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Nuclear Mass Measurements Map the Structure of Atomic Nuclei and Accreting Neutron Stars
Z. Meisel, S. George, S. Ahn +28
We present mass excesses (ME) of neutron-rich isotopes of Ar through Fe, obtained via TOF- mass spectrometry at the National Superconducting Cyclotron Laboratory. Our new resul…
Testing claims of the GW170817 binary neutron star inspiral affecting -decay rates
P. A. Breur, J. C. P. Y. Nobelen, L. Baudis +11
On August 17, 2017, the first gravitational wave signal from a binary neutron star inspiral (GW170817) was detected by Advanced LIGO and Advanced VIRGO. Here we present radioactive…
A Precision Experiment to Investigate Long-Lived Radioactive Decays
J. R. Angevaare, P. Barrow, L. Baudis +18
Radioactivity is understood to be described by a Poisson process, yet some measurements of nuclear decays appear to exhibit unexpected variations. Generally, the isotopes reporting…
Time-of-flight mass measurements of neutron-rich chromium isotopes up to N = 40 and implications for the accreted neutron star crust
Z. Meisel, S. George, S. Ahn +29
We present the mass excesses of 59-64Cr, obtained from recent time-of-flight nuclear mass measurements at the National Superconducting Cyclotron Laboratory at Michigan State Univer…
Mass measurement of 56Sc reveals a small A=56 odd-even mass staggering, implying a cooler accreted neutron star crust
Z. Meisel, S. George, S. Ahn +29
We present the mass excesses of 52-57Sc, obtained from recent time-of-flight nuclear mass measurements at the National Superconducting Cyclotron Laboratory at Michigan State Univer…
Mass Measurements Demonstrate a Strong N =28 Shell Gap in Argon
Z. Meisel, S. George, S. Ahn +28
We present results from recent time-of-flight nuclear mass measurements at the National Superconducting Cyclotron Laboratory at Michigan State University. We report the first mass…