Excercise Sheet 4 to General Relativity

Excercise Sheet 4 to General Relativity

Excercise Sheet 4 to General Relativity Prof. G¨unter Sigl II. Institut f¨urTheoretische Physik der Universit¨atHamburg Luruper Chaussee 149 D-22761 Hamburg Germany email: [email protected] tel: 040-8998-2224 Discussion on 16.11.2012 in the exercise classes 1. Maxwell's Equations in Terms of Differential Forms (a) Show that the homogeneous Maxwell equations @ρFµν + @µFνρ + @νFρµ = 0 can be written as @[µFνσ] = 0 ; or simply as dF = 0 in terms of the field strength tensor two form Fµν. (b) Show that the inhomogeneous Maxwell equations µν ν @µF = j ; ν with j = (ρe; j) the electric current density four-vector, can be written as d(∗F ) = ∗J; with the definition of the Hodge star operator given in the lectures and the current density ρ one-form Jν ≡ ηνρj . Hints: Show in a first step that 3 ν1ν2 [d(∗F )] = @[µ Fν ν ; µ1µ2µ3 2 1 µ2µ3] 1 2 and figure out over which values the indices ν1 and ν2 run for given mutually different indices µ1; µ2; µ3. Finally, express the result in terms of the unique index ν 6= (µ1; µ2; µ3) and keep track of all the numerical pre-factors. please turn over 1 2. Cross Product and Hodge Dual in 3 Dimensions Show that the cross product A × B of two vectors A and B in three-dimensional Euclidean i space can be understood as the Hodge product of the two corresponding one-forms Aidx and i Bidx , where Ai and Bi are the Euclidean components of A and B, respectively. 3. The Divergence of Vector Fields (a) Show that the Christoffel symbols satisfy µ 1 q Γµλ = q @λ jgj ; (1) jgj where g = det gµν. Hint: First show that for an infinitesimal variation δM of an invertible n × n matrix M one has δ ln det M = Tr M −1δM : (2) (b) Using this result show that the divergence of a vector field V µ can be written as µ 1 q µ rµV = q @µ jgjV ; (3) jgj 4. Paraboloidal Coordinates In Euclidean three-space, paraboloidal coordinates (u; v; φ) are defined by 1 x = uv cos φ ; y = uv sin φ ; z = u2 − v2 : (4) 2 µν (a) Calculate the metric gµν and the inverse metric g in paraboloidal coordinates. (b) Calculate the Christoffel symbols for the paraboloidal coordinates. 2.

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