Hasil Pencarian - W.P. Lin

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  1. 1
    Constraining the 12C+12C astrophysical S-factors with the 12C+13C measurements at very low energies

    Constraining the 12C+12C astrophysical S-factors with the 12C+13C measurements at very low energies oleh N.T. Zhang, X.Y. Wang, D. Tudor, B. Bucher, I. Burducea, H. Chen, Z.J. Chen, D. Chesneanu, A.I. Chilug, L.R. Gasques, D.G. Ghita, C. Gomoiu, K. Hagino, S. Kubono, Y.J. Li, C.J. Lin, W.P. Lin, R. Margineanu, A. Pantelica, I.C. Stefanescu, M. Straticiuc, X.D. Tang, L. Trache, A.S. Umar, W.Y. Xin, S.W. Xu, Y. Xu

    Diterbitkan 2020-02-01
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  2. 2
    Corrigendum to “Constraining the 12C+12C astrophysical S-factors with the 12C+13C measurements at very low energies” [Phys. Lett. B 801 (2020) 135170]

    Corrigendum to “Constraining the 12C+12C astrophysical S-factors with the 12C+13C measurements at very low energies” [Phys. Lett. B 801 (2020) 135170] oleh N.T. Zhang, X.Y. Wang, D. Tudor, B. Bucher, I. Burducea, H. Chen, Z.J. Chen, D. Chesneanu, A.I. Chilug, L.R. Gasques, D.G. Ghita, C. Gomoiu, K. Hagino, S. Kubono, Y.J. Li, C.J. Lin, W.P. Lin, R. Margineanu, A. Pantelica, I.C. Stefanescu, M. Straticiuc, X.D. Tang, L. Trache, A.S. Umar, W.Y. Xin, S.W. Xu, Y. Xu

    Diterbitkan 2020-04-01
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  3. 3
    Charge radii of 11−16C, 13−17N and 15−18O determined from their charge-changing cross-sections and the mirror-difference charge radii

    Charge radii of 11−16C, 13−17N and 15−18O determined from their charge-changing cross-sections and the mirror-difference charge radii oleh J.W. Zhao, B.-H. Sun, I. Tanihata, J.Y. Xu, K.Y. Zhang, A. Prochazka, L.H. Zhu, S. Terashima, J. Meng, L.C. He, C.Y. Liu, G.S. Li, C.G. Lu, W.J. Lin, W.P. Lin, Z. Liu, P.P. Ren, Z.Y. Sun, F. Wang, J. Wang, M. Wang, S.T. Wang, X.L. Wei, X.D. Xu, J.C. Zhang, M.X. Zhang, X.H. Zhang

    Diterbitkan 2024-11-01
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  4. 4
    Isospin-dependence of the charge-changing cross-section shaped by the charged-particle evaporation process

    Isospin-dependence of the charge-changing cross-section shaped by the charged-particle evaporation process oleh J.W. Zhao, B.-H. Sun, I. Tanihata, S. Terashima, A. Prochazka, J.Y. Xu, L.H. Zhu, J. Meng, J. Su, K.Y. Zhang, L.S. Geng, L.C. He, C.Y. Liu, G.S. Li, C.G. Lu, W.J. Lin, W.P. Lin, Z. Liu, P.P. Ren, Z.Y. Sun, F. Wang, J. Wang, M. Wang, S.T. Wang, X.L. Wei, X.D. Xu, J.C. Zhang, M.X. Zhang, X.H. Zhang

    Diterbitkan 2023-12-01
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  5. 5
    Evidence for prevalent Z = 6 magic number in neutron-rich carbon isotopes

    Evidence for prevalent Z = 6 magic number in neutron-rich carbon isotopes oleh D. T. Tran, H. J. Ong, G. Hagen, T. D. Morris, N. Aoi, T. Suzuki, Y. Kanada-En’yo, L. S. Geng, S. Terashima, I. Tanihata, T. T. Nguyen, Y. Ayyad, P. Y. Chan, M. Fukuda, H. Geissel, M. N. Harakeh, T. Hashimoto, T. H. Hoang, E. Ideguchi, A. Inoue, G. R. Jansen, R. Kanungo, T. Kawabata, L. H. Khiem, W. P. Lin, K. Matsuta, M. Mihara, S. Momota, D. Nagae, N. D. Nguyen, D. Nishimura, T. Otsuka, A. Ozawa, P. P. Ren, H. Sakaguchi, C. Scheidenberger, J. Tanaka, M. Takechi, R. Wada, T. Yamamoto

    Diterbitkan 2018-04-01
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