Find Flux Through Black Hole: Metric g & Gauge Field A

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Discussion Overview

The discussion revolves around calculating the flux through a sphere surrounding a black hole using a given black hole metric \( g_{\mu\nu} \) and gauge field \( A_\mu \). Participants explore the mathematical framework necessary for integrating forms and finding the total charge associated with the gauge field in a five-dimensional AdS space.

Discussion Character

  • Technical explanation
  • Mathematical reasoning

Main Points Raised

  • One participant inquires about finding the Hodge star \( \star F \) using the black hole metric.
  • Another participant presents a formula for the Hodge star in five-dimensional AdS space and seeks assistance on how to integrate it to find the total charge.
  • A different participant suggests using the covariant derivative of the field tensor to derive the current and mentions integrating the time component over a volume.
  • Another response discusses the process of integrating forms over a manifold, detailing how to pull back the n-form to an n-surface and perform the integral.
  • One participant emphasizes the need to integrate \( *F \) over a closed (d-2)-surface to find the electric charge, suggesting the use of spherical coordinates due to the presumed spherical symmetry in five dimensions.

Areas of Agreement / Disagreement

The discussion contains multiple competing views and approaches regarding the integration of forms and the calculation of flux and charge. No consensus is reached on a single method or solution.

Contextual Notes

Participants express varying assumptions about the dimensionality and symmetry of the space, and the integration steps remain unresolved. The discussion reflects a reliance on specific mathematical definitions and techniques that may not be universally agreed upon.

praharmitra
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Given a black hole metric [itex]g_{\mu\nu}[/itex] and gauge field [itex]A_\mu[/itex], how do I find the flux through a sphere of a black hole.

In simpler terms how do you find [itex]\star F[/itex] (the hodge star, I believe) using the metric ??
 
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Well, I found out that
[tex](\star F)_{\alpha\beta\gamma} = F^{\mu\nu} \sqrt{-g}\epsilon_{\mu\nu\alpha\beta\gamma}[/tex]
(I am in five dimensional AdS space)

How do I integrate this now to find the total charge? Please help
 
In tensor terms, use the covariant derivative of the field tensor to get the current and integrate the time component over a volume.

In this case J = d*F ( 4-form ?) which I presume is integrable.
 
Last edited:
It seems like you're just asking how to integrate forms.

To integrate a n-form K over an n-surface [itex]\Sigma[/itex], first you must find the pullback of K to [itex]\Sigma[/itex]; then you just do an ordinary n-dimensional integral. Suppose [itex]x^a[/itex] are the coordinates on your manifold. Then K can be written

[tex]K = \frac{1}{n!} K_{a_1 \ldots a_n} \; dx^{a_1} \wedge \ldots \wedge dx^{a_n}[/tex]

Now, if [itex]y^b[/itex] are the coordinates of the n-submanifold [itex]\Sigma[/itex], then

[tex]\int_\Sigma K = \underbrace{\idotsint}_n K_{a_1 \ldots a_n} \; \frac{\partial x^{a_1}}{\partial y^1} \ldots \frac{\partial x^{a_n}}{\partial y^n} \; dy^{1} \ldots dy^{n}[/tex]

To find the electric charge that sources some Maxwell field F, you integrate [itex]*F[/itex] over a closed (d-2)-surface that contains the charge. In your case, you are in 5 dimensions, and you probably have spherical symmetry. So use spherical coordinates, and integrate over a 3-sphere centered on the black hole (set R and T to constants).
 

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