Determination of the astrophysical S(E) factor for the 16O+16O reaction
This work aims to obtain the fusion excitation function for the 16O+16O system through gamma-spectroscopy measurements and gamma-charged particle coincidence, using the Saci-Perere system mounted at the end of the 30A beamline of the Open Laboratory of Nuclear Physics of the University of São Pa...
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| Language: | English |
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Universidade de São Paulo
2015
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| Online Access: | http://www.teses.usp.br/teses/disponiveis/43/43134/tde-06072015-050254/ |