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exotic nuclei structure and reaction noyaux exotiques ... - IPN - IN2P3

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the 605.9 keV line of the 74 Zn 2+ to gs transition,<br />

the 449.6 keV line from 73 Zn 3/2- to gs transition<br />

<strong>and</strong> a 653. keV line identified as 72 Zn 2+ to gs<br />

transition. In order to obtain these spectra a<br />

background subtraction was necessary.<br />

The background in this experiment can be divided<br />

in two type: prompt <strong>and</strong> r<strong>and</strong>om. The r<strong>and</strong>om<br />

background originate from room background, <strong>and</strong><br />

beta decay of the secondary beam stopped on the<br />

collimator slits placed at 2 m in front of the<br />

PLUNGER target. The prompt background is<br />

mainly composed of 511 keV line <strong>and</strong> gamma<br />

originating from (n,n' gamma) <strong>reaction</strong>s in the<br />

germanium detectors. The neutrons who interact<br />

with the germanium detectors are produced from<br />

the breakup of the deuterium found in the target<br />

<strong>and</strong> from the fusion-evaporation <strong>reaction</strong>s induced<br />

by secondary beam impinging the target <strong>and</strong><br />

degrader.<br />

Using the data obtained for 562,93 keV line from<br />

76 Ge in this experiment the lifetime extracted for<br />

76 Ge 2+ state is consistent with the tabulated value<br />

of 26.27(29) ps [12]. The distance between the<br />

target <strong>and</strong> degrader used are 1.2, 1.5, 3.0 <strong>and</strong> 20<br />

mm.<br />

The data for 74 Zn are under analysis. In the<br />

literature the values extracted from Coulomb<br />

excitation measurements supposing an quadrupole<br />

moment equal with 0 are 24.8(20) ps [13] <strong>and</strong> 24.5<br />

(17) ps [14].<br />

References<br />

[1] R. Broda et al., Phys. Rev. Lett. 74, 868 (1995)<br />

[2] R. Grzywacz et al., Phys. Rev. Lett. 81, 766<br />

(1998)<br />

[3] H. Grawe, Nucl. Phys. A704, 211c (2002)<br />

[4] M. Sawicka et al., Phys. Rev. C 68, 044304<br />

(2003)<br />

[5] T. Ishii et al., Phys. Rev. Lett. 84, 39 (2000)<br />

[6] O. Sorlin et al., Phys. Rev. Lett. 88, 092501<br />

(2002)<br />

[7] K. Langanke et al., Phys. Rev. C67, 044314<br />

(2003)<br />

[8] T. Otsuka et al., Phys. Rev. Lett. 87, 082502<br />

(2001)<br />

[9] T. Otsuka et al., Phys. Rev. Lett. 95, 232502<br />

(2005)<br />

[10] H. Grawe, Springer Lect. Notes in Phys. 651,<br />

33 (2004)<br />

[11] J.P. Dufour et al., NIM A 248, 267 (1986)<br />

[12] R. Lecomte Phys. Rev. C 22, 1530–1533<br />

(1980)<br />

[13] J. Van de Walle et al. Phys. Rev. C 79,<br />

014309 (2009)<br />

[14] O. Perru et al. Phys. Rev. Lett. 96, 232501<br />

(2006)<br />

18

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