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

In summary, to find the flux through a sphere of a black hole, you can use the Hodge star operation and the black hole metric and gauge field to calculate the 3-form *F. Then, you can integrate this 3-form over a 3-sphere surrounding the black hole to find the total charge. This can also be written in tensor terms, where the current J is equal to the covariant derivative of the field tensor F, and the time component of J can be integrated over a volume to find the total charge.
  • #1
praharmitra
311
1
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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  • #2
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
 
  • #3
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.
 
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  • #4
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).
 

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

What is the significance of finding flux through a black hole?

The flux through a black hole is an important measure of its gravitational pull. It tells us how much matter or energy is passing through the black hole's event horizon, and can help us understand the dynamics of the black hole and its surrounding environment.

How is the metric g used in calculating flux through a black hole?

The metric g, also known as the spacetime metric, is used to describe the curvature of spacetime around a black hole. It is a mathematical tool that allows us to calculate the gravitational field strength and thus the flux through the black hole.

Can flux through a black hole be measured directly?

No, flux through a black hole cannot be measured directly. Instead, it is calculated using theoretical models based on the black hole's mass and properties, such as its spin and charge.

What role does the gauge field A play in finding flux through a black hole?

The gauge field A represents the electromagnetic field around a black hole. It is an important factor in calculating the flux through the black hole, as it influences the trajectories of particles and radiation near the event horizon.

How does finding flux through a black hole contribute to our understanding of the universe?

Finding flux through a black hole is a crucial part of studying the behavior of these mysterious objects. It can help us test theories of gravity and black hole physics, and provide insights into the formation and evolution of galaxies and the universe as a whole.

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