Continuity equation (charge vs matter) in SR

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Discussion Overview

The discussion revolves around the continuity equation in the context of special relativity, specifically comparing the treatment of charge and matter within relativistic fluids. Participants explore the implications of the energy-momentum tensor and its relation to the continuity equations for both charged and uncharged fluids, examining whether a relativistic analogue exists for charge continuity.

Discussion Character

  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • Some participants present the energy-momentum tensor for a perfect relativistic fluid and derive the relativistic continuity equation from it.
  • Others suggest that a charged fluid can be considered, leading to a discussion about the electromagnetic stress-energy tensor (EM SET) and its role in the continuity equation.
  • One participant questions whether the continuity equation for charge has a relativistic analogue and discusses the charge-current density 4-vector, which follows a similar continuity equation.
  • There is mention of the pressure term in the relativistic generalization of the matter continuity equation and whether a charged relativistic fluid should also include a pressure term.
  • Some participants argue that the charge continuity equation does not contain a pressure term, while others clarify that the pressure is described in a separate set of equations related to the stress-energy tensor.
  • Discussion includes the distinction between isotropic and non-isotropic pressure in the context of electromagnetic fields and their stress-energy tensor.
  • One participant introduces the concept of "null dust" as a specific solution related to isotropic radiation, while others challenge the physical possibility of a spherical electromagnetic wave.

Areas of Agreement / Disagreement

Participants express differing views on the existence and form of a relativistic analogue for charge continuity compared to matter continuity. There is no consensus on whether a charged relativistic fluid should include a pressure term, with some arguing for its absence and others suggesting it is necessary in a different context.

Contextual Notes

The discussion highlights the complexity of relating charge and matter in relativistic frameworks, with unresolved questions about the nature of pressure in charged fluids and the implications of electromagnetic fields on the stress-energy tensor.

center o bass
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If we consider a perfect relativistic fluid it has energy momentum tensor

$$T^{\mu \nu} = (\rho + p) U^\mu U^\nu + p\eta^{\mu \nu} $$

where ##U^\mu## is the four-velocity field of the fluid. ##\partial_\mu T^{\mu \nu} = 0## then
implies the relativistic continuity equation

$$\partial_\mu(\rho U^\mu) + p \partial_\mu U^\mu = 0$$

which reduces to the ordinary continuity equation for matter

$$\partial_t \rho + \nabla \cdot (\rho \vec v) = 0$$

in the non-relativistic limit ##v << c## and ##p << \rho##. Charge obeys an identical equation in the same limit, but does it has a relativistic analogue? If not, why?
 
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Sure. Just consider a charged fluid.
 
center o bass said:
If we consider a perfect relativistic fluid it has energy momentum tensor

$$T^{\mu \nu} = (\rho + p) U^\mu U^\nu + p\eta^{\mu \nu} $$

where ##U^\mu## is the four-velocity field of the fluid. ##\partial_\mu T^{\mu \nu} = 0## then
implies the relativistic continuity equation

$$\partial_\mu(\rho U^\mu) + p \partial_\mu U^\mu = 0$$

which reduces to the ordinary continuity equation for matter

$$\partial_t \rho + \nabla \cdot (\rho \vec v) = 0$$

in the non-relativistic limit ##v << c## and ##p << \rho##. Charge obeys an identical equation in the same limit, but does it has a relativistic analogue? If not, why?
Sure, instead of the SET you use the EM SET in free space(electrovacuum). Look up the Einstein-Maxwell equations.
 
TrickyDicky said:
Sure, instead of the SET you use the EM SET in free space(electrovacuum). Look up the Einstein-Maxwell equations.

What does SET stand for? Could you provide a reference where I could find the relevant
equation? I could not find it when looking up the Einstein-Maxwell equations.
 
center o bass said:
What does SET stand for? Could you provide a reference where I could find the relevant
equation? I could not find it when looking up the Einstein-Maxwell equations.

SET= Stress-energy tensor
EM SET= Electromagnetic Stress-energy tensor, this is the SET of a charged fluid.
It is in Wikipedia, i think they even treat the continuity equation at the end of the article on the EM SET.
 
TrickyDicky said:
SET= Stress-energy tensor
EM SET= Electromagnetic Stress-energy tensor, this is the SET of a charged fluid.
It is in Wikipedia, i think they even treat the continuity equation at the end of the article on the EM SET.

Alright. I found two equations on the wikipedia article on the EM SET. But these are for the electromagnetic field itself. However the equation

$$\partial_t u_{em} + \nabla \cdot \vec{p}_{em} + \vec J \cdot \vec E = 0$$

where ##u_{em}, \vec p_{em}## is the electromagnetic field energy/momentum density. This does very much look like the one for a perfect fluid when ##\vec E = 0##.
 
WannabeNewton said:
Sure. Just consider a charged fluid.

You suggest just switching the energy density ##\rho## with the charge density and use exactly the same tensor?
 
center o bass said:
Charge obeys an identical equation in the same limit, but does it has a relativistic analogue?

There is a charge-current density 4-vector in relativity, which obeys a similar continuity equation to the stress-energy tensor. The 4-vector is usually written ##J^{\mu}##, where ##J^0 = \rho_c## is the charge density and ##J^k = \left( j_x, j_y, j_z \right)## is the current density. The continuity equation is just ##\partial_{\mu} J^{\mu} = 0##, which when written out in components becomes

$$
\frac{\partial \rho_c}{\partial_t} + \nabla \cdot \vec{j} = 0
$$

If we think of the charge as being carried by a fluid with ordinary velocity ##\vec{v}##, then ##\vec{j} = \rho_c \vec{v}## and the above equation becomes

$$
\frac{\partial \rho_c}{\partial_t} + \nabla \cdot \left( \rho \vec{v} \right) = 0
$$
 
PeterDonis said:
There is a charge-current density 4-vector in relativity, which obeys a similar continuity equation to the stress-energy tensor. The 4-vector is usually written ##J^{\mu}##, where ##J^0 = \rho_c## is the charge density and ##J^k = \left( j_x, j_y, j_z \right)## is the current density. The continuity equation is just ##\partial_{\mu} J^{\mu} = 0##, which when written out in components becomes

$$
\frac{\partial \rho_c}{\partial_t} + \nabla \cdot \vec{j} = 0
$$

If we think of the charge as being carried by a fluid with ordinary velocity ##\vec{v}##, then ##\vec{j} = \rho_c \vec{v}## and the above equation becomes

$$
\frac{\partial \rho_c}{\partial_t} + \nabla \cdot \left( \rho \vec{v} \right) = 0
$$

Indeed, but the relativistic generalization of the matter continuity equation also contains a pressure term. Is there any reason why a charged relativistic fluid should not contain pressure term?
 
  • #10
center o bass said:
Indeed, but the relativistic generalization of the matter continuity equation also contains a pressure term. Is there any reason why a charged relativistic fluid should not contain pressure term?

If you look at, for instance, http://web.mit.edu/edbert/GR/gr2b.pdf, you'll see that the stress energy tensor is the tensor product of the number-flux 4-vector and the energy-momentum 4-vecctor. This yields the pressure terms.

But for the charge continuity equation, you only need to take the tensor product of the charge (a scalar) and the number-flux 4-vector. Hence, you have a conserved 4-vector and no pressure terms. The components of the 4-vector are charge density and current.

For an informal diagram/description of the number-flux 4-vector and the charge continuity equation, take a look at the "flow of stuff" diagrams in https://www.physicsforums.com/showthr...04#post4632145 . And ignore the typo's (I switch midstream from meters to inches, for instance).

Once you know how worldline density transforms, you get the charge/current density by considering that each worldline carries charge, the energy-momentum 4-vector by considering that each worldline carries energy-momentum (a 4-vector).
 
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  • #11
center o bass said:
Indeed, but the relativistic generalization of the matter continuity equation also contains a pressure term. Is there any reason why a charged relativistic fluid should not contain pressure term?

There will in general be one, but it won't be contained in the charge-current density 4-vector. There are really two separate sets of equations: one describing the behavior of the charge-current and the EM fields, the other describing the behavior of stress-energy. The latter set of equations is what will contain the pressure term.

As far as how the presence of charged matter affects the latter set of equations, the electromagnetic stress-energy tensor on the Wikipedia page can help with that; but you should realize that this SET does not have the form of the perfect fluid, because the "pressure" it describes (which is stress-energy contained in the EM fields) is not isotropic; it is different in different spatial directions. So things won't look as simple as they do for a perfect fluid.
 
  • #12
PeterDonis said:
this SET does not have the form of the perfect fluid, because the "pressure" it describes (which is stress-energy contained in the EM fields) is not isotropic; it is different in different spatial directions. So things won't look as simple as they do for a perfect fluid.

Unless he is considering specific solutions like say isotropic radiation of a spherical EM wave, but yes in general the SET won't be a perfect fluid.
 
  • #13
TrickyDicky said:
Unless he is considering specific solutions like say isotropic radiation of a spherical EM wave

The proper term for what I think you're describing here is "null dust"--a perfect fluid composed of massless particles moving on null worldlines, whose pressure is one-third of its energy density.

A "spherical EM wave" is not physically possible: the lowest-order EM radiation is dipole, not monopole, and the SET associated with any kind of EM radiation will not be of the perfect fluid form. But null dust is a good approximation of a sort of spherically symmetric "average" of null radiation going in all directions equally. The Vaidya metric is the corresponding line element for this case.
 
  • #14
PeterDonis said:
The proper term for what I think you're describing here is "null dust"--a perfect fluid composed of massless particles moving on null worldlines, whose pressure is one-third of its energy density.
Right.
A "spherical EM wave" is not physically possible: the lowest-order EM radiation is dipole, not monopole, and the SET associated with any kind of EM radiation will not be of the perfect fluid form. But null dust is a good approximation of a sort of spherically symmetric "average" of null radiation going in all directions equally. The Vaidya metric is the corresponding line element for this case.

Well, I guess the spherical wave example is not the best example here. But saying they are physically imposible seems to me a bit of a strong statement. One should discuss first the possibility of point sources, certainly in practice they are accepted in astrophysics for distant stars light, pulsar radio sources... but I guess they are just an idealization.

Quoting Wikipedia:"a point source is a singularity from which flux or flow is emanating. Although singularities such as this do not exist in the observable universe"
Unless one decides on physical impossibility judging only from what is directly observable, most of modern physics including elementary point particles-charges, and BH's point masses would go out the window.
 
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  • #15
TrickyDicky said:
But saying they are physically imposible seems to me a bit of a strong statement.

Yes, it is, but it's a simple consequence of the fact that the EM field is spin-1, plus conservation laws. You can construct approximate models of spherically symmetric EM radiation, but they will always be approximate; there are no spherically symmetric exact solutions.

TrickyDicky said:
One should discuss first the possibility of point sources, certainly in practice they are accepted in astrophysics for distant stars light, pulsar radio sources... but I guess they are just an idealization.

Exactly. They're not exact models; they're just approximations that work well enough for the purpose intended.

TrickyDicky said:
Unless one decides on physical impossibility judging only from what is directly observable, most of modern physics including elementary point particles-charges, and BH's point masses would go out the window.

Those are idealizations as well; when taken literally they have obvious problems, such as the infinite self-field of a point particle. But as approximate models (in this case to an underlying physics that we don't fully understand right now, perhaps something like string theory at the Planck scale) they work fine for what we use them for.
 
  • #16
Agree.

Ironically all the important theories, CM, CED, QED, GR.. have those singularities built in their theoretical structure not just as idealizations or approximations but as a necessary part for them to be mathematically coherent.
 

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