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      Nuclear Charge Radii of Be-7,9,10 and the one-neutron halo nucleus Be-11

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          Abstract

          Nuclear charge radii of \(^{7,9,10,11}\)Be have been determined by high-precision laser spectroscopy. On-line measurements were performed with collinear laser spectroscopy in the \(2s_{1/2} \to 2p_{1/2}\) transition on a beam of Be\(^{+}\) ions. Collinear and anticollinear laser beams were used simultaneously and the absolute frequency determination using a frequency comb yielded an accuracy in the isotope-shift measurements of about 1 MHz. Combination with accurate calculations of the mass-dependent isotope shifts yield nuclear charge radii. The charge radius decreases from \(^7\)Be to \(^{10}\)Be and then increases for the halo nucleus \(^{11}\)Be. When comparing our results with predictions of {\it ab initio} nuclear structure calculations we find good agreement. Additionally, the nuclear magnetic moment of \(^7\)Be was determined to be \(-1.3995(5)\mu_{\rm N}\) and that of \(^{11}\)Be from a previous \(\beta\)-NMR measurement was confirmed.

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          Quantum Monte Carlo Calculations of Light Nuclei

          Accurate quantum Monte Carlo calculations of ground and low-lying excited states of light p-shell nuclei are now possible for realistic nuclear Hamiltonians that fit nucleon-nucleon scattering data. At present, results for more than 30 different (J^pi;T) states, plus isobaric analogs, in A \leq 8 nuclei have been obtained with an excellent reproduction of the experimental energy spectrum. These microscopic calculations show that nuclear structure, including both single-particle and clustering aspects, can be explained starting from elementary two- and three-nucleon interactions. Various density and momentum distributions, electromagnetic form factors, and spectroscopic factors have also been computed, as well as electroweak capture reactions of astrophysical interest.
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            Quantum Monte Carlo calculations of \(A=9,10\) nuclei

            We report on quantum Monte Carlo calculations of the ground and low-lying excited states of \(A=9,10\) nuclei using realistic Hamiltonians containing the Argonne \(v_{18}\) two-nucleon potential alone or with one of several three-nucleon potentials, including Urbana IX and three of the new Illinois models. The calculations begin with correlated many-body wave functions that have an \(\alpha\)-like core and multiple p-shell nucleons, \(LS\)-coupled to the appropriate \((J^{\pi};T)\) quantum numbers for the state of interest. After optimization, these variational trial functions are used as input to a Green's function Monte Carlo calculation of the energy, using a constrained path algorithm. We find that the Hamiltonians that include Illinois three-nucleon potentials reproduce ten states in \(^9\)Li, \(^9\)Be, \(^{10}\)Be, and \(^{10}\)B with an rms deviation as little as 900 keV. In particular, we obtain the correct 3\(^+\) ground state for \(^{10}\)B, whereas the Argonne \(v_{18}\) alone or with Urbana IX predicts a 1\(^+\) ground state. In addition, we calculate isovector and isotensor energy differences, electromagnetic moments, and one- and two-body density distributions.
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              Bethe Logarithm and QED Shift for Lithium

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                Author and article information

                Journal
                15 September 2008
                2009-02-05
                Article
                10.1103/PhysRevLett.102.062503
                0809.2607
                fcddf0e9-c782-4e12-86f6-7156aad3d56a

                http://arxiv.org/licenses/nonexclusive-distrib/1.0/

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                Phys.Rev.Lett.102:062503,2009
                4 pages, 2 figures calculated mass shift values have been re-evaluated with the latest mass values for the beryllium isotopes and the nuclear polarization contribution for Be-11, published by K. Pachucki et al. ater submission of our manuscript, is also included now
                nucl-ex

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