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Proton removal from $^{73,75}$Br to $^{72,74}$Se at intermediate energies

Authors :
Spieker, M.
Bazin, D.
Biswas, S.
Cottle, P. D.
Farris, P. J.
Gade, A.
Ginter, T.
Giraud, S.
Kemper, K. W.
Li, J.
Noji, S.
Pereira, J.
Riley, L. A.
Smith, M. K.
Weisshaar, D.
Zegers, R. G. T.
Source :
Phys. Rev. C 109, 014307 (2024)
Publication Year :
2024

Abstract

We report new experimental data for excited states of $^{72,74}$Se obtained from proton removal from $^{73,75}$Br secondary beams on a proton target. The experiments were performed with the Ursinus-NSCL Liquid Hydrogen Target and the combined GRETINA+S800 setup at the Coupled Cyclotron Facility of the National Superconducting Cyclotron Laboratory at Michigan State University. Within uncertainties, the inclusive cross sections for proton removal from $^{73,75}$Br on a proton target are identical suggesting that the same single-particle orbitals contribute to the proton-removal reaction. In addition, details of the partial cross section fragmentation are discussed. The data might suggest that $l = 1, 2, 3$, and 4 angular momentum transfers are important to understand the population of excited states of $^{72,74}$Se in proton removal. Available data for excited states of $^{74}$Ge populated through the $^{75}$As$(d,{}^{3}{\mathrm{He}}){}^{74}$Ge proton-removal reaction in normal kinematics suggest indeed that the $fp$ and $sd$ shell as well as the $1g_{9/2}$ orbital contribute. A comparison to data available for odd-$A$ nuclei supports that the bulk of the spectroscopic strengths could be found at lower energies in the even-even Se isotopes than in, for instance, the even-even Ge isotopes. In addition, the population of high-$J$ states seems to indicate that multi-step processes contribute to proton-removal reactions at intermediate energies in these collective nuclei.<br />Comment: 9 pages, 5 figures

Subjects

Subjects :
Nuclear Experiment
Nuclear Theory

Details

Database :
arXiv
Journal :
Phys. Rev. C 109, 014307 (2024)
Publication Type :
Report
Accession number :
edsarx.2411.09835
Document Type :
Working Paper
Full Text :
https://doi.org/10.1103/PhysRevC.109.014307