Non-Linear Theory: Summation Meaningful in Einstein Gravitation?

In summary, the conversation discusses the stress-energy tensor in the famous book "Gravitation" by Misner, Thorne, and Wheeler, and its relevance in the non-linear theory of Einstein's gravitation. The stress-energy tensor is summed up from different categories of particles in an infinitesimal region, but this method is not affected by the non-linearities mentioned. The conversation also clarifies that tensors are locally defined quantities and there is no such thing as a stress-energy tensor for a finite region. Additionally, it is noted that the equations of motion are linear in the stress-energy tensor but nonlinear in the metric and its derivatives.
  • #1
empdee4
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TL;DR Summary
In the Gravitation book by Misner, Thorne and Wheeler. The total stress-energy of a swarm of particles is summed up from all categories. Is summation meaningful in non-linear theory? Thanks.
In the famous book, Gravitation, by Misner, Thorne and Wheeler, it talks about the stress-energy tensor of a swarm of particles (p.138). The total stress-energy is summed up from all categories of particles. Is summation meaningful in the non-linear theory of Einstein gravitation? Thanks.
 
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  • #2
empdee4 said:
Is summation meaningful in the non-linear theory of Einstein gravitation?
It is the way MTW are doing it in that particular example. They are not summing over a finite volume of spacetime, which would require taking into account the non-linearities you mention. They are summing over different categories of particles in the same infinitesimal volume of spacetime, which is not affected by the non-linearities you mention.
 
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  • #3
Thanks very much. In MTW book, the stress-energy tensor of each category of particles is written as a vector product. Does it mean this also can happen in an infinitesimal region only? That is, in a finite region, it cannot be written as vector product
 
  • #4
There is no such thing as the stress energy tensor for a finite region. Tensors are locally defined quantities.
 
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In a manifold, each point in the manifold is associated with its own tangent space, and the stress-energy tensor (and other tensors, for that matter ) are defined in the tangent space of a particular point.

It is a common approximation, though, to lump together a bunch of nearby points into a small regoin as if they shared a common tangent space. Strictly speaking it's not correct, but it's a reasonable approximation in many cases.

As far as the non-linearites go, the right hand side of Einstein's field equations, ##T_{\mu\nu}## is perfectly linear. The left hand side , the Einstein tensor ##G_{\mu\nu## is where the non-linarities are.
 
  • #6
pervect said:
the right hand side of Einstein's field equations, ##T_{\mu\nu}## is perfectly linear.
To be clear, the SET will be linear in the metric; but it does not have to be linear in the matter fields or their derivatives.
 
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Thanks very much.
 
  • #8
But if one side of the equation is linear and the other side is non-linear, how can the two sides be equal?
 
  • #9
empdee4 said:
if one side of the equation is linear and the other side is non-linear, how can the two sides be equal?
The nonlinearities in the Einstein tensor are in derivatives of the metric, not the metric itself.
 
  • #10
PeterDonis said:
To be clear, the SET will be linear in the metric; but it does not have to be linear in the matter fields or their derivatives.
He means that the equations are linear in T.
 
  • #11
empdee4 said:
But if one side of the equation is linear and the other side is non-linear, how can the two sides be equal?
The stress energy tensor is the source of the Einstein equations. It need not depend on the metric at all. In general, the EFEs are a set of non-linear differential equations. This by no means imply that they cannot be solved.

What it does mean is that the solutions do not allow superpositioning. In other words, if you have two solutions with SETs T1 and T2, the sum of the solutions will not solve the EFEs with SET T1+T2.
 
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  • #12
empdee4 said:
But if one side of the equation is linear and the other side is non-linear, how can the two sides be equal?
$$x^2 + y^2 = 4y$$ is a perfectly valid equation.
 
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  • #13
PeterDonis said:
To be clear, the SET will be linear in the metric; but it does not have to be linear in the matter fields or their derivatives.
Indeed, e.g., for the em. field you have
$$T^{\mu \nu} =F^{\mu \rho} {F_{\rho }}^{\nu} + \frac{1}{4} F_{\rho \sigma} F^{\rho \sigma} g^{\mu \nu}.$$
 
  • #14
martinbn said:
He means that the equations are linear in T.
But they're also linear in the Einstein tensor ##G##, so if we just look to that level of detail, the equation is linear on both sides.

When people say the EFE is nonlinear, they mean that the Einstein tensor ##G## is nonlinear in the metric and its derivatives.
 
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  • #15
PeterDonis said:
But they're also linear in the Einstein tensor ##G##, so if we just look to that level of detail, the equation is linear on both sides.

When people say the EFE is nonlinear, they mean that the Einstein tensor ##G## is nonlinear in the metric and its derivatives.
I agree, i was just saying how i understood his post.
 
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  • #16
Thanks very much!
 

1. What is non-linear theory in Einstein gravitation?

Non-linear theory in Einstein gravitation is a mathematical framework used to describe the behavior of gravity in the presence of strong gravitational fields, such as those near massive objects like stars and black holes. It takes into account the non-linear interactions between matter and space-time, which are not accounted for in classical Newtonian gravity.

2. How does non-linear theory differ from linear theory in Einstein gravitation?

Linear theory in Einstein gravitation is based on the assumption that the gravitational field is weak and can be described by a linear relationship between matter and space-time. Non-linear theory, on the other hand, takes into account the non-linear effects of gravity, which become significant in strong gravitational fields.

3. What is the significance of summation in non-linear theory?

In non-linear theory, summation refers to the process of adding up the contributions of all the matter present in a given space to determine the overall gravitational field. This is important because in non-linear theory, the gravitational field is not simply the sum of the individual gravitational fields of each object, but rather a complex interaction between all the objects present.

4. How is summation meaningful in Einstein gravitation?

Summation is meaningful in Einstein gravitation because it allows us to accurately describe the behavior of gravity in the presence of strong gravitational fields. By taking into account the non-linear interactions between matter and space-time, summation allows us to make more accurate predictions and observations about the universe.

5. What are some real-world applications of non-linear theory in Einstein gravitation?

Non-linear theory in Einstein gravitation has many practical applications, such as predicting the behavior of black holes, understanding the formation and evolution of galaxies, and accurately measuring the expansion of the universe. It also plays a crucial role in modern technologies such as GPS systems, which rely on precise measurements of gravity to function.

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