Coulomb Dissociation of Proton-Rich sd-shell Nuclei for Astrophysical Interest and Their Implications.

التفاصيل البيبلوغرافية
العنوان: Coulomb Dissociation of Proton-Rich sd-shell Nuclei for Astrophysical Interest and Their Implications.
المؤلفون: Yoneda, Ken-ichiro
المصدر: AIP Conference Proceedings; 1/24/2008, Vol. 972 Issue 1, p240-248, 9p, 1 Diagram, 3 Graphs
مصطلحات موضوعية: NUCLEAR reactions, NUCLEAR astrophysics, RADIOISOTOPES, PROTON decay, PARTICLES (Nuclear physics)
مستخلص: Two astrophysical reactions, 22Mg(p,γ)23Al and 26Si(p,γ)27P, were investigated by using the Coulomb breakup of proton-rich isotopes 23Al and 27P. The radiative widths determined from the cross sections suggest that the β+ decay of 22Mg is favored over the 22Mg(p,γ)23Al reaction, while 26Si(p,γ)27P reaction is faster than the β+ decay of 26Si around the peak temperature of heavy novae. Two-neutron knockout reactions of the proton-rich sd-shell isotopes 26Si, 30S, and 34Ar were also studied. The measured branching ratios are well reproduced by a theoretical calculation which takes into account nucleon-nucleon correlation in a nucleus. [ABSTRACT FROM AUTHOR]
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قاعدة البيانات: Complementary Index
الوصف
تدمد:0094243X
DOI:10.1063/1.2870291