Calculating the area of a sphere

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To calculate the area of a sphere in Schwarzschild geometry, the formula used is 4πr², where the radial coordinate r is defined such that the area corresponds to this expression. For a sphere of radius 2M, the area is calculated as 16πM. The discussion also touches on the formulas for radial distance and volume between two radii, emphasizing that these calculations are valid up to the event horizon. There is clarification on the intrinsic definition of the radial coordinate in relation to the area, and it is noted that one can derive the area directly from mass without needing to reference the radius. The conversation concludes with agreement on the area calculation being 16πM.
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How do you calculate the area of a sphere? for example in schwarzschild geometry and considering only the three dimensional spatial metric, what would be the area (and how do u calculate it) of a sphere of radius 2M?
 
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It depends on how you define the radius. In Schwarzschild coordinates, the radial coordinate r is simply defined so that the surface area is 4\pi r^2 (or, equivalently, so that the circumference is 2\pi r).
 
The area is 4 pi M, approximately 12.56637062*M

For completeness sake:

The radial distance for an stationary observer between r1 and r2 is:

<br /> \sqrt {r_{{2}} \left( r_{{2}}-2\,M \right) }-\sqrt {r_{{1}} \left( r_{<br /> {1}}-2\,M \right) }+2\,M\ln \left( {\frac {\sqrt {r_{{2}}}+\sqrt {r_{<br /> {2}}-2\,M}}{\sqrt {r_{{1}}}+\sqrt {r_{{1}}-2\,M}}} \right) <br />

The volume between r1 and r2 is :

<br /> 4/3\,\pi \,\sqrt {{r_{{2}}}^{5} \left( r_{{2}}-2\,M \right) }+10/3\,<br /> \pi \,M\sqrt {{r_{{2}}}^{3} \left( r_{{2}}-2\,M \right) }+10\,\pi \,{M<br /> }^{2}\sqrt {r_{{2}} \left( r_{{2}}-2\,M \right) }+20\,\pi \,{M}^{3}<br /> \ln \left( 1/2\,{\frac {r_{{2}}}{M}}+1/2\,\sqrt {2\,{\frac {r_{{2}}}{<br /> M}}-4} \right) -4/3\,\pi \,\sqrt {{r_{{1}}}^{5} \left( r_{{1}}-2\,M<br /> \right) }-10/3\,\pi \,M\sqrt {{r_{{1}}}^{3} \left( r_{{1}}-2\,M<br /> \right) }-10\,\pi \,{M}^{2}\sqrt {r_{{1}} \left( r_{{1}}-2\,M<br /> \right) }-20\,\pi \,{M}^{3}\ln \left( 1/2\,{\frac {r_{{1}}}{M}}+1/2<br /> \,\sqrt {2\,{\frac {r_{{1}}}{M}}-4} \right) <br />

The Latex is cut off, but if you click on it you get the complete formula. I do not know how to use line breaks as the standard \\ does not seem to work, perhaps a moderator could help.

These formulas work up to and including the EH. There are other formulas that work passed the EH but only up to and not including r=0.
 
Last edited:
Passionflower, you're assuming what you want to prove, because the r coordinate you're using was defined so that the result was true.

See, for example, Hawking and Ellis, p. 149: "The coordinate r in this metric form is intrinsically defined by the requirement that 4\pi r^2 is the area of these surfaces of transitivity."
 
bcrowell said:
Passionflower, you're assuming what you want to prove, because the r coordinate you're using was defined so that the result was true.

See, for example, Hawking and Ellis, p. 149: "The coordinate r in this metric form is intrinsically defined by the requirement that 4\pi r^2 is the area of these surfaces of transitivity."
I don't want to prove anything I simply gave the poster the formulas to calculate area, distance and volume using Schwarzschild coordinates.

If there is something wrong with the formulas please tell if not I do not know what your problem is.
 
So is it 4 pi M or 16 pi M. Because if the area is 4*pi*r^2 and r = 2M it should be 16*pi*M right?
 
vitaniarain said:
...the area is 4*pi*r^2 and r = 2M it should be 16*pi*M right?
Right!

Or if you want to be complete:

A = 16 pi G2 m2/c4.​

You can go directly from the mass to the area, there is no need to actually consider the radius.
 

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