Decay Partial Half-Life ofand Cosmic Ray Chronometry
- 9 March 1998
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review Letters
- Vol. 80 (10) , 2085-2088
- https://doi.org/10.1103/physrevlett.80.2085
Abstract
The weak decay of the astrophysically significant radioisotope has been observed. The energies of positrons from a chemically purified source were measured using the APEX spectrometer at Argonne National Laboratory. We deduce a decay branch of , corresponding to a partial half-life of . The implications of this value for cosmic-ray confinement times are discussed in light of recent satellite measurements of the cosmic-ray abundance of .
Keywords
This publication has 15 references indexed in Scilit:
- Galactic Cosmic‐Ray Manganese:UlyssesHigh Energy Telescope ResultsThe Astrophysical Journal, 1997
- A solenoidal spectrometer for positron-electron pairs produced in heavy-ion collisionsNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 1996
- Trigger processor for the APEX positron-electron spectrometerNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 1995
- Effective interactions for A = 41–66 nucleiNuclear Physics A, 1994
- Proton Inelastic Scattering onin Inverse KinematicsPhysical Review Letters, 1994
- Search for thedecay ofPhysical Review C, 1993
- The Mn-54 clock and its implications for cosmic-ray propagation and Fe isotope studiesThe Astrophysical Journal, 1991
- New effective interactions for the 0f1p shellNuclear Physics A, 1991
- β+decay and cosmic-ray half-life ofMn54Physical Review C, 1989
- MANGANESE-54 and the Lifetime of Relativistic Cosmic RaysThe Astrophysical Journal, 1973