Maxwell's equations in curved spacetime.

In summary: F^{ac}+g_{ab}\nabla^c F^{ac}In summary, the conversation discusses the equivalence of two sets of Maxwell's equations in curved spacetime, which can be written as \nabla^a F_{ab} = -4\pi j_b, \nabla_{[a} F_{bc] = 0 or as d*F = 4\pi*j, dF = 0. The person is seeking help in proving the equivalence of the first equations in each set, and has tried working it out in local coordinates and an orthonormal frame, but has not been successful. They have completed problem 1 and
  • #1
eok20
200
0
Maxwell's equations in curved spacetime can be written as
[tex]\nabla^a F_{ab} = -4\pi j_b, \nabla_{[a} F_{bc] = 0[/tex] or as [tex] d*F = 4\pi*j, dF = 0[/tex], where F is a two-form, j is a one-form and * is the Hodge star. How do you show that these two sets of equations are equivalent (basically, that the first from each set are equivalent since I see how the second ones are equivalent)? I tried working it out in local coordinates but it got really messy e.g. derivatives of the determinant of the metric and I was unable to get anywhere. I also tried to work it out in terms of an orthonormal frame (tetrad) but that didn't work since I don't know if the Christoffel symbols for the connection have a nice form in that basis.

Any help would GREATLY be appreciated.

Note this is problem 2 in chapter 4 of Wald's text.
 
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  • #2
eok20 said:
Any help would GREATLY be appreciated.

Note this is problem 2 in chapter 4 of Wald's text.

Are you done with problem 1? Completely? Sure?
 
  • #3
arkajad said:
Are you done with problem 1? Completely? Sure?

Yes, I've done problem 1 (showing that [tex]\nabla^b j_b = 0[/tex]) as well as problem 2a (showing that ** = +- 1). I am confident in both of my solutions to these-- does one of these help?
 
  • #4

FAQ: Maxwell's equations in curved spacetime.

What are Maxwell's equations in curved spacetime?

Maxwell's equations in curved spacetime are a set of equations that describe the behavior of electromagnetic fields in the presence of a curved spacetime, as described by Einstein's theory of general relativity. They are a modification of the original Maxwell's equations, which describe electromagnetic fields in flat spacetime.

How are Maxwell's equations in curved spacetime different from the original equations?

The main difference between Maxwell's equations in curved spacetime and the original equations is that the former takes into account the curvature of spacetime. This means that the equations are modified to include terms that account for the effects of gravity on electromagnetic fields.

Why are Maxwell's equations in curved spacetime important?

Maxwell's equations in curved spacetime are important because they allow us to understand how electromagnetic fields behave in the presence of massive objects, such as planets and stars. They also play a crucial role in understanding the behavior of electromagnetic waves in the context of general relativity.

What is the significance of Maxwell's equations in curved spacetime in modern physics?

Maxwell's equations in curved spacetime are a cornerstone of modern physics, as they bridge the gap between classical electromagnetism and Einstein's theory of general relativity. They are also essential for understanding and predicting the behavior of electromagnetic waves in the presence of massive objects, such as black holes.

How are Maxwell's equations in curved spacetime used in practical applications?

Maxwell's equations in curved spacetime have many practical applications, such as in the design of satellite communication systems and GPS technology. They are also used in the development of gravitational wave detectors, which rely on precise measurements of electromagnetic fields to detect the ripples in spacetime predicted by general relativity.

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