Condition of Helmholtz theorem to hold.

In summary, the constraints on \vec{F} come from the need for integrals to converge and the assumption that the integrand is zero at infinity, but there may be additional constraints in practice.
  • #1
yungman
5,718
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I want to verify this, according to Griffiths p 557:
[tex]\vec{F}(\vec r')=-\nabla U+\nabla\times\vec A[/tex]
ONLY if both ##\nabla U\; and \; \nabla\times\vec A\rightarrow\;0## faster than ##\frac 1 {r^2}## as ##r\rightarrow\;\infty##.

But the requirement of ##\vec{F}(\vec r')## is only ##|\vec{F}(\vec r')|\rightarrow\;0## as ##r\rightarrow\;\infty##.

If divergence or curl of ##\vec{F}(\vec r')## has to roll off faster than ##\frac 1 {r^2}##, then ##\vec{F}(\vec r')## must roll off at least as fast as ##\frac 1 {r^2}##. Why is it not a requirement?

I read quite a few article, it is very unclear in this condition. Only Griffiths spelled out clearly, all the other books just beat around this.

Thanks
 
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  • #2
It appears that the constraints on [itex]\vec{F}[/itex] come from a different place than the constraints on its divergence and curl.

The reason why one needs [itex]\nabla \cdot \vec{F}[/itex] and [itex]\nabla \times \vec{F}[/itex] to decay like they do is because the solution is given explicitly by integrals such as

$$ \int d^3\vec{r}' \frac{\nabla \cdot \vec{F}(\vec{r}')}{|\vec{r}-\vec{r}'|} .$$

In order for this integral to converge, the integrand needs to decay faster than the measure, so like [itex]\frac{1}{r'^3}[/itex], so this gives your constraint on [itex]\nabla \cdot \vec{F}[/itex]. Furthermore, in the course of the proof, you integrate by parts, and you set the boundary term to zero. The boundary term from the "divergence" part looks like

$$ \oint_{r' = \infty} d^2\vec{a}' \frac{\vec{F}(\vec{r}') \cdot \hat{n}}{|\vec{r}-\vec{r}'|} $$

so by setting this to zero, you are merely assuming that the integrand is zero at [itex]r' = \infty[/itex].

Now in practice, in order for the conditions on the divergence and curl to hold, I suppose there are more stringent conditions on the function [itex]\vec{F}(\vec{r}')[/itex], so the second assumption might be superfluous in applications. However, most physicists are comfortable with setting everything to zero at infinity as soon as they see fit and don't really look twice at either of these conditions (you usually read "decays sufficiently quickly" without qualifications).
 

1. What is the Helmholtz theorem?

The Helmholtz theorem is a fundamental theorem in vector calculus that states that any sufficiently smooth vector field in three-dimensional space can be decomposed into the sum of an irrotational field (curl-free) and a solenoidal field (divergence-free).

2. What is the condition for the Helmholtz theorem to hold?

The condition for the Helmholtz theorem to hold is that the vector field must be defined and continuous in all of three-dimensional space, and its first and second partial derivatives must also be continuous.

3. What is an irrotational field?

An irrotational field is a vector field in which the curl (rotational component) is equal to zero at every point in space. This means that the field is conservative and can be described by a scalar potential function.

4. What is a solenoidal field?

A solenoidal field is a vector field in which the divergence (expansive component) is equal to zero at every point in space. This means that the field is divergence-free and has no sources or sinks.

5. Why is the Helmholtz theorem important?

The Helmholtz theorem is important because it allows us to simplify complex vector fields into simpler components, making them easier to analyze and understand. It also has various applications in physics, engineering, and other fields of science.

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