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Riemann Extension of Minkowski Line Element in the Rindler Chart Gen. Math. Notes, Vol. 30, No. 1, September 2015, pp.21-27 ISSN 2219-7184; Copyright c ICSRS Publication, 2015 www.i-csrs.org Available free online at http://www.geman.in Riemann Extension of Minkowski Line Element in the Rindler Chart H.G. Nagaraja1 and D. Harish2 1;2Department of Mathematics, Bangalore University Central College Campus, Bengaluru-560001, India 1E-mail: [email protected] 2E-mail: [email protected] (Received: 16-7-15 / Accepted: 29-8-15) Abstract In this paper, we discuss Riemannian extension of Minkowski metric in Rindler coordinates and its geodesics. Keywords: Riemannian curvature, Riemann extension, Flat metric, geodesic equations, constant positive curvature. 1 Introduction Patterson and Walker[7] have defined Riemann extensions and showed how a Riemannian structure can be given to the 2n dimensional tangent bundle of an n− dimensional manifold with given non-Riemannian structure. This shows Riemann extension provides a solution of the general problem of embedding a manifold M carrying a given structure in a manifold M 0 carrying another structure, the embedding being carried out in such a way that the structure on M 0 induces in a natural way the given structure on M. The Riemann ex- tension of Riemannian or non-Riemannian spaces can be constructed with the i help of the Christoffel coefficients Γjk of corresponding Riemann space or with i connection coefficients Πjk in the case of the space of affine connection[5]. The theory of Riemann extensions has been extensively studied by Afifi[1] and Dryuma[2],[3], [4] [5]. 22 H.G. Nagaraja et al. 2 Preliminaries Let (M; g) be a Riemannian manifold and let gij be components of the metric tensor g. The system of geodesic equations are d2xk dxi dxj + Γk = 0; (1) ds2 ij ds ds k where Γij are the Christoffel symbols constructed from g given by 1 Γk = gkm(g + g − g ): (2) ij 2 mi;j mj;i ij;m The geodesic deviation equations or the Jacobi equations are given by D2ηi dxk dxm + Ri ηj = 0; (3) ds2 kjm ds ds i where Rkjm is Riemann curvature tensor of the manifold and Dηi dηi dxk = + Γi ηj : (4) ds ds jk ds Using (1) and simplifying the equation (3) reduces to d2ηi dxm dηl @Γi dxk dxl + 2Γi + kl ηj = 0: (5) ds2 lm ds ds @xj ds ds The Riemann extension[7] of the metric g is given by 2 k l i j k ds = −2Γij(x ) kdx dx + 2d kdx ; (6) where k are the coordinates of additional space. The geodesic equations of (6) consists of two parts, d2xk dxi dxj + Γk = 0 (7) ds2 ij ds ds and δ2 dxj dxi k + Rl = 0; (8) ds2 kji ds ds l where δ2 d dxj k = k − Γl : (9) ds2 ds jk l ds Riemann Extension of Minkowski Line... 23 The system of equations (7) is the system of geodesic equations for geodesics of basic space with local coordinates xi and it does not contain the coordinates k. The system of equations (8) is a n × n linear matrix system of second order in the form d2 d + A(s) + B(s) = 0; (10) ds2 ds where A(s) and B(s) are matrices. 3 Minkowski Metric in Rindler Coordinates In relativistic physics, the Rindler coordinate chart is an important and useful coordinate chart representing part of flat spacetime, also called the Minkowski vacuum. The Rindler coordinate system or frame describes a uniformly acceler- ating frame of reference in Minkowski space. In special relativity, a uniformly accelerating particle undergoes hyperbolic motion. For each such particle a Rindler frame can be chosen in which it is at rest. The Rindler chart is named after Wolfgang Rindler who popularised its use, although it was already well known in 1935[6]. In Rindler chart the Minkowski line element is given by ds2 = dx2 + dy2 + dz2 − a2x2dt2; (11) where x, y and z are space coordinates, t is time coordinate and 'a' is a constant called proper acceleration. The non vanishing Christoffel symbols of the metric (11) are 1 2 4 1 Γ44 = a x; Γ14 = x : (12) The spatial metric of any four dimensional metric 2 α β 0 α 0 0 ds = gαβdx dx + 2g0αdx dx + g00dx dx (13) has the form 2 α β dl = γαβdx dx ; (14) where g0αg0β γαβ = −gαβ + (15) g00 is a three dimensional tensor determining the properties of the space. In the case of the Minkowski metric in Rindler coordinates, − dl2 = dx2 + dy2 + dz2; (16) which is a flat metric. 24 H.G. Nagaraja et al. 3.1 Geodesic Deviation Equations The connection coefficients are clearly very simple. Using the Christoffel sym- bols (12) in equation (5) and simplifying we get a system of Jacobi equations. d2η1 dt dη4 dt 2 + 2a2x + a2 η1 = 0; (17) ds2 ds ds ds d2η2 = 0; (18) ds2 d2η3 = 0; (19) ds2 d2η4 2 dt dη1 1 dx dt + − η1 = 0; (20) ds2 x ds ds x2 ds ds where d2x dt 2 + a2x = 0 (21) ds2 ds and d2t 2 dx dt + = 0: (22) ds2 x ds ds Equations (21) and (22) are the geodesic equations obtained from (1). Simpli- fying and substituting for 't' the system reduces to d2η1 2a2k2 dη4 a2k4 + + η1 = 0 (23) ds2 x ds x4 d2η2 = 0 (24) ds2 d2η3 = 0 (25) ds2 d2η4 2k2 dη1 k2 dx + − η1 = 0 (26) ds2 x3 ds x4 ds d2x k4 + a2 = 0: (27) ds2 x3 Solving we get p p p Z 2 2 4 2 2 5 − 5 1 (ak + a k + c x ) x η = x(c1( p dx) (28) a2k4 + c2x2 p p p Z (ak2 + a2k4 + c2x2)− 5x 5 +c2( p dx)) + c3; a2k4 + c2x2 Riemann Extension of Minkowski Line... 25 2 η = a1s + a2; (29) 3 η = a3s + a4; (30) Z 1 Z 1 p p η4 = p (x(( p (2(ak2 + a2k4 + c2x2)− 5 a2k4 + c2x2 x3 a2k4 + c2x2 p p p p 1+ 5 2 2 4 2 2 5 1− 5 c2x + 2(ak + a k + c x ) c2x 1 p + η1 a2k4 + c2x2dx)k2 + c )))dx + c ; (31) x 4 5 and (32) 1 x2 = [c4(s + d)2 − a2k4]; (33) c2 where a1; a2; a3; a4; c1; c2; c3; c4; c5; d are arbitrary constants. 3.2 Riemann Extension The metric in the extended space is given by 4 ds2 = −2xa2P dt2 − V dxdt + 2dxdP + 2dydQ + 2dzdU + 2dtdV: (34) x The Christoffel symbols in the extended space are 2V 1 2V Γ5 = Γ5 = a2P Γ5 = − Γ8 = 14 x2 44 48 x 11 x2 1 (35) Γ8 = a2P Γ8 = − Γ8 = 2V a2 Γ8 = −a2x: 14 18 x 44 45 The geodesic equations are given by d2x dt 2 + a2x = 0 (36) ds2 ds d2y = 0 (37) ds2 d2z = 0 (38) ds2 26 H.G. Nagaraja et al. d2t 2 dx dt + = 0 (39) ds2 x ds ds d2P 4V dx dt dt 2 2 dt dV + + a2P − = 0 (40) ds2 x2 ds ds ds x ds ds d2Q = 0 (41) ds2 d2U = 0 (42) ds2 d2V 2V dx dx dt 2 dx dV dt 2 + ( )2 + 2a2P − + 2a2V (43) ds2 x2 ds ds ds x ds ds ds dt dP −2a2x = 0: (44) ds ds Solving the above equations, we obtain y = a1s + b1; z = a2s + b2;Q = a3s + b3;U = a4s + b4, c2 c2(s + d) − ak2 1 t = log and x2 = [c4(s + d)2 − a2k4]. 2a c2(s + d) + ak2 c2 Transforming the remaining equations from s to x, we get d2P dP x3(c2x2 + a2k4) − a2k4x2 + a2k4xP dx2 dx (45) p dV = 2k2 a2k4 + c2x2 x − 2V dx and d2V dV x2(c2x2 + a2k4) − (3a2k4x + 2c2x3) + (4a2k4 + 2c2x2)V dx2 dx (46) p dP = 2a2k2x c2x2 + a2k4 x − P : dx Solving (45) and (46) we get, p b (a2k4 + c2x2) + b a2k4 + c2x2 + b P (x) = 1 2 3 (47) x and p Z 4 2 4 2 2 2 4 2 4 2 2 2 4 ! 2 2k a (k b1 + b3) + c x (b1a k + b3) + 2 a k + c x b2a k V (x) = x b4 + p dx ; k2x3 a2k4 + c2x2 (48) Riemann Extension of Minkowski Line... 27 where b1; b2; b3; b4 are constants determined by the given initial conditions. Thus we have obtained Riemann extension of Minkowski metric in Rindler coordinates and have obtained solution of its geodesic equations. Acknowledgements: This work is supported by CSIR:09/039(0106)2012- EMR-I. References [1] Z. Afifi, Riemann extensions of affine connected spaces, Quart. J. Math., Oxford Ser., 2(5) (1954), 312-320. [2] V.S. Dryuma, Toward a theory of spaces of constant curvature, Teoret. Mat. Fiz., 146(1) (2006), 42-54. [3] V.S. Dryuma, On geodesical extension of the Schwarzshild space-time, Proceedings of Institute of Mathematics of NAS of Ukraine, 50(3) (2004), 1294-1300. [4] V.S. Dryuma, On Riemann extension of the Schwarzschild metric, Bul. Acad. S¸tiint¸e Repub. Mold. Mat., 3(2003), 92-103. [5] V.S. Dryuma, Four dimensional Einstein spaces on six dimensional Ricci flat base spaces, arXiv:gr-qc/0601051, January (2006), v1 12.1. [6] A. Einstein and N. Rosen, A particle problem in the general theory of relativity, Physical Review, 48(1935), 73-77. [7] E.M. Patterson and A.G. Walker, Riemann extensions, Quart. J. Math., Oxford Ser., 2(3) (1952), 19-28..
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