Conservation of energy-momentum (tensor)

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Discussion Overview

The discussion revolves around the conservation of energy-momentum in the context of differential geometry and tensor calculus. Participants explore the implications of covariant derivatives, the dimensionality of manifolds, and the proper notation for expressing these concepts. The conversation includes technical aspects of tensor notation and the relationship between covariant divergence and covariant derivatives.

Discussion Character

  • Technical explanation
  • Conceptual clarification
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • Some participants discuss the parametrization of curves and the implications for tangent vectors in a potentially two-dimensional manifold.
  • Others argue that energy-momentum conservation pertains to four-dimensional spacetime, suggesting a misunderstanding of dimensionality in the original post.
  • There is a contention regarding the proper notation for tensors and vectors, with some participants emphasizing the need for consistency in conventions.
  • Participants question whether the covariant derivative of the energy-momentum tensor can be non-zero, with conflicting views on the requirements of the Einstein Field Equation.
  • Some participants clarify that the covariant divergence of a vector is distinct from the covariant derivative along a curve, leading to confusion in the original queries.
  • There are discussions about the notation used in expressing covariant derivatives and the potential for misunderstanding in the context of vector fields and basis vectors.

Areas of Agreement / Disagreement

Participants express differing views on the dimensionality of the manifold and the implications for energy-momentum conservation. There is no consensus on the correct interpretation of covariant derivatives versus covariant divergence, leading to ongoing debate and clarification attempts.

Contextual Notes

Participants note that the notation for covariant derivatives can be ambiguous, which may lead to confusion regarding the operations performed on vector fields and tensors. The discussion highlights the importance of clear definitions and conventions in tensor calculus.

Who May Find This Useful

This discussion may be useful for students and practitioners of differential geometry, general relativity, and theoretical physics who are grappling with the complexities of tensor notation and energy-momentum conservation.

Apashanka
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For a curve parametrised by ##\lambda## where ##\lambda## is along length of the curve and is 0 at one end point.
At each ##\lambda## say tangent vector V and A be the two possible vectors of the tangent space.
where ##V=V^\mu e_\mu## and ##A=A^\nu e_\nu##, {e} are the basis vectors.
Now ## \nabla_A V=A^\mu \nabla_\mu(V^\nu e_\nu)=A^\mu(\nabla_\mu V^\nu)e_\nu+A^\mu V^\nu(\nabla_\mu e_\nu)##Now if ##\nabla_\mu V^\nu=0## then the covariant derivative is still not zero .
Similarly from the energy-momentum conservation ##\nabla_\mu T^{\mu \nu}=0 ## from this can we say that in general the covariant derivative of this energy --momentum is non-zero by just comparing to rank 1 tensor??
May be there is something wrong above (I apologise) as I am trying to learn these things...
Thank you
 
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Apashanka said:
At each ##\lambda## say tangent vector V and A be the two possible vectors of the tangent space.

This would mean that the manifold is two-dimensional. Is that your intent? If you are asking about energy-momentum conservation, you are asking about spacetime, which is four-dimensional, not two-dimensional.

Apashanka said:
Now ##\nabla_A V=A^\mu \nabla_\mu(V^\nu e_\nu)=A^\mu(\nabla_\mu V^\nu)e_\nu+A^\mu V^\nu(\nabla_\mu e_\nu)##

Apashanka said:
Similarly from the energy-momentum conservation ##\nabla_\mu T^{\mu \nu}=0##
You're confusing yourself by writing formulas using two different conventions. If you are going to write a vector as ##V = V^\mu e_\mu##, then you need to also write a tensor as ##T = T^{\mu \nu} e_\mu e_\nu##. And you need to write the covariant derivative of a tensor similarly.

Apashanka said:
Now if ##\nabla_\mu V^\nu=0## then the covariant derivative is still not zero

If it happens to be the case that ##\nabla_\mu e_\nu \neq 0## in the coordinates you are using, yes. But there are coordinates in which ##\nabla_\mu e_\nu = 0##.

Apashanka said:
from this can we say that in general the covariant derivative of this energy --momentum is non-zero

Certainly not. The covariant derivative of the energy-momentum tensor is always zero; that is required by the Einstein Field Equation. But you have to write it down properly using the convention you want to use.
 
PeterDonis said:
This would mean that the manifold is two-dimensional. Is that your intent? If you are asking about energy-momentum conservation, you are asking about spacetime, which is four-dimensional, not two-dimensional.

You're confusing yourself by writing formulas using two different conventions. If you are going to write a vector as ##V = V^\mu e_\mu##, then you need to also write a tensor as ##T = T^{\mu \nu} e_\mu e_\nu##. And you need to write the covariant derivative of a tensor similarly.
If it happens to be the case that ##\nabla_\mu e_\nu \neq 0## in the coordinates you are using, yes. But there are coordinates in which ##\nabla_\mu e_\nu = 0##.
Certainly not. The covariant derivative of the energy-momentum tensor is always zero; that is required by the Einstein Field Equation. But you have to write it down properly using the convention you want to use.
Is it then ##\nabla_? T=0## where ##T=T^{\mu \nu}e_\mu e_\nu## from the energy momentum conservation ??
What will be then the subscript of ##\nabla##??
 
Apashanka said:
Is it then ##\nabla_? T=0## where ##T=T^{\mu \nu}e_\mu e_\nu## from the energy momentum conservation ??

Energy-momentum conservation is a covariant divergence; that's why the index ##\mu## is repeated in the expression ##\nabla_\mu T^{\mu \nu}##. It's a sum over all four possible values of ##\mu##. It's not a covariant derivative along a curve.
 
PeterDonis said:
Energy-momentum conservation is a covariant divergence; that's why the index ##\mu## is repeated in the expression ##\nabla_\mu T^{\mu \nu}##. It's a sum over all four possible values of ##\mu##. It's not a covariant derivative along a curve.
Ok if I want to compare this with the covariant derivative of a tangent vector V along the tangent vector then ##\nabla_V V=V^\mu \nabla_\mu(V^\nu e_\nu)=V^\mu (\nabla_\mu V^\nu) e_\nu + V^\mu V^\nu (\nabla_\mu e_\nu)## Are the two bracketed terms in the last called the covariant divergence of a vector and similarly for tensors it become ##\nabla_i A^{jk}=0## and for energy momentum tensor ##\nabla_\mu T^{\mu \nu}=0## but why can't it be ##\nabla_\alpha T^{\mu \nu}=0## where all three ##\alpha,\mu,\nu=0,1,2,3##??
 
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Apashanka said:
if I want to compare this with the covariant derivative of a tangent vector V along the tangent vector

Then you are doing it wrong. The covariant derivative along a curve is a different thing from a covariant divergence.

Apashanka said:
Are the two bracketed terms in the last called the covariant divergence of a vector

No. See above.
 
@Apashanka, you say you are trying to learn these things, but making repeated posts here about extremely basic questions--the kind people usually learn by working through a textbook--seems to be a very inefficient way of doing it. What textbooks on differential geometry have you studied?
 
PeterDonis said:
@Apashanka, you say you are trying to learn these things, but making repeated posts here about extremely basic questions--the kind people usually learn by working through a textbook--seems to be a very inefficient way of doing it. What textbooks on differential geometry have you studied?
Studying from books I find it confusing and sometimes out of my capacity...that's why I am trying to make these concepts clear by the people of this community
 
Apashanka said:
Studying from books I find it confusing and sometimes out of my capacity...that's why I am trying to make these concepts clear by the people of this community
Much much more effective is to work through a textbook until you find yourself stuck, and then asking for help getting past the hard spot.
 
  • #10
PeterDonis said:
Then you are doing it wrong. The covariant derivative along a curve is a different thing from a covariant divergence.
Ok then the covariant divergence of a vector ##V=V^\nu e_\nu## will be ##\nabla_\mu V^\mu## e.g sum over ##\mu## .
Thanks sir I got it now.
 
  • #11
Apashanka said:
the covariant divergence of a vector ##=V^\nu e_\nu## will be ##\nabla_\mu V^\mu## e.g sum over ##\mu## .

Yes.
 
  • #12
Apashanka said:
Now ## \nabla_A V=A^\mu \nabla_\mu(V^\nu e_\nu)=A^\mu(\nabla_\mu V^\nu)e_\nu+A^\mu V^\nu(\nabla_\mu e_\nu)##Now if ##\nabla_\mu V^\nu=0## then the covariant derivative is still not zero .

I think you are getting confused by the notation. When people write the expression ##\nabla_\mu V^\nu##, what they really mean is something like:

##(\nabla_\mu V)^\nu##

##\nabla_\mu## operates on a vector field to produce another vector field. Then you take component ##\nu## of that vector field. The result is ##\nabla_\mu V^\nu##.

##\nabla_\mu## already takes into account BOTH (1) the variation of the components ##V^\nu##, and (2) the variation of the basis vectors ##e_\nu##.

In terms of components, you could write:

##\nabla_\mu (V^\nu e_\nu) = (\partial_\mu V^\nu) e_\nu + V^\nu (\nabla_\mu e_\nu)##

By definition, the connection coefficient ##(\nabla_\mu e_\nu) = \Gamma^\lambda_{\mu \nu} e_\lambda##. So we have:

##\nabla_\mu (V^\nu e_\nu) = (\partial_\mu V^\nu) e_\nu + V^\nu (\Gamma^\lambda_{\mu \nu} e_\lambda)##

In the second term, ##\nu## and ##\lambda## are dummy indices, since they are summed over. So switching ##\nu## and ##\lambda## does nothing:
##V^\nu (\Gamma^\lambda_{\mu \nu} e_\lambda) = V^\lambda (\Gamma^\nu_{\mu \lambda} e_\nu)##

Substituting this into our expression for ##\nabla_\mu (V^\nu e_\nu)## gives:

##\nabla_\mu (V^\nu e_\nu) = (\partial_\mu V^\nu) e_\nu + V^\lambda (\Gamma^\nu_{\mu \lambda} e_\nu) = (\partial_\mu V^\nu + \Gamma^\nu_{\mu \lambda} V^\lambda) e_\nu##

The expression ##(\partial_\mu V^\nu + \Gamma^\nu_{\mu \lambda} V^\lambda)## is what people usually write as ##\nabla_\mu V^\nu##. So you can write, with a little ambiguity of notation:

##\nabla_\mu (V^\nu e_\nu) = (\nabla_\mu V^\nu) e_\nu##
 
  • #13
This has been my complaint about the notation ##\nabla_\mu V^\nu##. It looks like it's an operator on components of a vector field, but it isn't. It's an operator on vector fields. You take the covariant derivative of the vector field ##V##. That produces a new vector field. Then you take component ##\nu## of that new field. The result is ##\nabla_\mu V^\nu##.
 
  • #14
stevendaryl said:
This has been my complaint about the notation ##\nabla_\mu V^\nu##. It looks like it's an operator on components of a vector field, but it isn't. It's an operator on vector fields. You take the covariant derivative of the vector field ##V##. That produces a new vector field. Then you take component ##\nu## of that new field. The result is ##\nabla_\mu V^\nu##.
If V be a tangent vector to a curve then the covariant derivative of V along V is ##\nabla_V V## ...(1)
##\nabla_V=V^i\nabla_i##www.physicsforums.com/threads/covariant-derivative-of-tangent-vector-for-geodesic.966893/#post-6138635##
therefore (1) becomes ##V^i\nabla_i V## and the ##\nu^{th}## component of this new vector is ##(V^i\nabla_i V)^\nu=V^i\nabla_i V^\nu## then what will be the next step in expanding this??
 
  • #15
Apashanka said:
If V be a tangent vector to a curve then the covariant derivative of V along V is ##\nabla_V V## ...(1)

I think you are misunderstanding what "covariant derivative" means. In general, if you have TWO different vector fields ##U## and ##V## then the meaning of ##\nabla_U V## is this: ##\nabla_U V = U^\alpha (\partial_\alpha V^\beta + \Gamma^\beta_{\alpha \lambda} V^\lambda) e_\beta##. Or in terms of components,

##\nabla_U V^\beta = U^\alpha (\partial_\alpha V^\beta + \Gamma^\beta_{\alpha \lambda} V^\lambda)##

The case where ##V = U## is a special case, but that's not what "covariant derivative" means.
 
  • #16
Apashanka said:
If V be a tangent vector to a curve then the covariant derivative of V along V is ##\nabla_V V## ...(1)
##\nabla_V=V^i\nabla_i##www.physicsforums.com/threads/covariant-derivative-of-tangent-vector-for-geodesic.966893/#post-6138635##
therefore (1) becomes ##V^i\nabla_i V## and the ##\nu^{th}## component of this new vector is ##(V^i\nabla_i V)^\nu=V^i\nabla_i V^\nu## then what will be the next step in expanding this??

The meaning of ##\nabla_V V## is the vector field with components ##V^\alpha (\partial_\alpha V^\beta + \Gamma^\beta_{\alpha \lambda} V^\lambda)##
 
  • #17
stevendaryl said:
The meaning of ##\nabla_V V## is the vector field with components ##V^\alpha (\partial_\alpha V^\beta + \Gamma^\beta_{\alpha \lambda} V^\lambda)##
Yaa got it now thanks
 
  • #18
stevendaryl said:
This has been my complaint about the notation ##\nabla_\mu V^\nu##. It looks like it's an operator on components of a vector field, but it isn't. It's an operator on vector fields. You take the covariant derivative of the vector field ##V##. That produces a new vector field. Then you take component ##\nu## of that new field. The result is ##\nabla_\mu V^\nu##.
But I find it still confusing with covariant divergence of a vector field V which is ##\nabla_\mu V^\mu## where ##V^\mu## are the components of the vector and,, ##\mu^{th}## component of covariant derivative of a vector field V which is ##(\nabla_\mu V)^\mu##
 
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  • #19
Apashanka said:
But I find it still confusing with covariant divergence of a vector field V which is ##\nabla_\mu V^\mu## where ##V^\mu## are the components of the vector and,, ##\mu^{th}## component of covariant derivative of a vector field V which is ##(\nabla_\mu V)^\mu##
Yaa got it now in covariant divergence there is a summation over ##\mu## and in covariant derivative it is not.
Is it right??
 
  • #20
Apashanka said:
But I find it still confusing with covariant divergence of a vector field V which is ##\nabla_\mu V^\mu## and ##\mu^{th}## component of covariant derivative of a vector field V which is ##(\nabla_\mu V)^\mu##

Let's go through a simple example. Two-dimensional space with Cartesian coordinates ##x## and ##y##. In that case

##\nabla_\mu V^\nu = \partial_\mu V^\nu##

because ##\Gamma^\nu_{\mu \lambda}## is zero for Cartesian coordinates.

The covariant divergence is ##\nabla_\mu V^\mu = \partial_\mu V^\mu = \partial_x V^x + \partial_y V^y##

Now, let's switch to polar coordinates ##r, \theta##.

##\nabla_\mu V^\mu = \nabla_r V^r + \nabla_\theta V^\theta = \partial_r V^r + \Gamma^r_{r \lambda} V^\lambda + \partial_\theta V^\theta + \Gamma^\theta_{\theta \lambda} V^\lambda##

where ##\lambda## is summed over. So expanding the sum over ##\lambda##:

##\nabla_\mu V^\mu = \partial_r V^r + \Gamma^r_{r r} V^r + \Gamma^r_{r \theta} V^\theta + \partial_\theta V^\theta + \Gamma^\theta_{\theta r} V^r + \Gamma^\theta_{\theta \theta} V^\theta##

For polar coordinates, the only nonzero connection coefficients are ##\Gamma^r_{\theta \theta} = -r## and ##\Gamma^\theta_{r \theta} = \Gamma^\theta_{\theta r} = \frac{1}{r}##. So

##\nabla_\mu V^\mu = \partial_r V^r + \partial_\theta V^\theta + \frac{1}{r} V^r ##
 
  • #21
stevendaryl said:
Let's go through a simple example. Two-dimensional space with Cartesian coordinates ##x## and ##y##. In that case

##\nabla_\mu V^\nu = \partial_\mu V^\nu##

because ##\Gamma^\nu_{\mu \lambda}## is zero for Cartesian coordinates.

The covariant divergence is ##\nabla_\mu V^\mu = \partial_\mu V^\mu = \partial_x V^x + \partial_y V^y##

Now, let's switch to polar coordinates ##r, \theta##.

##\nabla_\mu V^\mu = \nabla_r V^r + \nabla_\theta V^\theta = \partial_r V^r + \Gamma^r_{r \lambda} V^\lambda + \partial_\theta V^\theta + \Gamma^\theta_{\theta \lambda} V^\lambda##

where ##\lambda## is summed over. So expanding the sum over ##\lambda##:

##\nabla_\mu V^\mu = \partial_r V^r + \Gamma^r_{r r} V^r + \Gamma^r_{r \theta} V^\theta + \partial_\theta V^\theta + \Gamma^\theta_{\theta r} V^r + \Gamma^\theta_{\theta \theta} V^\theta##

For polar coordinates, the only nonzero connection coefficients are ##\Gamma^r_{\theta \theta} = -r## and ##\Gamma^\theta_{r \theta} = \Gamma^\theta_{\theta r} = \frac{1}{r}##. So

##\nabla_\mu V^\mu = \partial_r V^r + \partial_\theta V^\theta + \frac{1}{r} V^r ##
Yaa similarly I have thought for a 2-D space the covariant divergence of a vector field V is ##\nabla_i V^i=\nabla_1 V^1+\nabla_2 V^2## where ##V=V^\mu e_\mu##
And ith component of covariant derivative of V is ##(\nabla_i V)^i## which is either of ##\nabla_1 V^1## or ##\nabla_2 V^2## ,thats how the two term differs
 
  • #22
Apashanka said:
Yaa similarly I have thought for a 2-D space the covariant divergence of a vector field V is ##\nabla_i V^i=\nabla_1 V^1+\nabla_2 V^2## where ##V=V^\mu e_\mu##
And ith component of covariant derivative of V ##(\nabla_i V)^i## which is either of ##\nabla_1 V^1## or ##\nabla_2 V^2## ,thats how the two term differs

Usually, when someone writes ##\nabla_i V^i## they mean the sum over ##i##. So the result is not a vector any more. So it doesn't make sense to take a component of it.

Going back to coordinates ##x## and ##y##:

##\nabla_x V## is a vector, with components ##\nabla_x V^x## and ##\nabla_x V^y##
##\nabla_y V## is a different vector, with components ##\nabla_y V^x## and ##\nabla_y V^y##.

When people write ##\nabla_i V^i## they typically mean the sum: ##\nabla_x V^x + \nabla_y V^y##. That is not a vector. It is the sum of components of a vector. [edit] It is the sum of components of two different vectors.
 
  • #23
stevendaryl said:
Usually, when someone writes ##\nabla_i V^i## they mean the sum over ##i##. So the result is not a vector any more. So it doesn't make sense to take a component of it.

Going back to coordinates ##x## and ##y##:

##\nabla_x V## is a vector, with components ##\nabla_x V^x## and ##\nabla_x V^y##
##\nabla_y V## is a different vector, with components ##\nabla_y V^x## and ##\nabla_y V^y##.

When people write ##\nabla_i V^i## they typically mean the sum: ##\nabla_x V^x + \nabla_y V^y##. That is not a vector. It is the sum of components of a vector.
Yes ,,now got it...
 

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