Experimentally well-constrained masses of 27P and 27S: Implications for studies of explosive binary systems

The mass of 27P is expected to impact the X-ray burst (XRB) model predictions of burst light curves and the composition of the burst ashes, but large uncertainties and inconsistencies still exist in the reported 27P masses. We have used the β-decay spectroscopy of 27S to determine the most precise m...

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Main Authors: L.J. Sun, X.X. Xu, S.Q. Hou, C.J. Lin, J. José, J. Lee, J.J. He, Z.H. Li, J.S. Wang, C.X. Yuan, F. Herwig, J. Keegans, T. Budner, D.X. Wang, H.Y. Wu, P.F. Liang, Y.Y. Yang, Y.H. Lam, P. Ma, F.F. Duan, Z.H. Gao, Q. Hu, Z. Bai, J.B. Ma, J.G. Wang, F.P. Zhong, C.G. Wu, D.W. Luo, Y. Jiang, Y. Liu, D.S. Hou, R. Li, N.R. Ma, W.H. Ma, G.Z. Shi, G.M. Yu, D. Patel, S.Y. Jin, Y.F. Wang, Y.C. Yu, Q.W. Zhou, P. Wang, L.Y. Hu, X. Wang, H.L. Zang, P.J. Li, Q.Q. Zhao, H.M. Jia, L. Yang, P.W. Wen, F. Yang, M. Pan, X.Y. Wang, Z.G. Hu, R.F. Chen, M.L. Liu, W.Q. Yang, Y.M. Zhao
Format: Article
Language:English
Published: Elsevier 2020-03-01
Series:Physics Letters B
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269320300174