Magnetic dipole excitations of 50 Cr
Magnetic dipole excitations of 50 Cr
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DOI:
10.1103/physrevc.93.014318
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发表时间:
2016-01
影响因子:
3.1
通讯作者:
H. Pai;T. Beck;J. Beller;R. Beyer;M. Bhike;V. Derya;U. Gayer;J. Isaak;Krishichayan;J. Kvasil;B. Löher;V. Nesterenko;N. Pietralla;G. Martínez-Pinedo;L. Mertes;V. Ponomarev;P. Reinhard;A. Repko;P. Ries;C. Romig;D. Savran;R. Schwengner;W. Tornow;V. Werner;J. Wilhelmy;A. Zilges;M. Zweidinger
中科院分区:
文献类型:
--
作者:
H. Pai;T. Beck;J. Beller;R. Beyer;M. Bhike;V. Derya;U. Gayer;J. Isaak;Krishichayan;J. Kvasil;B. Löher;V. Nesterenko;N. Pietralla;G. Martínez-Pinedo;L. Mertes;V. Ponomarev;P. Reinhard;A. Repko;P. Ries;C. Romig;D. Savran;R. Schwengner;W. Tornow;V. Werner;J. Wilhelmy;A. Zilges;M. Zweidinger
The low-lying $M1$-strength of the open-shell nucleus $^{50}$Cr has been studied with the method of nuclear resonance fluorescence up to 9.7 MeV, using bremsstrahlung at the superconducting Darmstadt linear electron accelerator S-DALINAC and Compton backscattered photons at the High Intensity $\gamma$-ray Source (HI$\gamma$S) facility between 6 and 9.7 MeV of the initial photon energy. Fifteen $1^{+}$ states have been observed between 3.6 and 9.7 MeV. Following our analysis, the lowest $1^{+}$ state at 3.6 MeV can be considered as an isovector orbital mode with some spin admixture. The obtained results generally match the estimations and trends typical for the scissors-like mode. Detailed calculations within the Skyrme Quasiparticle Random-Phase-Approximation method and the Large-Scale Shell Model justify our conclusions. The calculated distributions of the orbital current for the lowest $1^{+}$-state suggest the schematic view of Lipparini and Stringari (isovector rotation-like oscillations inside the rigid surface) rather than the scissors-like picture of Lo Iudice and Palumbo. The spin M1 resonance is shown to be mainly generated by spin-flip transitions between the orbitals of the $fp$-shell.