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Phys. Rev. C 65, 024610 (2002) [5 pages]

Existence of a proton halo in 23Al and its significance

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X. Z. Cai1, H. Y. Zhang1, W. Q. Shen1,2,5, Z. Z. Ren4, J. Feng1, D. Q. Fang1, Z. Y. Zhu1, W. Z. Jiang1, Y. G. Ma1,2, C. Zhong1, W. L. Zhan3, Z. Y. Guo3, G. Q. Xiao3, J. S. Wang3, Y. T. Zhu3, J. C. Wang3, J. X. Li3, M. Wang3, J. F. Wang3, Z. J. Ning3, Q. J. Wang3, and Z. Q. Chen3
1Shanghai Institute of Nuclear Research, Chinese Academy of Sciences, Shanghai 201800, China
2CCAST (World Laboratory), P.O. Box 8730, Beijing 100080, China
3Institute of Modern Physics, Chinese Academy of Sciences, Lanzhou 730000, China
4Physics Department of Nanjing University, Nanjing 210008, China
5Physics Department of Ningbo University, Ningbo 315211, China

Received 21 June 2001; published 16 January 2002

Reaction cross section σR of proton-rich isotones (N=10) near 23Al and Al isotopes (23-28Al) on C target have been measured at intermediate energies around 30 MeV/nucleon. An abnormal increase of the experimental σR is observed for 23Al and it suggests that there is an anomalously large matter rms radius in 23Al. Together with the very weakly binding of the last proton (Sp=0.125MeV), it indicates that there is a proton halo in 23Al. This conclusion is also supported by the difference factor d which is deduced from the measured and theoretical σR in the Glauber or Boltzmann-Uehling-Uhlenbeck model and is used for the manifest of halo phenomena. The theoretical calculation based on the relativistic density dependent Hartree model shows that there is a proton halo when the last proton is in the 2s1/2 orbit in 23Al. The significance of the proton halo in 23Al is discussed.

© 2002 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevC.65.024610
DOI:
10.1103/PhysRevC.65.024610
PACS:
25.60.Dz, 21.10.Ft, 27.30.+t