Mass Measurement of Sc 56 Reveals a Small A = 56 Odd-Even Mass Staggering, Implying a Cooler Accreted Neutron Star Crust

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Veröffentlicht in:Physical review letters 2015-10, Vol.115 (16), Article 162501
Hauptverfasser: Meisel, Z., George, S., Ahn, S., Bazin, D., Brown, B. A., Browne, J., Carpino, J. F., Chung, H., Cole, A. L., Cyburt, R. H., Estradé, A., Famiano, M., Gade, A., Langer, C., Matoš, M., Mittig, W., Montes, F., Morrissey, D. J., Pereira, J., Schatz, H., Schatz, J., Scott, M., Shapira, D., Smith, K., Stevens, J., Tan, W., Tarasov, O., Towers, S., Wimmer, K., Winkelbauer, J. R., Yurkon, J., Zegers, R. G. T.
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container_issue 16
container_start_page
container_title Physical review letters
container_volume 115
creator Meisel, Z.
George, S.
Ahn, S.
Bazin, D.
Brown, B. A.
Browne, J.
Carpino, J. F.
Chung, H.
Cole, A. L.
Cyburt, R. H.
Estradé, A.
Famiano, M.
Gade, A.
Langer, C.
Matoš, M.
Mittig, W.
Montes, F.
Morrissey, D. J.
Pereira, J.
Schatz, H.
Schatz, J.
Scott, M.
Shapira, D.
Smith, K.
Stevens, J.
Tan, W.
Tarasov, O.
Towers, S.
Wimmer, K.
Winkelbauer, J. R.
Yurkon, J.
Zegers, R. G. T.
description
doi_str_mv 10.1103/PhysRevLett.115.162501
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title Mass Measurement of Sc 56 Reveals a Small A = 56 Odd-Even Mass Staggering, Implying a Cooler Accreted Neutron Star Crust
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