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| Hauptseite > Publikationsdatenbank > Resolution of a discrepancy in the γ -ray emission probability from the β decay of Ce g 137 > print |
| Hauptseite > Publikationsdatenbank > Resolution of a discrepancy in the γ -ray emission probability from the β decay of Ce g 137 > print |
| 001 | 886126 | ||
| 005 | 20230217124324.0 | ||
| 024 | 7 | _ | |a 10.1103/PhysRevC.101.064619 |2 doi |
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| 024 | 7 | _ | |a 1089-490X |2 ISSN |
| 024 | 7 | _ | |a 1538-4497 |2 ISSN |
| 024 | 7 | _ | |a 2469-9985 |2 ISSN |
| 024 | 7 | _ | |a 2469-9993 |2 ISSN |
| 024 | 7 | _ | |a 2470-0002 |2 ISSN |
| 024 | 7 | _ | |a 2128/26063 |2 Handle |
| 024 | 7 | _ | |a WOS:000541414000001 |2 WOS |
| 037 | _ | _ | |a FZJ-2020-04289 |
| 082 | _ | _ | |a 530 |
| 100 | 1 | _ | |a Basunia, M. S. |0 0000-0002-2643-0901 |b 0 |
| 245 | _ | _ | |a Resolution of a discrepancy in the γ -ray emission probability from the β decay of Ce g 137 |
| 260 | _ | _ | |a Woodbury, NY |c 2020 |b Inst. |
| 264 | _ | 1 | |3 online |2 Crossref |b American Physical Society (APS) |c 2020-06-19 |
| 264 | _ | 1 | |3 print |2 Crossref |b American Physical Society (APS) |c 2020-06-01 |
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| 520 | _ | _ | |a We have deduced the emission probability of the 447-keV γ ray from the ɛ+β+ decay of 137Ceg (9.0 h) relative to that of the 254-keV γ ray from the 137Cem (34.4 h) decay in transient equilibrium. The time-dependent factor in transient equilibrium was applied following the Bateman equation for a radioactive decay chain. The isotope was produced via the 139La(p,3n)137Cem,g reaction by bombarding natLa with a proton beam from the 88-in. cyclotron at Lawrence Berkeley National Laboratory. γ-ray intensities were measured using an HPGe detector. The emission probability for the 447-keV γ ray deduced in this work is 1.21(3) (that is 1.21 ± 0.03) per hundred parent decays, which differs significantly from an earlier published value of 2.24(10). We identify the source of this discrepancy to be an incorrect use of the time-dependent factor. Additionally, we have deduced the emission probability of the 504-keV γ ray from the decay of 85Yg (2.68 h) relative to that of the 232-keV γ ray from the 85Srm (1.127 h) decay in transient equilibrium. The isotope was produced via the 86Sr(p,2n)85Yg reaction by bombarding 86SrCO3 with a proton beam at the same facility. The study confirms the assumption of the time-dependent correction for recommending the emission probability of the 504-keV γ ray in the literature. Our work highlights the importance of explicit description by authors of any time-dependent correction they have made when reporting γ-ray intensities for nuclides in transient equilibrium. The need and significance of accurate and precise decay data of 137Ceg and 85Yg in basic science and medicine is briefly outlined. |
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| 542 | _ | _ | |i 2020-06-19 |2 Crossref |u https://link.aps.org/licenses/aps-default-license |
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| 700 | 1 | _ | |a Voyles, A. S. |0 0000-0002-1446-416X |b 3 |
| 700 | 1 | _ | |a Nesaraja, C. D. |0 0000-0001-5571-8341 |b 4 |
| 700 | 1 | _ | |a Bernstein, L. A. |0 0000-0002-9589-1752 |b 5 |
| 700 | 1 | _ | |a Browne, E. |0 P:(DE-HGF)0 |b 6 |
| 700 | 1 | _ | |a Martin, M. J. |0 P:(DE-HGF)0 |b 7 |
| 700 | 1 | _ | |a Qaim, S. M. |0 P:(DE-Juel1)131840 |b 8 |e Corresponding author |
| 773 | 1 | 8 | |a 10.1103/physrevc.101.064619 |b American Physical Society (APS) |d 2020-06-19 |n 6 |p 064619 |3 journal-article |2 Crossref |t Physical Review C |v 101 |y 2020 |x 2469-9985 |
| 773 | _ | _ | |a 10.1103/PhysRevC.101.064619 |g Vol. 101, no. 6, p. 064619 |0 PERI:(DE-600)2844098-5 |n 6 |p 064619 |t Physical review / C |v 101 |y 2020 |x 2469-9985 |
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