Jump to content

Swartzchild metric?


Endercreeper01

Recommended Posts

Not sure what "gab" is supposed to be, but what you posted seems like a single entry of the Schwarzschild metric, at best. The Schwarzschild metric is a tensor (written in particular coordinates), and some of its entries do depend on the mass.

Link to comment
Share on other sites

Not sure what "gab" is supposed to be, but what you posted seems like a single entry of the Schwarzschild metric, at best. The Schwarzschild metric is a tensor (written in particular coordinates), and some of its entries do depend on the mass.

gab is the meric tensor

Edited by Endercreeper01
Link to comment
Share on other sites

[latex]g_{ab} = \left( \begin{matrix}-(1-2M/r) & 0 & 0 & 0 \\0 & (1-2M/r)^{-1} & 0 & 0 \\0 & 0 & r^2 & 0\\0 & 0 & 0 & r^2sin^2\theta \end{matrix} \right)[/latex]

 

It is slightly more complicated than you first posted

Link to comment
Share on other sites

the Swartzchild metric (using spherical coordinates are t, r, Θ, Φ) ds2=(1-2GM/rc2)dt2- (1-2GM/rc2)-1dr2-r2(dΘ2+r2sin2ΘdΦ). The metric tensor, gab=ds2/Σdxadxb. If you work everything out, then it becomes -r4sin2θ


[latex]g_{ab} = \left( \begin{matrix}-(1-2M/r) & 0 & 0 & 0 \\0 & (1-2M/r)^{-1} & 0 & 0 \\0 & 0 & r^2 & 0\\0 & 0 & 0 & r^2sin^2\theta \end{matrix} \right)[/latex]

 

It is slightly more complicated than you first posted

(1-m/r) and (1-m/r)-1 cancel out and make -1, and the other part becomes r4sin2θ and so it all becomes -r4sin2θ

Link to comment
Share on other sites

Do you know what a matrix and/or a tensor are?

 

http://en.wikipedia.org/wiki/Tensor

 

you wrote this ds2=(1-2GM/rc2)dt2- (1-2GM/rc2)-1dr2-r2(dΘ2+r2sin2ΘdΦ)

 

that is the flat space limit which shows we get agreement with newtonian gravitation - although I think you are missing a c^2 from the first part. you can think of it - in a hazy way - of multiplying through that tensor and each section is multiplied by a different factor c^2dt^2, dr^2 dphi^2 and dtheta^2. what it actually is, i hope, is a line element; which is the summation of products of the tensor and four coordinate vectors (phi, theta, radius, and time*c^2) giving the square of the arc length

Link to comment
Share on other sites

Do you know what a matrix and/or a tensor are?

 

http://en.wikipedia.org/wiki/Tensor

 

you wrote this ds2=(1-2GM/rc2)dt2- (1-2GM/rc2)-1dr2-r2(dΘ2+r2sin2ΘdΦ)

 

that is the flat space limit which shows we get agreement with newtonian gravitation - although I think you are missing a c^2 from the first part. you can think of it - in a hazy way - of multiplying through that tensor and each section is multiplied by a different factor c^2dt^2, dr^2 dphi^2 and dtheta^2. what it actually is, i hope, is a line element; which is the summation of products of the tensor and four coordinate vectors (phi, theta, radius, and time*c^2) giving the square of the arc length

then how would you calculate the determinant of a 4x4 matrix? and yes, I do

and it is actually the swartzchild metric:

Schwarzschild metric[edit source | edit]

Besides the flat space metric the most important metric in general relativity is the Schwarzschild metric which can be given in one set of local coordinates by

ab2394b74a7ad0e022164f78636f25ce.png

Link to comment
Share on other sites

the Swartzchild metric (using spherical coordinates are t, r, Θ, Φ) ds2=(1-2GM/rc2)dt2- (1-2GM/rc2)-1dr2-r2(dΘ2+r2sin2ΘdΦ). The metric tensor, gab=ds2/Σdxadxb. If you work everything out, then it becomes -r4sin2θ

(1-m/r) and (1-m/r)-1 cancel out and make -1, and the other part becomes r4sin2θ and so it all becomes -r4sin2θ

Nonsense, you are confusing a matrix with its determinant.

Link to comment
Share on other sites

agree with xyzt - you seem to be thinking a matrix is merely its determinant.

 

What you have is the line element - which is the distance along an arc squared.

 

Your second equation is exactly the same as the first just represented in terms of solid angle rather than azimuth and inclination. If you really do understand matrices and tensors - then here is a page that describes line elements which is what you are getting with your ds^2 equations

 

http://en.wikipedia.org/wiki/Line_element

Link to comment
Share on other sites

Schwarzschild metric[edit source | edit]

Besides the flat space metric the most important metric in general relativity is the Schwarzschild metric which can be given in one set of local coordinates by

7200864b10447f816a79acc0d56107c5.png

where

dff0668f010356be54f01a28210139f6.png

from Wikipedia

agree with xyzt - you seem to be thinking a matrix is merely its determinant.

 

What you have is the line element - which is the distance along an arc squared.

 

Your second equation is exactly the same as the first just represented in terms of solid angle rather than azimuth and inclination. If you really do understand matrices and tensors - then here is a page that describes line elements which is what you are getting with your ds^2 equations

 

http://en.wikipedia.org/wiki/Line_element

oh

Link to comment
Share on other sites

  • 4 weeks later...

the exterior Schwarzschild metric is "four-volume preserving", i.e. space stretches, but time compresses, such that (c dt) dx dy dz = [math](c dt) r^2 dr sin(\theta) d\theta d\phi[/math] = constant

 

trying to take the Trace or determinant, and observing cancelations of crucial coefficients, is essentially the same, as noting that the warping of space-time about the body is "four-volume preserving", space stretches, but time "thins out", preserving the over-all (four) volume, a little like a piece of putty stretching in one dimension, but thinning out in orthogonal directions, preserving the overall volume of putty

Link to comment
Share on other sites

Create an account or sign in to comment

You need to be a member in order to leave a comment

Create an account

Sign up for a new account in our community. It's easy!

Register a new account

Sign in

Already have an account? Sign in here.

Sign In Now
×
×
  • Create New...

Important Information

We have placed cookies on your device to help make this website better. You can adjust your cookie settings, otherwise we'll assume you're okay to continue.