2003
DOI: 10.1016/s0375-9474(03)01554-9
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Nuclear resonance fluorescence experiments on 204,206,207,208Pb up to 6.75 MeV

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Cited by 88 publications
(59 citation statements)
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“…The low-energy dipole states have been observed in a number of nuclei: neutron-rich O isotopes [1,2], 26 Ne [3], stable Ca isotopes [4,5], 56 Fe and 58 Ni [6], 68 Ni [7], 88 Sr [8], 90 Zr [9,10], Sn isotopes [11][12][13][14][15], N = 82 isotones [16][17][18][19][20][21], and stable Pb isotopes [22][23][24][25][26]. The observed low-energy E1 strength exhausts less than 1% of the Thomas-Reiche-Kuhn (TRK) sum-rule value in stable isotopes, while it may amount up to about 5% in neutron-rich nuclei.…”
Section: Introductionmentioning
confidence: 99%
“…The low-energy dipole states have been observed in a number of nuclei: neutron-rich O isotopes [1,2], 26 Ne [3], stable Ca isotopes [4,5], 56 Fe and 58 Ni [6], 68 Ni [7], 88 Sr [8], 90 Zr [9,10], Sn isotopes [11][12][13][14][15], N = 82 isotones [16][17][18][19][20][21], and stable Pb isotopes [22][23][24][25][26]. The observed low-energy E1 strength exhausts less than 1% of the Thomas-Reiche-Kuhn (TRK) sum-rule value in stable isotopes, while it may amount up to about 5% in neutron-rich nuclei.…”
Section: Introductionmentioning
confidence: 99%
“…208 Pb has always been a benchmark and the PDR has been studied in various recent (γ, γ ′ ) experiments [14][15][16][17]. Theoretically, closed-shell nuclei permit the inclusion of complex degrees of freedom beyond the mean-field level in the microscopic calculations [14,18].…”
Section: The Heaviest Stable Doubly Magic Nucleusmentioning
confidence: 99%
“…The remaining redundant N r − N n coefficients are undetermined and, therefore, can be safely put equal to zero. The eigenvalue problem within the n-phonon subspace is thereby solved exactly and yields a basis of orthonormal correlated n-phonon states of the form (8).…”
Section: Brief Description Of the Methodsmentioning
confidence: 99%
“…Radioactive beam experiments have extracted an appreciable dipole strength just above the neutron decay threshold in unstable nuclei, like neutron rich oxygen [3] or tin isotopes around 132 Sn [4]. More detailed data were obtained for stable nuclei by combining (γ, γ ′ ) [5][6][7][8][9][10][11][12][13][14] with (α, α ′ γ) measurements [15][16][17][18] which have detected rich low lying spectra of weakly excited discrete levels below the neutron threshold over different mass regions.…”
Section: Introductionmentioning
confidence: 99%