Low-energy structure of 61Mn populated following $β$ decay of 61Cr

Simple item page
dc.creatorCrawford, H. L.
dc.creatorMantica, P. F.
dc.creatorBerryman, J. S.
dc.creatorBroda, R.
dc.creatorFornal, B.
dc.creatorHoffman, C. R.
dc.creatorHoteling, N.
dc.creatorJanssens, R. V. F.
dc.creatorLenzi, S. M.
dc.creatorPereira, J.
dc.creatorStoker, J. B.
dc.creatorTabor, S. L.
dc.creatorWalters, W. B.
dc.creatorWang, X.
dc.creatorZhu, S.
dc.date2009-04-29
dc.date.accessioned2026-07-07T13:10:05Z
dc.date.available2026-07-07T13:10:05Z
dc.description$β$ decay of the $^{61}$Cr$_{37}$ ground state has been studied. A new half-life of 233 +/- 11 ms has been deduced, and seven delayed $γ$ rays have been assigned to the daughter, $^{61}$Mn$_{36}$. The low-energy level structure of $^{61}$Mn$_{36}$ is similar to that of the less neutron-rich $^{57,59}$Mn nuclei. The odd-A $_{25}$Mn isotopes follow the systematic trend in the yrast states of the even-even, Z + 1 $_{26}$Fe isotopes, and not that of the Z - 1 $_{24}$Cr isotopes, where a possible onset of collectivity has been suggested to occur already at N = 36.
dc.description19 pages, 7 figures, accepted to Physical Review C
dc.identifierhttps://arxiv.org/abs/0904.4710
dc.identifierhttp://arxiv.org/abs/0904.4710
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/228947
dc.subjectNuclear Experiment
dc.titleLow-energy structure of 61Mn populated following $β$ decay of 61Cr
dc.typetext

Files

Collections

arXiv