1979
DOI: 10.1016/0370-1573(79)90048-6
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Isospin effect in photoproton reaction on heavy nuclei

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Cited by 33 publications
(8 citation statements)
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“…2. The results for r pn = Np Nn vary smoothly from 1 in 12 C and 16 O to 3.5 in 40 Ca, in good agreement with the σ(γ,p) σ(γ,n) trend although not with the magnitude. In fact, it is known that the Np Nn ratio is representative of σ(γ,p) σ(γ,n) for the lower energy half of the GDR and it is associated with the statistical nature of the levels in the residual nuclei [24].…”
Section: Open Channelssupporting
confidence: 62%
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“…2. The results for r pn = Np Nn vary smoothly from 1 in 12 C and 16 O to 3.5 in 40 Ca, in good agreement with the σ(γ,p) σ(γ,n) trend although not with the magnitude. In fact, it is known that the Np Nn ratio is representative of σ(γ,p) σ(γ,n) for the lower energy half of the GDR and it is associated with the statistical nature of the levels in the residual nuclei [24].…”
Section: Open Channelssupporting
confidence: 62%
“…Instead, isospin symmetry is broken by the Coulomb force and the sum rules for transition strengths, shown in Fig. 3, favors the (γ, p) decay from the T = 1 resonance [40,60]. This, together with the fact that neutron emission to the T = 1/2 residual states is highly suppressed because of their expected high excitation energies -i.e.…”
Section: Isospin Selection Rulesmentioning
confidence: 98%
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“…The (n,p) charge exchange reaction (85) excites numerous spin-fl ip transitions, which severely hinder the data analysis. The failure of electron scattering (86) to see the isovector monopole is more subtle. Because the electron is a weak…”
Section: Giant Isovector Monopole Resonancementioning
confidence: 99%