Observation of 10He

Korsheninnikov, A. A.; Yoshida, Kôichi; Aleksandrov, D.; Aoi, N.; Doki, Y.; Inabe, N.; Fujimaki, M.; Kobayashi, Toshio; Kumagai, Hiroshi; Moon, C.-B.; Nikolskii, E. Yu.; Obuti, M.M.; Ogloblin, A. A.; Ozawa, A.; Shimoura, S.; Suzuki, Takeshi; Tanihata, I.; Watanabe, Y.; Yanokura, Minoru

doi:10.1016/0370-2693(94)91188-6

Cited by 107 publications

(59 citation statements)

References 18 publications

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“…For example, proton elastic scattering angular distributions were measured at incident energies less than 100 MeV/nucleon for He isotopes (e.g., Refs. [11][12][13][14][15][16][17][18][19][20]) and Li isotopes (e.g., Refs. [9,16]) and at an energy of 700 MeV/nucleon for the same nuclei at GSI (Darmstadt) (e.g., Refs.…”

Section: Introductionmentioning

confidence: 99%

Charge and matter distributions and form factors of light, medium, and heavy neutron-rich nuclei

et al. 2005

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Results of charge form factors calculations for several unstable neutron-rich isotopes of light, medium, and heavy nuclei (He, Li, Ni, Kr, Sn) are presented and compared to those of stable isotopes in the same isotopic chain. For the lighter isotopes (He and Li) the proton and neutron densities are obtained within a microscopic large-scale shell-model, while for heavier ones Ni, Kr, and Sn the densities are calculated in deformed self-consistent mean-field Skyrme HF+BCS method. We also compare proton densities to matter densities together with their rms radii and diffuseness parameter values. Whenever possible comparison of form factors, densities and rms radii with available experimental data is also performed. Calculations of form factors are carried out both in plane wave Born approximation (PWBA) and in distorted wave Born approximation (DWBA). These form factors are suggested as predictions for the future experiments on the electron-radioactive beam colliders where the effect of the neutron halo or skin on the proton distributions in exotic nuclei is planned to be studied and thereby the various theoretical models of exotic nuclei will be tested.

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Section: Introductionmentioning

confidence: 99%

Charge and matter distributions and form factors of light, medium, and heavy neutron-rich nuclei

et al. 2005

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“…Instead, direct reactions with RNB can be done in inverse kinematics where the role of beam and target are interchanged. For example, the proton elastic-scattering angular distributions were measured for several incident energies, namely 25.1A MeV [6,7], 41.6A MeV [8,9,10] and 71A MeV [11,12] for 6 He, 26.25A MeV (the preliminary data obtained in Dubna [13]), 32A MeV [11,12], 66A MeV [11,12] and 73A MeV [11,12,14,15] for 8 He, as well as for energies less than 100A MeV [11,1] in the cases of 6 Li, 11 Li and others. In some of the theoretical analyses (e.g.…”

Section: Introductionmentioning

confidence: 99%

Charge Density Distributions and Related Form Factors in Neutron-Rich Light Exotic Nuclei

Antonov

Gaidarov

Kadrev

et al. 2004

Int. J. Mod. Phys. E

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Charge form factors corresponding to proton density distributions in exotic nuclei, such as 6,8 He, 11 Li, 17,19 B and 14 Be are calculated and compared. The results can be used as tests of various theoretical models for the exotic nuclei structure in possible future experiments using a colliding electron-exotic nucleus storage ring. The result of such a comparison would show the effect of the neutron halo or skin on the proton distributions in exotic nuclei.

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“…The system 10 He has already been discovered and studied in the 1990s [60][61][62]. It has also been shown [63] that the strength of interaction observed in 9 He = 8 He + n strongly affects the ground-state properties of 10 He.…”

Section: Across the Drip-line: 10 Hementioning

confidence: 99%

Halo nuclei, stepping stones across the drip-lines

Simon

2013

Phys. Scr.

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Observation of 10He

Cited by 107 publications

References 18 publications

Charge and matter distributions and form factors of light, medium, and heavy neutron-rich nuclei

Charge and matter distributions and form factors of light, medium, and heavy neutron-rich nuclei

Charge Density Distributions and Related Form Factors in Neutron-Rich Light Exotic Nuclei

Halo nuclei, stepping stones across the drip-lines

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