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Three-Laboratory Measurement of the 44Ti Half-Life

I. Ahmad, G. Bonino, G. Cini Castagnoli, S. M. Fischer, W. Kutschera, and M. Paul
Phys. Rev. Lett. 80, 2550 – Published 23 March 1998
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Abstract

We report on a measurement of the 44Ti half-life aimed at lowering existing systematic uncertainties in this value, which is important to astrophysics. The half-life was measured by following the decay of 44Ti relative to 60Co for about 5 yr and the measurements were performed independently in three laboratories—Argonne, Jerusalem, and Torino. We suggest to combine our result, 59.0±0.6 yr, with the one from the accompanying Letter by Görres et al., 60.3±1.3 yr, to obtain a current “best value” for the half-life of 44Ti of 59.2±0.6 yr ( 1σ error).

  • Received 21 October 1997

DOI:https://doi.org/10.1103/PhysRevLett.80.2550

©1998 American Physical Society

Authors & Affiliations

I. Ahmad1, G. Bonino2,3, G. Cini Castagnoli2,3, S. M. Fischer1, W. Kutschera1,4, and M. Paul1,5

  • 1Physics Division, Argonne National Laboratory, Argonne, Illinois 60439
  • 2Istituto di Cosmo-Geofisica, Consiglio Nazionale delle Ricerche, Corso Fiume 4, I-10133 Torino, Italy
  • 3and Dipartimento di Fisica Generale dell'Università, Via P. Giuria 1, I-10125 Torino, Italy
  • 4Institut fuer Radiumforschung und Kernphysik der Universitaet Wien, Boltzmanngasse 3, A-1090 Vienna, Austria
  • 5Racah Institute of Physics, Hebrew University, Jerusalem, Israel 91904

See Also

A Supernova Puzzle is Resolved

Phys. Rev. Focus 1, 4 (1998)

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Issue

Vol. 80, Iss. 12 — 23 March 1998

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