Understanding the stress-energy tensor

In summary, the stress-energy-tensor is a mathematical concept used to describe the distribution of energy and momentum in a physical system. One term in the tensor, T^(12), represents the flux of x-component momentum in the y-direction. This can be understood as the average momentum of particles passing through a membrane in that direction. For non-interacting particles, this is simply the product of the average velocity and the number of particles. In the case of an electromagnetic wave, the stress is given by the Maxwell stress tensor, which is the space-space component of the electromagnetic stress-energy tensor. This concept can be further understood through considering the flux of particle momentum through a membrane.
  • #1
Higgsono
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I have trouble understanding some terms in the stress-energy-tensor. For instance T^(12) stands for the flux of the x-component of momentum in the y-direction. But what does it means for the x-component of momentum to flow in the y direction? Since momentum is a vector should't the x-component always point in the x-direction?
 
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  • #2
Higgsono said:
But what does it means for the x-component of momentum to flow in the y direction? Since momentum is a vector should't the x-component always point in the x-direction?
This is a shear stress. In a shear stress you have a force in the x direction on a face which is normal to the y direction. The x component of the force does always point in the x direction, but it can cross a face which is normal to the y direction.
 
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  • #3
Dale said:
This is a shear stress. In a shear stress you have a force in the x direction on a face which is normal to the y direction. The x component of the force does always point in the x direction, but it can cross a face which is normal to the y direction.

So what does this mean for say an electromagnetic wave propagating through vacuum or a medium?
 
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  • #5
Higgsono said:
I have trouble understanding some terms in the stress-energy-tensor. For instance T^(12) stands for the flux of the x-component of momentum in the y-direction. But what does it means for the x-component of momentum to flow in the y direction? Since momentum is a vector should't the x-component always point in the x-direction?

In 3 dimensions, imagine that you have lots of particles moving around. You want to compute the flux of y-momentum in the x-direction. The way you do it is to consider a membrane that is set up parallel to the y-z plane, as shown in the figure. Let ##\Delta \overrightarrow{P}## be the momentum that passes through the membrane from left to right during a small time interval ##\Delta t##. The momentum flux in the x-direction will then be: ##\frac{\Delta \overrightarrow{P}}{A \Delta t}## (change in momentum per unit area per unit time).

So how do we calculate ##\Delta \overrightarrow{P}##? Well, in the simplest case, the particles are non-interacting. So the amount of momentum passing through the membrane is just the average momentum of each particle that passes through times the number of particles.

So we have: ##\Delta \overrightarrow{P} = \overrightarrow{P}_{av} \Delta N##

The number of particles that pass through the membrane during time ##\Delta t## is just:

##\Delta N = \rho V^x_{av} A \Delta t##

It's proportional to the area of the membrane, ##A##, the average velocity in the direction perpendicular to the membrane, ##(V^x)_{av}## and the number of particles per unit volume, ##\rho##, and the time ##\Delta t##. So putting it all together:

##\frac{\Delta \overrightarrow{P}}{A \Delta t} = \frac{\overrightarrow{P}_{av} \rho V^x_{av} A \Delta t}{A \delta t} = \overrightarrow{P}_{av} \rho V^x_{av}##

The flux of y-momentum in the x-direction would then be:

##P^y_{av} V^x_{av} \rho##

Nonrelativistically, ##P^y = m V^y##, so you have:

##T^{yx} = V^y_{av} V^x_{av} \rho_{m}## (where ##\rho_m## is ##m \rho##, the mass density, rather than the number density).

Relativistically, ##P^y = E/c^2 V^y## (where ##E## is the relativistic energy), so you have:

##T^{yx} = V^y_{av} V^x_{av} \rho_{E}/c^2## (where ##\rho_E## is ##E \rho##, the energy density, rather than the number density).
 
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  • #6
stevendaryl said:
In 3 dimensions, imagine that you have lots of particles moving around. You want to compute the flux of y-momentum in the x-direction. The way you do it is to consider a membrane that is set up parallel to the y-z plane, as shown in the figure. Let ##\Delta \overrightarrow{P}## be the momentum that passes through the membrane from left to right during a small time interval ##\Delta t##. The momentum flux in the x-direction will then be: ##\frac{\Delta \overrightarrow{P}}{A \Delta t}## (change in momentum per unit area per unit time).

So how do we calculate ##\Delta \overrightarrow{P}##? Well, in the simplest case, the particles are non-interacting. So the amount of momentum passing through the membrane is just the average momentum of each particle that passes through times the number of particles.

So we have: ##\Delta \overrightarrow{P} = \overrightarrow{P}_{av} \Delta N##

The number of particles that pass through the membrane during time ##\Delta t## is just:

##\Delta N = \rho V^x_{av} A \Delta t##

It's proportional to the area of the membrane, ##A##, the average velocity in the direction perpendicular to the membrane, ##(V^x)_{av}## and the number of particles per unit volume, ##\rho##, and the time ##\Delta t##. So putting it all together:

##\frac{\Delta \overrightarrow{P}}{A \Delta t} = \frac{\overrightarrow{P}_{av} \rho V^x_{av} A \Delta t}{A \delta t} = \overrightarrow{P}_{av} \rho V^x_{av}##

The flux of y-momentum in the x-direction would then be:

##P^y_{av} V^x_{av} \rho##

Nonrelativistically, ##P^y = m V^y##, so you have:

##T^{yx} = V^y_{av} V^x_{av} \rho_{m}## (where ##\rho_m## is ##m \rho##, the mass density, rather than the number density).

Relativistically, ##P^y = E/c^2 V^y## (where ##E## is the relativistic energy), so you have:

##T^{yx} = V^y_{av} V^x_{av} \rho_{E}/c^2## (where ##\rho_E## is ##E \rho##, the energy density, rather than the number density).

Thanks, I think it made it clearer.
 

Related to Understanding the stress-energy tensor

1. What is the stress-energy tensor and why is it important in physics?

The stress-energy tensor is a mathematical representation of the distribution of energy and momentum in a physical system. It is important in physics because it allows us to understand how energy and momentum are conserved and how they interact with the fabric of spacetime.

2. How is the stress-energy tensor calculated?

The stress-energy tensor is calculated using the Einstein field equations, which relate the curvature of spacetime to the distribution of matter and energy within it. It involves complex mathematical calculations and is usually done using computer simulations.

3. What are some physical quantities that can be derived from the stress-energy tensor?

Some physical quantities that can be derived from the stress-energy tensor include the energy density, momentum density, pressure, and stress. These quantities can help us understand the behavior of matter and energy in a given system.

4. Can the stress-energy tensor be used to study different types of energy, such as dark energy?

Yes, the stress-energy tensor can be used to study all forms of energy, including dark energy. It is a universal concept in physics and can be applied to any physical system, regardless of its composition or properties.

5. How does the stress-energy tensor relate to Einstein's theory of general relativity?

The stress-energy tensor is a fundamental concept in Einstein's theory of general relativity. It is used to describe the curvature of spacetime and how it is affected by the distribution of matter and energy. This, in turn, helps us understand the gravitational forces between objects and how they move in space.

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