On the half-life of {sup 44}Ti
Description:
One of the few long-lived gamma-ray emitting radioisotopes expected to be produced in substantial quantities during a supernova explosion is {sup 44}Ti. The relevant portions of the decay schemes of {sup 44}Ti and its daughter {sup 44}Sc are shown. {sup 44}Ti decays to {sup 44}Sc emitting {gamma} rays of 68 and 78 keV. {sup 44}Sc subsequently decays with a 3.93-hour half life to {sup 44}Ca emitting an 1,157-keV {gamma}ray. This characteristic 1,157-keV {gamma} ray from the decay of {sup 44}Ti h…
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Date:
June 19, 1996
Creator:
Norman, E.B.; Browne, E.; Chan, Y.D.; Goldman, I.D.; Larimer, R.M.; Lesko, K.T. et al.
Item Type:
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Report
Partner:
UNT Libraries Government Documents Department