Energy of the 2.3-MeV γ ray from the first excited state of 14N

P. H. Barker
Phys. Rev. C 63, 024302 – Published 5 January 2001
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Abstract

Using an unusual technique for precisely locating γ ray peaks in a spectrum from a Ge semiconductor detector, the energy of the 2.31-MeV γ ray which follows 14O positron decay has been measured on a scale derived from the known energies of 56Co lines, as have the energies of the 2.18- and 2.32-MeV γ rays which follow the decay of 90Nb. Values of 2312.603(10), 2186.253(10), and 2318.973(10) keV, respectively, were determined. When taken together with updated, previously accepted values, these lead to recommended energies of 2312.590(10), 2186.244(7), and 2318.962(6) keV.

  • Received 2 August 2000

DOI:https://doi.org/10.1103/PhysRevC.63.024302

©2001 American Physical Society

Authors & Affiliations

P. H. Barker

  • Physics Department, University of Auckland, Private Bag 92019, Auckland, New Zealand

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Vol. 63, Iss. 2 — February 2001

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