corner
corner

Phys. Rev. C 57, 2010–2016 (1998)

Half-life of 44Ti

Download: PDF (125 kB) Buy this article Export: BibTeX or EndNote (RIS)

E. B. Norman1, E. Browne1, Y. D. Chan1, I. D. Goldman2, R.-M. Larimer1, K. T. Lesko1, M. Nelson1, F. E. Wietfeldt1,3, and I. Zlimen1
1Nuclear Science Division, Lawrence Berkeley National Laboratory, Berkeley, California 94720
2Instituto de Fisica, Universidade de Sao Paulo, Sao Paulo, Brazil
3National Institute of Standards and Technology, Gaithersburg, Maryland 20899

Received 20 October 1997; published in the issue dated April 1998

We present the results of two separate measurements of the half-life of 44Ti relative to those of 22Na and 207Bi, respectively. By comparing the numbers of 1157-keV γ rays from 44Ti to those of 1274-keV γ rays from 22Na observed from a mixed source over a period of approximately 2 yr, we determined the half-life of 44Ti to be 61.5±1.0yr. From an approximately 1-yr-long study of another mixed source, where we compared the numbers of 1157-keV γ rays from 44Ti to those of 1064-keV γ rays from 207Bi, we determined the 44Ti half-life to be 62±5yr. From these two results, we have obtained a best value of 62±2yr for the half-life of 44Ti. The astrophysical implications of this result are discussed.

© 1998 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevC.57.2010
DOI:
10.1103/PhysRevC.57.2010
PACS:
21.10.Tg, 98.70.Rz, 27.40.+z, 23.40.-s