skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Half-life of {sup 44}Ti

Technical Report ·
DOI:https://doi.org/10.2172/166365· OSTI ID:166365
; ;  [1];  [2]
  1. Instituto di Cosmogeofisica, Torino (Italy)
  2. Hebrew Univ., Jerusalem (Israel)

The measurement of the {sup 44}Ti half-life, started 3 years ago, is still continuing. The goal of this measurement is to determine the half-life of {sup 44}Ti, which is {approximately}52 y, to a precision of {approximately}5%. An accurate value of this half-life is of interest to cosmologists who need it to determine the production of heavy elements in supernova. Three sets of samples - a pure 200-nCi {sup 44}Ti sample, a pure 300-nCi {sup 60}Co source, and a mixed {sup 44}Ti-{sup 60}Co source of similar strength - were prepared and their spectra are being measured with Ge spectrometers at Argonne, Torino and Jerusalem. Each sample is counted for a period of 2 days, at approximate intervals of 4 months. The room background is also measured for the same length of time. We hope to start data analysis at the end of summer and obtain a value for the {sup 44}Ti half-life.

Research Organization:
Argonne National Lab. (ANL), Argonne, IL (United States)
OSTI ID:
166365
Report Number(s):
ANL-95/14; ON: DE96000985; TRN: 95:007970-0078
Resource Relation:
Other Information: PBD: Aug 1995; Related Information: Is Part Of Physics Division Annual Report, April 1, 1994--March 31, 1995; Henning, W.F.; PB: 207 p.
Country of Publication:
United States
Language:
English

Similar Records

Three-Laboratory Measurement of the {sup 44}Ti Half-Life
Journal Article · Sun Mar 01 00:00:00 EST 1998 · Physical Review Letters · OSTI ID:166365

Measurement of the {sup 44}Ti half-life and its significance for supernova.
Conference · Sat Aug 28 00:00:00 EDT 1999 · OSTI ID:166365

Improved measurement of the {sup 44}Ti half-life from a 14-year long study
Journal Article · Fri Dec 15 00:00:00 EST 2006 · Physical Review. C, Nuclear Physics · OSTI ID:166365