High-precision mass measurements for the isobaric multiplet mass equation at A = 52
nucl-ex
/ Authors
D. A. Nesterenko, A. Kankainen, L. Canete, M. Block, D. Cox, T. Eronen, C. Fahlander, U. Forsberg, J. Gerl, P. Golubev
and 14 more authors
J. Hakala, A. Jokinen, V. S. Kolhinen, J. Koponen, N. Lalović, Ch. Lorenz, I. D. Moore, P. Papadakis, J. Reinikainen, S. Rinta-Antila, D. Rudolph, L. G. Sarmiento, A. Voss, J. Äystö
/ Abstract
Masses of $^{52}$Co, $^{52}$Co$^m$, $^{52}$Fe, $^{52}$Fe$^m$, and $^{52}$Mn have been measured with the JYFLTRAP double Penning trap mass spectrometer. Of these, $^{52}$Co and $^{52}$Co$^m$ have been experimentally determined for the first time and found to be more bound than predicted by extrapolations. The isobaric multiplet mass equation for the $T=2$ quintet at $A=52$ has been studied employing the new mass values. No significant breakdown (beyond the $3σ$ level) of the quadratic form of the IMME was observed ($χ^2/n=2.4$). The cubic coefficient was 6.0(32) keV ($χ^2/n=1.1$). The excitation energies for the isomer and the $T=2$ isobaric analogue state in $^{52}$Co have been determined to be 374(13) keV and 2922(13) keV, respectively. The $Q$ value for the proton decay from the $19/2^-$ isomer in $^{53}$Co has been determined with an unprecedented precision, $Q_{p} = 1558.8(17)$ keV. The proton separation energies of $^{52}$Co and $^{53}$Ni relevant for the astrophysical rapid proton capture process have been experimentally determined for the first time. \end{abstract}