General relativity, integration over a manifold exercise

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SUMMARY

The discussion centers on problem 2.9 from Sean Carroll's "Geometry and Spacetime," focusing on evaluating the Hodge dual of a two-form in Minkowski space. The user, Matt, successfully derived the expression for the current density *J and the two-form F, using a TI-89 calculator for assistance. He calculated the electric field components as E_r = -q/(r^4 sin(θ)), E_θ = 0, and E_φ = 0, while noting that the magnetic field B_μ = 0. Matt seeks clarification on integrating the three-form d*F over a volume V, specifically how to convert it into a standard volume integral.

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  • Understanding of Hodge duals and exterior derivatives in differential geometry.
  • Familiarity with two-forms and their representation in matrix form.
  • Knowledge of electric and magnetic field components in the context of electromagnetism.
  • Basic skills in multivariable calculus for evaluating integrals.
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  • Learn how to compute Hodge duals in various coordinate systems.
  • Study the properties of two-forms and their applications in physics.
  • Explore techniques for integrating differential forms over manifolds.
  • Review the relationship between differential forms and classical electromagnetism.
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Students and enthusiasts of general relativity, particularly those tackling differential forms and their applications in physics, as well as anyone looking to deepen their understanding of electromagnetism in a geometric context.

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Homework Statement



The problem I am facing is 2.9 in Sean Carroll's book on general relativity (Geometry and Spacetime) I should note that I am not studying this formally and so a full solution would not be unwelcome, though I understand that forum policy understandably prohibits it. The full problem is stated as

In Minkowski space, suppose that [tex]*F = q \sin{\theta} d\theta\wedge d\phi[/tex].

a.) Evaluate [tex]d*F=*J[/tex]
b.) What is the two-form [tex]F[/tex] equal to?
c.) What are the electric and magnetic fields equal to for this solution?
d.) Evaluate [tex]\int_V d*F[/tex], where [tex]V[/tex] is a ball of radius [tex]R[/tex] in Euclidean three-space at a fixed moment of time.

Homework Equations



In the above the asterisk denotes the Hodge dual and the [tex]d[/tex] denotes the exterior derivative. The definitions of these operators should be well known.

The Attempt at a Solution



I think I have the first three parts solved. For each part a.) I arrived at the lengthy result of

[tex] \frac{1}{2}[\partial_\mu(*F)_{\mu\rho} - \partial_\nu(*F)_{\mu\rho} + \partial_\nu(*F)_{\rho\mu} - \partial_\rho(*F)_{\nu\rmu} + \partial_\rho(*F)_{\mu\nu} - \partial_\mu(*F)_{\rho\nu} = \epsilon^\sigma_{\mu\nu\rho}J_\sigma[/tex]

For part b.) I got (with the help of my TI-89) the two-form, in matrix form,

[tex] F = -(**F) = \left[<br /> \begin{array}{cccc}<br /> 0 & \frac{q}{r^4 \sin{\theta}} & 0 & 0\\<br /> \frac{-q}{r^4 \sin{\theta}} & 0 & 0 &0\\<br /> 0 & 0 & 0 & 0\\<br /> 0 & 0 & 0 & 0<br /> \end{array}<br /> \right][/tex]

and for c.) I arrived at, directly from part b.),

[tex]E_r = \frac{-q}{r^4 \sin{\theta}}[/tex]
[tex]E_\theta = 0[/tex]
[tex]E_\phi = 0[/tex]

[tex]B_\mu = 0[/tex]

For [tex]\mu=1,2,3[/tex].

Verification of these would be appreciated but I am especially confused about the last part d.). In particular the integrand is a three-form and I have no idea how to integrate this and how to transform the integral into a familiar volume integral that can be computed by standard multivariable calculus.
 
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This needs to be moved to the Special and General Relativity forum.

Perhaps there is will get some attention.

Thanks
Matt
 
Thanks, I will try my luck over there.
 

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