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SMuK 2023 – wissenschaftliches Programm

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HK: Fachverband Physik der Hadronen und Kerne

HK 70: Structure and Dynamics of Nuclei XV

HK 70.3: Vortrag

Donnerstag, 23. März 2023, 16:30–16:45, SCH/A215

The isovector spin-M1 response of 90Zr and 92Mo — •A. Gupta1, V. Werner1, K.E. Ide1, A.D. Ayangeakaa2, 3, M. Beuschlein1, S.W. Finch3,4, U. Friman-Gayer3,4,5, D. Gribble2, 3, J. Hauf1, J. Isaak1, X. James2, 3, R.V.F. Janssens2, 3, S.R. Johnson2, 3, J. Kleemann1, P. Koseoglou1, T. Kowalewski2, 3, B. Löher6, O. Papst1, N. Pietralla1, A. Saracino2, 3, and D. Savran61IKP, TU Darmstadt — 2UNC, Chapel Hill, NC, USA — 3TUNL, Durham, NC, USA — 4Duke U., Durham, NC, USA — 5ESS, Lund, SE — 6GSI, Darmstadt

For the N=50 isotones 90Zr and 92Mo, additional isovector spin-flip M1 (IVSM1) strength is expected for 92Mo in comparison to 90Zr because of the two additional protons in the proton g9/2 orbital above the closed pf shell. In addition, the IVSM1 resonance is closely related to Gamow-Teller strengths and can serve to constrain the calculation of electron-capture rates in core-collapse supernova scenarios[1]. Using the newly available hybrid array of HPGe Clover and LaBr3 detectors at the High Intensity γ-ray source (HIγS), we probed the dipole response of both isotopes in an integral-spectroscopy approach below neutron separation thresholds.The E1 and M1 strengths will be determined up to about 9 MeV by measuring the asymmetries resulting from the excitation of the target nuclei by the fully-polarized γ-ray beam. The experimental method and first results will be discussed.

Supported by DFG Project No.279384907-SFB 1245 and the U.S. DOE Grant No. DE-FG02-97ER41041 and No. DE-FG02-97ER41033.

[1] K. Langanke et al., Rep. Prog. Phys. 84, 066301 (2021)

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