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Matter radii of Na and Mg isotopes

✍ Scribed by T. Suzuki; H. Geissel; O. Bochkarev; L. Chulkov; M. Golovkov; D. Hirata; H. Irnich; Z. Janas; H. Keller; T. Kobayashi; G. Kraus; G. Muenzenberg; S. Neumaier; F. Nickel; A. Ozawa; A. Piechaczeck; E. Roeckl; W. Schwab; K. Suemmerer; K. Yoshida; I. Tanihata


Publisher
Elsevier Science
Year
1997
Tongue
English
Weight
519 KB
Volume
616
Category
Article
ISSN
0375-9474

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✦ Synopsis


The interaction cross sections (01) of ANa (A= 20-23,25-32) and AMg (A= 20,22-25, 27, 29-33) on a carbon target have been measured at a beam energy of around 950 A MeV. The effective root-mean-square matter radii of these isotopes were deduced from 01 by a Glauber-type calculation. Combining the isotope-shift data with the present Na data the radii of neutrons have been compared with those of protons for the first time along a chain of stable and unstable isotopes. A monotonic increase in the neutron skin thickness has been observed as the neutron number increases in Na isotopes. The Mg data are also consistent with the claim that the formation of a neutron/proton skin is a universal feature in P-unstable nuclei.


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Nuclear radii of Na and Mg isotopes
✍ T. Suzuki; H. Geissel; O. Bochkarev; L. Chulkov; M. Golovkov; N. Fukunishi; D. H πŸ“‚ Article πŸ“… 1998 πŸ› Elsevier Science 🌐 English βš– 862 KB

The effective root-mean-square (rms) matter radii of ANa (A = 20-23,25-32) and aMg (A = 20.22, 23, 27,29-32) have been deduced from the measured interaction cross sections using a Glauber-type calculation. It was found that the increase of rms matter radii in Na isotopes is primarily a consequence o