Internal Conversion Spectrum ofAu198

1956 ◽  
Vol 102 (6) ◽  
pp. 1584-1586 ◽  
Author(s):  
Donald R. Connors ◽  
Walter C. Miller ◽  
Bernard Waldman
1969 ◽  
Vol 24 (12) ◽  
pp. 1893-1897 ◽  
Author(s):  
E Bashandy

AbstractThe internal conversion spectrum of γ transitions in the decay of 99Mo has been re-studied using a high resolution double focusing β-ray spectrometer. In addition to γ-rays previously reported, seven more γ-rays could be observed. Internal conversion coefficients and multipolarities of γ transitions are given. Energies, spins and parities of high excited levels in 99Tc are confirmed.


1957 ◽  
Vol 35 (5) ◽  
pp. 672-692 ◽  
Author(s):  
G. T. Ewan

Au193 has been produced as the daughter of Hg193 formed by the reaction Au197(p, 5n)Hg193 in the McGill synchrocyclotron. The internal conversion spectrum and unconverted γ-ray spectrum have been examined using β-ray spectrometers, Nal spectrometers, and coincidence techniques. Au193 decays by electron capture to Pt193 with a half-life of 17.5 ± 0.2 hr. An upper limit of 0.08% per disintegration has been placed on the probability of emission of positrons in this decay. Twenty-eight γ-rays, all below 500 kev., have been observed associated with the decay of Au193. The first excited state of Pt193 has been shown to be at 12.7 kev. and the lifetime of this state measured as (2.2 ± 0.8) × 10−9sec. A level scheme is proposed for Pt193.


1967 ◽  
Vol 100 (2) ◽  
pp. 351-368 ◽  
Author(s):  
Ö. Nilsson ◽  
S. Högberg ◽  
S.-E. Karlsson ◽  
G.M. El-Sayad

1962 ◽  
Vol 39 ◽  
pp. 613-620 ◽  
Author(s):  
J.L. Wolfson ◽  
J.J.H. Park ◽  
L. Yaffe

1967 ◽  
Vol 22 (3) ◽  
pp. 299-308
Author(s):  
M. S. El-Nesr ◽  
M. R. El-Aassar

A photoline spectrum from the γ rays of energies greater than 200 keV following the decay of 40-hour 140La has been studied using a high resolution double focusing ß-ray spectrometer. The photoelectrons are produced from an uranium radiator of thickness 2.9 mg/cm2. The resulting momentum resolution was 0.3 → 0.8% depending on energy. In addition to γ rays previously reported, we have observed 17 new γ transitions in the energy region of about one MeV to 2.53 MeV. The relative γ-ray intensities have been determined from the external conversion spectrum applying the corrections for the angular dependence of the photo-electric process. Gamma energies and intensities higher than 2.53 MeV have been investigated by means of a scintillation spectrometer using a RiDL-transistorized 400 channel analyzer. A complete set of energy sums was computed in order to survey the possibilities of cascade crossover combinations. Thirteen direct ground state transitions of energies 204.87, 241.95, 993.12, 1597.48, 1973.38, 2026.37, 2350.23, 2371.11, 2410.33, 2530.03, 2900, 3100 and 3471 keV were observed. A few modifications on the previously reported level scheme of 140Ce are proposed after the addition of the 17 new γ rays. Conversion coefficients were obtained by normalizing the ratios of conversion and photon intensities with respect to the 487 keV-E2 transition in 140Ce. From the known internal conversion coefficient of this transition, the absolute K-internal conversion coefficients of the transitions 200.08, 241.95, 273.69, 337.50, 374.81, 400.53 and 875.30 keV were determined to confirm their multipolarities and support spin and parity assignments of the levels 242, 617, 1260, 1323, 2184, 2515, 2585 and 3390 keV.The absolute K-internal conversion coefficients of the 542.43, 641.41, 752.62, 927.41, 980.19, 1016.20, 1040.31 and 1054.65 keV transitions were measured for the first time. The multipolarity assignments of these transitions were studied on the basis of the conversion coefficients. These measurements together with the previously known assigned levels establish the spins and parities 3-, 0+, 2+, 4+, 2+, and 2+ for the levels 205, 1889, 1973, 2084, 2350 and 2530 keV, respectively. Spin and parity assignments of 1+ and 4- are proposed for the 2900 and 3100 keV excited levels in 140Ce respectively.


1964 ◽  
Vol 42 (7) ◽  
pp. 1387-1410 ◽  
Author(s):  
J. L. Wolfson ◽  
J. J. H. Park

The low-energy gamma-ray transitions in Np237 following α decay of Am241 have been studied by examination of the internal conversion spectrum at good resolution. Improved measurements of the energies and intensities of the lines due to the well-known transitions of energies 26.36, 33.21, 43.44, 55.56, 59.57, and 99.00 keV have been made. The existence of a weak transition of energy 67.52 keV has been confirmed. The existence of weak transitions of energies 27, 42.8, 70, and 76 keV, previously reported, has not been substantiated.For the 43.44-keV transition the L subshell ratios LI/LIII and LII/LIII are in disagreement as to the proportion of E2 component in the M1, E2 mixture assigned to this radiation, while the M subshell ratios are in disagreement with both L subshell ratios.The binding energies of the L, M, and N subshells in Np have been measured. All values are slightly higher than found by extrapolation from values at lower Z, though within experimental uncertainty the values are in agreement with such extrapolations.


1964 ◽  
Vol 2 (4) ◽  
pp. 241-262 ◽  
Author(s):  
S. Forberg ◽  
E. Odeblad ◽  
R. Söremark ◽  
S. Ullberg

In a previous paper the absorption of γ-rays in the K-X-ray levels of the atom in which they are emitted was calculated according to the Quantum Mechanics, supposing the γ-rays to be emitted from a doublet of moment f ( t ) at the centre of the atom. The non-relativity wave equation derived from the relativity wave equation for an electron of charge — ε moving in an electro-magnetic field of vector potential K and scalar potential V is h 2 ∇ 2 ϕ + 2μ ( ih ∂/∂ t + εV + ih ε/μ c (K. grad)) ϕ = 0. (1) Suppose, however, that K involves the space co-ordinates. Then, (K. grad) ϕ ≠ (grad . K) ϕ , and the expression (K . grad) ϕ is not Hermitic. Equation (1) cannot therefore be the correct non-relativity wave equation for a single electron in an electron agnetic field, and we must substitute h 2 ∇ 2 ϕ + 2μ ( ih ∂/∂ t + εV) ϕ + ih ε/ c ((K. grad) ϕ + (grad. K) ϕ ) = 0. (2)


2009 ◽  
Vol 79 (3) ◽  
Author(s):  
Péter Kálmán ◽  
Tamás Keszthelyi

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