Matter radii of {sup 32-35}Mg

Journal Article · Tue Feb 15 00:00:00 EST 2011 · Physical Review. C, Nuclear Physics

DOI:https://doi.org/10.1103/PHYSREVC.83.021302· OSTI ID:21499390

Kanungo, R; Perro, C ^[1]; Prochazka, A; Farinon, F; Knoebel, R ^[2]; Horiuchi, W; Nociforo, C; Aumann, T; Geissel, H; Gerl, J; Kindler, B; Lommel, B; Mahata, K; Scheidenberger, C; Weick, H; Winkler, M ^[2]; Boutin, D; Lenske, H ^[3]; Cortina-Gil, D ^[4]; Davids, B ^[5]

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1. Astronomy and Physics Department, Saint Mary's University, Halifax, Nova Scotia B3H 3C3 (Canada)
2. GSI Helmholtzzentrum fuer Schwerionenforschung, D-64291 Darmstadt (Germany)
3. Justus-Liebig University, D-35392 Giessen (Germany)
4. Universidad de Santiago de Compostela, E-15706 Santiago de Compostella (Spain)
5. TRIUMF, Vancouver, British Columbia V6T 2A3 (Canada)

The interaction cross sections of {sup 32-35}Mg at 900A MeV have been measured using the fragment separator at GSI. The deviation from the r{sub 0}A{sup 1/3} trend is slightly larger for {sup 35}Mg, signaling the possible formation of a longer tail in the neutron distribution for {sup 35}Mg. The radii extracted from a Glauber model analysis with Fermi densities are consistent with models predicting the development of neutron skins.

• OSTI ID: 21499390
• Journal Information: Physical Review. C, Nuclear Physics, Vol. 83, Issue 2; Other Information: DOI: 10.1103/PhysRevC.83.021302; (c) 2011 American Institute of Physics; ISSN 0556-2813
• Country of Publication: United States
• Language: English

Related Subjects

73 NUCLEAR PHYSICS AND RADIATION PHYSICS
CROSS SECTIONS
DISTRIBUTION
INTERACTIONS
MAGNESIUM 32
MAGNESIUM 33
MAGNESIUM 34
MAGNESIUM 35
MEV RANGE 100-1000
NEUTRONS
SIMULATION
ALKALINE EARTH ISOTOPES
BARYONS
BETA DECAY RADIOISOTOPES
BETA-MINUS DECAY RADIOISOTOPES
ELEMENTARY PARTICLES
ENERGY RANGE
EVEN-EVEN NUCLEI
EVEN-ODD NUCLEI
FERMIONS
HADRONS
ISOTOPES
LIGHT NUCLEI
MAGNESIUM ISOTOPES
MEV RANGE
NUCLEI
NUCLEONS
RADIOISOTOPES