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- W1993758192 abstract "Modeling the composition of neutron-star crusts depends strongly on binding energies of neutron-rich nuclides near the N = 50 and N = 82 shell closures. Using a recent development of time-of-flight mass spectrometry for on-line purification of radioactive ion beams to access more exotic species, we have determined for the first time the mass of (82)Zn with the ISOLTRAP setup at the ISOLDE-CERN facility. With a robust neutron-star model based on nuclear energy-density-functional theory, we solve the general relativistic Tolman-Oppenheimer-Volkoff equations and calculate the neutron-star crust composition based on the new experimental mass. The composition profile is not only altered but now constrained by experimental data deeper into the crust than before." @default.
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- W1993758192 date "2013-01-22" @default.
- W1993758192 modified "2023-09-30" @default.
- W1993758192 title "Plumbing Neutron Stars to New Depths with the Binding Energy of the Exotic Nuclide<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:mmultiscripts><mml:mi>Zn</mml:mi><mml:mprescripts /><mml:none /><mml:mn>82</mml:mn></mml:mmultiscripts></mml:math>" @default.
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- W1993758192 doi "https://doi.org/10.1103/physrevlett.110.041101" @default.
- W1993758192 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/25166148" @default.
- W1993758192 hasPublicationYear "2013" @default.
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