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2021 IPS Conference
Study Materials
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Home
About/Contact
Newsletters
Events/Seminars
2021 IPS Conference
Study Materials
Corporate Members
The masses of exotic nuclei provide key information for the understanding of nuclear structure and astrophysics. At the FRS (FRagment Separator) at GSI Helmholtz Centre for Heavy Ion Research, exotic nuclei are produced at relativistic energies by projectile fragmentation or fission and separated in-flight. At the FRS Ion Catcher experiment the nuclei are thermalized and stopped in a Cryogenic Stopping Cell and are transported via a radio-frequency quadrupole (RFQ) beamline to a Multiple-Reflection Time-of-Flight Mass Spectrometer (MR-TOF-MS) for high-precision direct mass measurements. The MR-TOF-MS has single-ion sensitivity and features resolving powers at full width at half maximum of up to one million. Consequently, the system enables us to handle very low yields and perform mass measurements with relative mass accuracies down to 1.7 · 10−8 [1], reaching the level of Penning traps.
The average interaction strength between the last (highest energy orbitals) proton(s) and neutron(s) in a nucleus (denoted as δVpn), may be derived from differences of accurate atomic masses, and in turn point empirically to various aspects of nuclear structure and interactions. This has been investigated especially in nuclei with N=Z [2] and neutron-rich nuclei with equal proton and neutron numbers above doubly-magic cores [3].
Confirmed by mass measurements at the FRS Ion Catcher, the detailed structure of δVpn along the N=Z, Z+2 and Z+4 lines has been investigated recently [1]. In addition, a systematic search for deviations from the expected δVpn trends throughout the nuclear chart, may indicate that the mass values in the Atomic Mass Evaluation [4] are not correct or even some mass measurements are questionable. These results and planned investigations will be discussed.
[1] I. Mardor et al., Phys. Rev. C 103, 034319 (2021)
[2] P. Van Isacker et al., Phys. Rev. Lett. 74, 4607 (1995)
[3] R. B. Calkirli et al., Phys. Rev. C82, 061304(R) (2010)
[4] M. Wang et al., Chinese Phys. C 45, 030003 (2021)