NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Neutron emission following muon capture in Ce-142, Ce-140, Ba-138, and Sn-120.Branching ratios to excited nuclear states formed after muon capture have been measured with Ge(Li) detectors. The delayed gamma rays were observed in studies of muonic Ce-142, Ce-140, Ba-138, and Sn-120, using separated isotopes. The resulting isotopes formed indicate at least a 60% probability of neutron emission upon muon capture, with the most likely product resulting from single-neutron emission. No evidence for delayed proton emission with a probability higher than 2% was found. Using our more precise energies for the observed nuclear transitions, we present revised energy levels schemes for La-141, La-139, Cs-137, and In-119.
Document ID
19730043848
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Lucas, G. R., Jr.
Martin, P.
Welsh, R. E.
(College of William and Mary Williamsburg, Va., United States)
Jenkins, D. A.
Powers, R. J.
(Virginia Polytechnic Institute and State University Blacksburg, Va., United States)
Kunselman, A. R.
(Wyoming, University Laramie, Wyo., United States)
Miller, G. H.
Date Acquired
August 7, 2013
Publication Date
April 1, 1973
Publication Information
Publication: Physical Review C - Nuclear Physics
Subject Category
Physics, Atomic, Molecular, And Nuclear
Accession Number
73A28650
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available