摘要The energy distribution of the Kerr-NUT (Newman--Unti--Tamburino) spacetime is calculated using Moller's energy--momentum complex within the framework of the Riemannian geometry.
Abstract：The energy distribution of the Kerr-NUT (Newman--Unti--Tamburino) spacetime is calculated using Moller's energy--momentum complex within the framework of the Riemannian geometry.
(Canonical formalism, Lagrangians, and variational principles)
引用本文:
Gamal G. L. Nashed. Moller's Energy of Kerr-NUT Metric[J]. 中国物理快报, 2008, 25(4): 1202-1204.
Gamal G. L. Nashed. Moller's Energy of Kerr-NUT Metric. Chin. Phys. Lett., 2008, 25(4): 1202-1204.
[1]Tolman R C 1930 Phys. Rev. 35 875 [2] Landau L D and Lifshitz E M 1980 The Classical Theoryof Fields (Oxford: Pergamon) [3] Goldberg J N 1958 Phys. Rev. 111 315 [4] Bergmann P G and Thomson R 1953 Phys. Rev. 89401 Bergman P G 1958 Phys. Rev. 112 287 [5] M\o ller C 1958 Ann. Phys. (N.Y.) 4 347 [6] Komar A 1959 Phys. Rev. 113 934 [7] Arnowitt R, Deser S and Misner C W 1961 Phys. Rev. 122 997 [8] Nahmad-Achar E and Schutz B F 1987 Gen. Relat.Grav. 19 7 [9] Bartink R 1989 Phys. Rev. Lett. 62 2346 [10] Katz J and Ori A 1990 Class. Quant. Grav. 7787 [11] M\o ller C 1961 Ann. Phys. (N.Y.) 12 118 [12] Lessner G 1996 Gen. Relat. Grav. 28 527 [13] Bondi H 1990 Proc. R. Soc. London A 427 249 [14] Kovacs D 1985 Gen Relat. Grav. 17 927 [15] Novotny J 1987 Gen. Relat. Grav. 19 1043 [16] Komar A 1959 Phys. Rev. 113 934 [17] Rosen N and Virbhadra K S 1993 Gen. Relat. Grav. 26 429 Virbhadra K S 1990 Phys. Rev. D 41 1086 Virbhadra K S 1990 Phys. Rev. D 42 1066 Virbhadra K S 1999 Phys. Rev. D 60 104041 Virbhadra K S 1990 Phys. Rev. D 42 2919 Virbhadra K S and Parikh J C 1993 Phys. Lett. B 317 312 Virbhadra K S and Parikh J C 1994 Phys. Lett. B 331 302 [18] Aguirregabiria J M, Chamorro A, Virbhadra K S andParikh J C 1996 Gen. Relat. Grav. 28 1393 [19] Xulu S S 2000 Int. J. Mod. Phys. A 15 1979Xulu S S 2000 Mod. Phys. Lett. A 15 1151 [20] Radinschi I 2000 Mod. Phys. Lett. A 15 803 [21] Newman E T, Tamburino L and Unti T 1963 J. Math.Phys. 4 915 [22] Bini D, Cherubini C, Jantzen R T and Mashhoon B 2003 Phys.\ Rev. D 67 084013 [23] Carter B 1968 Commun. Math. Phys. 10 280 [24] Bini D, Cherubini C, Jantzen R T and Ruffini R 2002 Prog. Theor. Phys. 107 1 [25] Bini D, Cherubini C and Jantzen R T 2002 Class.Quant. Grav. 19 1 [26] Nashed G G L 2007 Mod. Phys. Lett. A 22 1047 Nashed G G L 2003 Chaos, Soliton and Fractals 15687 [27] Nashed G G L and Shirafuji T 2007 Int. J. Mod.Phys. D 16 65 Nashed G G L 2006 Mod. Phys. Lett. A 21 2241 [28] Shirafuji T, Nashed G G L and Hayashi K 1996 Prog. Theor. Phys. 95 665 [29] Ahmed M and Hossain S M 1995 Prog. Theor. Phys. 93 901 [30]Penrose R 1982 Proc. R. Soc. London A 381 53
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