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Copyright © 2002, 2014 jsd

Conservation
as related to
Continuity and Constancy

John Denker

*   Contents

1  Conservation : The Basic Idea
2  Warning: Conflicting Terminology
3  The Current is Not Conserved
4  Conservation in Spacetime
5  Conservation versus Constancy
6  Quantifying Conservation
6.1  Differential Version
6.2  Integral Version
7  References

1  Conservation : The Basic Idea

When electric charge flows from place to place, it obeys a local conservation law. By that we mean something very specific:

Any decrease in the amount of charge in a given region of space
must be exactly balanced by
a simultaneous increase in the amount of charge in an adjacent region of space.

We can express the same idea in the form of an equation:

change in charge = net flow of charge 
(inside boundary)   (inward minus outward across boundary)
             (1)

The word “flow” in this expression has a very precise technical meaning, closely corresponding to one of the meanings it has in everyday life. Specifically: Charge cannot be created or destroyed, but it can flow one from one region to another. Any decrease in one region is exactly balanced by a simultaneous increase in an adjacent region.

(By way of contrast, if you want an example of something that flows but is not conserved, consider “the flow of ideas”. You can give me an idea without decreasing your own stock of ideas. As usual, flow refers to spreading from one region to a neighboring region.)

At this point we have three ideas on the table: conservation, change, and flow. In accordance with equation 1, we can understand conservation as a combination of change plus just the right amount of flow.

To repeat: electric charge cannot change arbitrarily; only certain types of changes are allowed. The relationship between the broad concept of “change” and the more-precise concept of “conservation” can be summarized as follows:

Conservation =  change+equal-and-opposite change + simultaneity + adjacency          
  = change+matching flow
             (2)

 
The use of the world “simultaneity” causes some people to wonder whether equation 2 can be relativistically correct. Well, it turns out that this equation is 100% kosher, relativistically and otherwise. We get into trouble with relativity when we talk about simultaneity at a distance, but since we are taking about adjacent changes – zero distance – there is no problem with simultaneity. Indeed, our notion of conservation is beautifully matched to modern notions of relativity. In spacetime, local conservation can be expressed in elegant, informative, and easy-to-visualize form, in terms of the continuity of world lines. This is discussed in section 4.

Our local conservation law is much more useful than the corresponding non-local conservation law would be, for the following reason: suppose I were to observe that some charge has vanished from my laboratory. It would do me no good to have a global law that asserts that a corresponding amount of charge has appeared “somewhere” else in the universe. There is no way of checking that assertion, so I would not know and not care whether charge was being globally conserved. Also there is no way to reconcile a non-local law with the requirements of special relativity.1 See reference 1 for more on this.

To summarize: The laws of physics do not permit charge to disappear now and reappear later. Similarly the laws do not permit charge to disappear from here and reappear at some distant place. Charge is conserved right here, right now.

As a corollary, as a special case of equation 2:

This stands in contrast to the general case. In general, it is important to distinguish the notion of conservation from the notion of constancy. In general, conservation does not imply constancy, nor vice versa. This is discussed in section 5.

2  Warning: Conflicting Terminology

Beware: The term “conservation” has two wildly different meanings.

The physics notion of conservation is the topic of this document. It is defined by expressions of the form equation 1.   The vernacular notion of conservation refers to protecting something against destruction, or especially against waste.

Example: Charge is always conserved – automatically, strictly, and locally – in accordance with equation 1.   Example: Conservation of endangered wildlife. People get to decide whether they want to conserve this-or-that. Sometimes they decide yes, sometimes no.

While we’re on the subject: Beware: There are two different notions of energy. There is a vernacular notion of energy that is important and widely used, yet is very different from the physics energy.

The physics energy includes all forms of energy, whether useful or not.   The vernacular energy refers to some ill-defined notion of “useful energy” or “available energy”.

Example: The rest energy is given by E=mc2.   Examples: The energy industry. The Department of Energy.

Suppose you see a statement of the form “Please conserve energy by turning out the lights”. Be careful not to intepret that in physics terms, because both of the key words – “conserve” and “energy” – are being given meanings wildly different from their physics meanings.

3  The Current is Not Conserved

Just because electrical charge is conserved does not mean that electrical current is conserved. In fact, the current is definitely not conserved. Imaging a loop of wire with some current flowing in it initially. If you just leave it alone, the current will die out. The current will not move into some neighboring region; it will just remain in place and get weaker. This is an absolutely clear example of non-conservation.

This is mostly just a terminology issue, because physically the current is intimately associated with the thing that is conserved. Indeed, you cannot even write down the equation for conservation of charge without mentioning the current also:

0 = 
∂ρ
t
 + ∇ · j
             (3)

One thing that we can say is that the current obeys an approximate continuity equation in three dimensions. More specifically, in the low-frequency limit – for so-called “DC” circuits – we can ignore the first term on the RHS of equation 3, and what’s left is a continuity equation for the current, namely equation 4:

0  ∇ · j     (3D continuity of current)       
         (provided there is no accumulation)            
             (4)

While we’re in the neighborhood, if we instead ignore the other term on the RHS of equation 3,

0  
∂ρ
t
      (constancy of charge)    
         (provided there is no flow)                
             (5)

In fluid dynamics, vortex lines obey a continuity equation. In electrodynamics, magnetic field lines obey an exact continuity equation in three dimensions. In any region where there are no electrical charges, electric field lines obey a continuity equation.

The important idea is that the full conservation equation – equation 3 – can be understood as a spacetime continuity equation, as discussed in section 4.

In some weird sense, the idea of constancy (equation 5) is an amputated part of the idea of conservation, and also the idea of three-dimensional continuity (equation 4) is an amputated part of conservation. These two terms working together give the proper idea of conservation, i.e. four-dimensional continuity (equation 3).

Bottom line: You shouldn’t talk about “conservation” of the current vector; that gives entirely the wrong idea. If you want to say something about the current, talk about the spacetime continuity of the [charge, current] 4-vector.

4  Conservation in Spacetime

An ordinary box in D=3 space has six faces. We can call them the ± X faces, the ± Y faces, and the ± Z faces. In D=4 spacetime, the corresponding object has eight faces. It has two ± T faces in addition to the six spatial faces.

Now let’s draw some spacetime diagrams. For simplicity we will conceal the Y and Z dimensions, and portray only the ± T and ± X faces of the box.

Figure 1 shows the world-line of a stationary parcel of electrical charge sitting at the location of our box. The world-line enters on the T=0 face and exits on the T=1 face. In other words, it was initially within the spatial extent of our box, and it remained so.

conservation-stationary
Figure 1: World-line of Stationary Parcel

World-lines crossing the ± T faces contribute to the time derivative of the amount of charge in the box. In the foregoing case, there are two equal and opposite contributions (one flowing in at T=0, and one flowing out at T=1). To say the same thing in other words, the amount of charge within the spatial extent of the box is the same at T=0 and T=1, so the amount of charge in that spatial region is constant, i.e. not changing with time.

In contrast, figure 2 shows the world-line of a non-stationary parcel of charge. The world-line enters via the T=0 face and exits via the X=1 face. In other words, the parcel was initially within the spatial extent of our box, but then it departed toward the right.

conservation-moving
Figure 2: World-line of Moving Parcel

In this case, the amount of charge in the spatial box at T=1 is less than the amount of charge at T=0. The charge is not locally constant, but it is locally conserved. The charge wasn’t destroyed, it just flowed across the X=1 boundary into the neighboring region.

We will make this more quantitative in a moment.

You can see where this line of reasoning is leading. The following notions are formally equivalent:

Contrast this with some non-conserved object, such as a photon. Here is the world-line of a photon that enters the box and gets absorbed; the world line enters the box but doesn’t go out again:

nonconservation-moving
Figure 3: World-line of Non-Conserved Object

To quantify the net flow across the ± X boundaries, we need to know something about velocity and charge density. Imagine a fluid that has the same velocity and the same charge-density everywhere. An example of such a situation is shown in figure 4.

conservation-replacement
Figure 4: Conservation with Replacement

In this case, the amount of charge in the box is constant, because whenever a parcel of charge leaves via the X=0 face, an equivalent amount of charge is entering via the X=1 face. Contrast this with figure 2, where the charge flowed out and was not replaced. This non-replacement could occur because the charge density was lower off to the left, and/or the velocity was lower off to the left. So we see we need to be concerned with

Another case that needs to be considered combines the previous idea of non-conservation with the idea of replacement, as shown in figure 5. You can see that the number of objects in the region of interest is constant, because every time one of them is destroyed it is replaced.

nonconservation-replacement
Figure 5: Non-Conservation with Replacement

A real-life example of this concerns the number of working light-bulbs in a room. The number of working light bulbs is not a conserved quantity, but the number is approximately constant, because every time a light bulb is destroyed you replace it.

Another example along the same lines is a continuous-flow reactor in a chemical plant, where chemicals of type A flow in and chemicals of type B flow out.

5  Conservation versus Constancy

It is important to distinguish the notion of constancy from the notion of conservation:

To be explicit: Conservation does not imply constancy, nor vice versa. Change does not imply non-conservation, nor vice versa. All four of the possibilities have already been illustrated:

    constant   non-constant    
conservation   Figure 1 (static)   Figure 2 (outflow)   
    Figure 4 (steady flow)   
    
non-conservation   Figure 5 (steady replacement)   Figure 3 (annihilation)   

As touched upon section 1, if you integrate the local conservation law over all space, you can derive a global conservation law as a corollary. It is true that global conservation is the same as global constancy ... but that does not mean that conservation is the came as constancy in general.

6  Quantifying Conservation

Now that we have a firm qualitative idea of conservation, let us now make the idea completely quantitative.

6.1  Differential Version

For an electrically-charged fluid, the product of charge density times velocity is called the current. A spatially-uniform current isn’t interesting from a conservation point of view, so we shall be particular interested in the spatial variation in the current. If there is more than one spatial direction, the current is a vector (just like the velocity) with X, Y, and Z components. What matters is the X-derivative of the X-component of flux, the Y-derivative of the Y-component, and the Z-derivative of the Z-component — in other words, the divergence.

So we can write the local conservation law as

∂ 
t
 (charge density) = − div(current density)              (6)

or equivalently

∂ 
t
 ρ + ∇ · j = 0              (7)


This is a 100% formal accurate statement of the local conservation law. It expresses the continuity of the world-line of each little bit of charge.

Homework: Check equation 7 using dimensional analysis. It shouldn’t take very long!

The structure of equation 7 is very elegant. It has the form

∂ 
t
(...) + 
∂ 
x
(...) + 
∂ 
y
(...) + 
∂ 
z
(...)
 = ...
             (8)

which is most elegantly understood as a four-dimensional divergence. If you leave off the ∂/∂t term you’ve got the plain old three-dimensional divergence. The key concept is that the world lines of a conserved quanity (such as charge) are divergence-free in D=4. They have no beginning or end. By way of contrast, if you projected the world lines onto three dimensions, they would not be divergence-free; there would be a nonzero divergence at any location where charge is accumulating. The timelike term in equation 8 is needed to make the equation correct. On the third hand, we can contrast this with magnetic field lines, which are divergence-free – i.e. endless – even in three dimensions.

In more detail: The world line of an element of a charge has a tangent vector at every point. This defines a vector field. At each point along the world line, there is a four-vector consisting of the three components of current plus a fourth component, representing the “flux” of charge flowing in the “time direction” – which is just the density of charge itself. Overall, this vector field is divergence-free in D=4.

Equation 7 is frame-independent. Each of the terms on the LHS is frame-dependent, but the LHS as a whole is the same in all frames, the same for all observers. The RHS is zero, which is manifestly invariant.

To repeat: In D=3 you can (temporarily) have a whole bunch of current diverging from some region of space. [In contrast, you cannot have magnetic flux lines diverging like this, not even temporarily.] The divergent current will deplete the charge density in that region. Meanwhile, if you take a D=4 view of the same situation, you will find that the [charge,current] four-vector has zero divergence. The world-lines of any conserved quantity are endless.

In the preceding paragraph, all the D=3 statements are frame-dependent, but the D=4 statements are frame-independent.

Of course, charge is by no means the only thing that behaves this way. There are lots of conserved quantities.

The picture of world-line continuity applies to them all.

The formulation in this section applies at a single point, or perhaps in the infinitesimal neighborhood of a point. (A neighborhood is necessary to make derivatives meaningful.) It involved density and flux, in particular the four-dimensional divergence of the [charge-density,current-density] 4-vector.

Similar laws apply to the [energy,momentum] 4-vector, but the details are messier. Note the contrast:

6.2  Integral Version

Rather than considering a single point, we now consider a region.

We take the differential version (as discussed in the previous section) and integrate it over a region. Using Stokes’s law, we find that the time-rate-of-change of current inside the boundary is equal to the amount of current flowing across the boundary.

The integral formulation implies the differential formulation and vice versa, subject to mild restrictions. Obviously things must be sufficiently differentiable, and the region of interest must be simply connected (no wormholes).

7  References

1.
John Denker,
“Modern Thermodynamics”
./thermo/

2.
John Denker,
“A Non-Sneaky Derivation of Euler’s Equation”
//www.av8n.com/physics/euler-flow.htm

3.
John Denker,
“Introduction to Force, Momentum, Torque, and Angular Momentum”
//www.av8n.com/physics/force-intro.htm

1
In some special cases, such as Wheeler/Feynman absorber theory, it is possible to make sense of non-local laws, provided we have a non-local conservation law plus a lot of additional information. Such theories are unconventional and very advanced, far beyond the scope of this document.
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Copyright © 2002, 2014 jsd