Isospin mixing in the hot compound nucleus Zr-80 was studied by measuring and comparing the gamma-ray emission from the fusion reactions Ca-40 + Ca-40 at E-beam = 200 MeV and Cl-37 + Ca-44 at E-beam = 153 MeV. The gamma yield associated with the giant dipole resonance is found to be different in the two reactions because, in self-conjugate nuclei, the E1 selection rules forbid the decay between states with isospin I = 0. The degree of mixing is deduced from statistical-model analysis of the gamma-ray spectrum emitted by the compound nucleus Zr-80 with the standard parameters deduced from the gamma decay of the nucleus Rb-81. The results are used to deduce the zero-temperature value, which is then compared with the latest predictions. The Coulomb spreading width is found to be independent of temperature.

Measurement of isospin mixing at a finite temperature in 80Zr via giant dipole resonance decay

Giaz, A.;
2011-01-01

Abstract

Isospin mixing in the hot compound nucleus Zr-80 was studied by measuring and comparing the gamma-ray emission from the fusion reactions Ca-40 + Ca-40 at E-beam = 200 MeV and Cl-37 + Ca-44 at E-beam = 153 MeV. The gamma yield associated with the giant dipole resonance is found to be different in the two reactions because, in self-conjugate nuclei, the E1 selection rules forbid the decay between states with isospin I = 0. The degree of mixing is deduced from statistical-model analysis of the gamma-ray spectrum emitted by the compound nucleus Zr-80 with the standard parameters deduced from the gamma decay of the nucleus Rb-81. The results are used to deduce the zero-temperature value, which is then compared with the latest predictions. The Coulomb spreading width is found to be independent of temperature.
2011
http://oai.aps.org/filefetch?identifier=10.1103/PhysRevC.84.041304&component=fulltext&description=markup&format=xml
Nuclear and High Energy Physics
Corsi, A.; Wieland, O.; Barlini, S.; Bracco, A.; Camera, F.; Kravchuk, V. L.; Baiocco, G.; Bardelli, L.; Benzoni, G.; Bini, M.; Blasi, N.; Brambilla, ...espandi
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11383/2101561
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