Time-of-flight mass measurements for nuclear processes in neutron star crusts

Becerri, A.; Portillo, M.; Estrade, A.; Galaviz, D.; Stolz, A.; Schatz, H.; Lau, R.; Wallace, M.; Rogers, A. M.; Brown, E. F.; Gupta, S. S.; Hix, W. R.; Amthor, A.M.; Pereira, J.; Elliot, T.; Bazin, D.; George, S.; Gade, A.; Cyburt, R.; Shapira, D.; Lorusso, G.; Smith, E.; Beard, M.; Wiescher, M.; Matos, M.; Moller, P.

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Time-of-flight mass measurements for nuclear processes in neutron star crusts

Estrade, A.; Matos, M.; Schatz, H.; Amthor, A.M.; Bazin, D.; Beard, M.; Becerri, A.; Brown, E. F.; Cyburt, R.; Elliot, T.; Gade, A.; Galaviz, D.; George, S.; Gupta, S. S.; Hix, W. R.; Lau, R.; Lorusso, G.; Moller, P.; Pereira, J.; Portillo, M.; Rogers, A. M.; Shapira, D.; Smith, E.; Stolz, A.; Wallace, M.; Wiescher, M.

URI: http://localhost:8080/xmlui/handle/123456789/648

Date: 2016-11-28

Abstract:

We present results from time-of-flight nuclear mass measurements at the National Superconducting Cyclotron Laboratory that are relevant for neutron star crust models. The masses of 16 neutron-rich nuclei in the scandium–nickel range were determined simultaneously, with the masses of 61V, 63Cr, 66Mn, and 74Ni measured for the first time with mass excesses of 30:510ð890Þ MeV, 35:280ð650Þ MeV, 36:900ð790Þ MeV, and 49:210ð990Þ MeV, respectively. With these results the locations of the dominant electron capture heat sources in the outer crust of accreting neutron stars that exhibit super bursts are now experimentally constrained. We find the experimental Q value for the 66Fe ! 66Mn electron capture to be 2.1 MeV (2:6 ) smaller than predicted, resulting in the transition occurring significantly closer to the neutron star surface.

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