• [1]

    Gerasimov S. Yaz. Phys. Rev. Lett., 1965, 2: 598[2] Drell S D, Hearn A C. Phys. Rev. Lett., 1966, 16: 908[3] Fermi E. Phys. Rev., 1940, 57: 458[4] Singh J, Sulkosky V. Radiation Thickness, Collisional Thickness and Most Probable Collisional Energy Loss for E97110: The GDH Sum Rule, the Spin Structure of 3He and the Neutron using Nearly Real Photons, JLab Hall-A Technique Note, 2007[5] Bethe H, Heitler W. Containing Papers of a Mathematical and Physical Character, 1934, 146(856): 83--112[6] Wheeler J A, Lamb W E. Phys. Rev., 1939, 55(9): 858--862[7] Wheeler J A, Lamb W E. Phys. Rev., 1956, 101(6): 1836[8] Bethe H A, Askin J. Experimental Nuclear Physics, 1953, 1: 166--357[9] Tsai Y S. Rev. Mod. Phys., 1974, 46(4): 815--851[10] Tsai Y S. Rev. Mod. Phys., 1977, 49(2): 421--423[11] Particle Data Group. Physics Letters B, 2004, 592: 1--1109[12] Davies H, Bethe H A, Maximon L C. Phys. Rev., 1954, 93(4): 788--795[13] Willliam R L. A. How-to Approach. Berlin: Springer-Verlag, Second revised edition, 1994[14] Enrico Fermi. Phys. Rev., 1940, 57(6): 485--493[15] Maccabee H D, Papworth D G. Physics Letters A, 1969, 30: 241--242[16] Sternheimer R M, Berger M J, Seltzer S M. Atomic Data and Nuclear Data Tables, 1984, 30(2): 261--271[17] Sternheimer R M, Peierls R F. Phys. Rev. B, 1971, 3(11): 3681--3692[18] Seltzer S M, Berger M J. Int. J. Appl. Radiat. Isot., 1982, 33: 1189--1218