZN=Z even nuclei from 56^{56}Ni to 96^{96}Cd reveals that the region of prolate deformation is bounded by a pair of transitional nuclei 72^{72}Kr and 84^{84}Mo in which prolate ground state bands are predicted to dominate, though coexisting with oblate ones,Comment: Replacement I) Title simplified. II) Major revision: structure of paper kept but two thirds totally rewritten (same number of pages); 20 references adde

    Intact Mucosa Coloplasty Pouch (IMCP) - a modification of colonic coloplasty pouch

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    Editorial

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    Deformation of the lowermost mantle from seismic anisotropy

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    Understanding the lowermost part of the Earth’s mantle—known as D''—can help us investigate whole-mantle dynamics, core-mantle interactions and processes such as slab deformation in the deep Earth. D'' shows significant seismic anisotropy, the variation of seismic wave speed with direction. This is likely due to deformation- induced alignment of MgSiO3-post-perovskite (ppv), believed to be the main mineral phase present in the region; however if this is the case, then previous measurements of D'' anisotropy, which are generally made in one direction only, are insufficient to distinguish candidate mechanisms of slip in ppv because the mineral is orthorhombic. Here we measure anisotropy in D'' beneath North and Central America, where slab material impinges6 on the core-mantle boundary (CMB), using shallow as well as deep earthquakes to increase the azimuthal coverage in D!. We make >700 individual measurements of shear wave splitting in D'' in three regions from two different azimuths in each case, and we show that the previously-assumed case of vertical transverse isotropy (VTI, where wave speed shows no azimuthal variation) is not possible; more complicated mechanisms must be involved. We test the fit of different MgSiO3-ppv deformation mechanisms to our results and find that shear on (001) is most consistent with observations and expected shear above the CMB beneath subduction zones. With new models of mantle flow, or improved experimental evidence of which ppv slip systems dominate, this method will allow us to map deformation at the CMB and link processes in D'', such as plume initiation, to the rest of the mantle

    Backbending in 50Cr

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    The collective yrast band and the high spin states of the nucleus 50Cr are studied using the spherical shell model and the HFB method. The two descriptions lead to nearly the same values for the relevant observables. A first backbending is predicted at I=10\hbar corresponding to a collective to non-collective transition. At I=16\hbar a second backbending occurs, associated to a configuration change that can also be interpreted as an spherical to triaxial transition.Comment: ReVTeX v 3.0 epsf.sty, 5 pages, 5 figures included. Full Postscript version available at http://www.ft.uam.es/~gabriel/Cr50art.ps.g

    Shell-model calculations of two-neutrino double-beta decay rates of 48^{48}Ca with GXPF1A interaction

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    The two-neutrino double beta decay matrix elements and half-lives of 48^{48}Ca, are calculated within a shell-model approach for transitions to the ground state and to the 2+2^+ first excited state of 48^{48}Ti. We use the full pfpf model space and the GXPF1A interaction, which was recently proposed to describe the spectroscopic properties of the nuclei in the nuclear mass region A=47-66. Our results are T1/2(0+0+)T_{1/2}(0^{+}\to 0^{+}) = 3.3×10193.3\times 10^{19} yryr and T1/2(0+2+)T_{1/2}(0^{+}\to 2^{+}) = 8.5×10238.5\times 10^{23} yryr. The result for the decay to the 48^{48}Ti 0+^+ ground state is in good agreement with experiment. The half-life for the decay to the 2+^+ state is two orders of magnitude larger than obtained previously.Comment: 6 pages, 4 figure
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