1956
DOI: 10.1103/physrev.103.1035
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Electric-Monopole Transitions in Atomic Nuclei

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Cited by 233 publications
(44 citation statements)
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“…The IC process for E0 occurs primarily through the 1s(K) and 2s(L 1 ) shells. Typical probabilities [14][15][16] for IC in the various atomic subshells are P K :P L1 :P L2 :P L3 : P M1 = 0.83 : 0.13 : 10 −3 : 10 −9 : 0.04. The E0 transition rate,…”
Section: A Introductionmentioning
confidence: 99%
“…The IC process for E0 occurs primarily through the 1s(K) and 2s(L 1 ) shells. Typical probabilities [14][15][16] for IC in the various atomic subshells are P K :P L1 :P L2 :P L3 : P M1 = 0.83 : 0.13 : 10 −3 : 10 −9 : 0.04. The E0 transition rate,…”
Section: A Introductionmentioning
confidence: 99%
“…The coefficient σ depends on the assumed nuclear charge distribution but in any reasonable case it is smaller than 0.1 and can be neglected if the leading term is not too small [1]. The charge radius of a state |s is given by…”
mentioning
confidence: 99%
“…For transition energies greater than 2m e c 2 , electronpositron pair creation is also possible; two-photon emission is possible at all energies but extremely improbable. The total probability for a transition between initial and final states |i and |f can be separated into an electronic and a nuclear factor, P = Ωρ 2 , where the nuclear factor ρ is [1] …”
mentioning
confidence: 99%
“…2) and from the γ-times (relative to the beta-triggers) of 511 keV photons, many of them following the annihilation of positrons originating from E0 transition. Based on tabulated [13][14][15] electronic factors Γ IC =3.68x107 s −1 and Γ IPF =2.69x109 s −1 , the monopole strength ρ 2 (E0,0 + 2 →0 + 1 )=13.0(0.9) 10 −3 is extracted. A 607 keV gamma peak corresponding to the transition from the 2 + 1 state at 3326 keV to the 0 + 2 state is observed with a very small intensity in the gamma spectrum with a multiplicity higher than 2 for the Si detectors.…”
Section: Experimental Setup and Resultsmentioning
confidence: 99%