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A divergence-free field on a star-shaped open subset of has a vector potential
Statement
Let be open and star-shaped with star centre , and let be with on . Then has a vector potential on in the sense of Vector potentials of a continuous field on an open subset of : the map
understood coordinatewise, is on and satisfies .
Facts & Assumptions
Given: The star-shaped open set with centre , and the field with on . Throughout, and .
Given a continuous on an open , a map is a vector potential for when is on and (Vector potentials of a continuous field on an open subset of ).
A nonempty open is star-shaped with respect to when for every and (Star-shaped open subsets of Euclidean space).
For and in , (The cross product in ).
The divergence of a field on an open is , and for its curl is (Divergence and curl of a vector field).
If every partial derivative of exists, the Jacobian matrix is (The Jacobian matrix of partial derivatives and the gradient in the scalar-valued case).
For fields on an open subset of , (The divergence and curl of a cross product).
Let and , let be continuous, and suppose for every fixed that is differentiable on with derivative . Then is differentiable on with (Leibniz's rule on a compact rectangle: an interior parameter derivative with a continuous extension may be passed through a Riemann integral).
If is continuous on and differentiable on , and is Riemann integrable on with on , then (Newton–Leibniz needs only continuity on , differentiability on , and a Riemann-integrable extension of the interior derivative).
If is totally differentiable at and at , then (The chain rule for total derivatives: ).
If is totally differentiable at then for every ; in particular , and the matrix of is (A total derivative computes every directional derivative, and its matrix is the Jacobian).
If every partial derivative of exists on a neighbourhood of and is continuous at , then is totally differentiable at and is the linear map with matrix (If all partial derivatives exist on a neighbourhood and are continuous at a point, then the map is totally differentiable there with Jacobian derivative).
For real functions of one real variable differentiable at a point, is differentiable there and (Sums, scalar multiples, products and quotients: , , , and when ).
A continuous map from a compact metric space to a metric space is uniformly continuous (Heine-Cantor: a continuous map from a compact metric space to any metric space is uniformly continuous); a closed bounded subset of is compact (Heine-Borel in : with the Euclidean metric a subset of is compact if and only if it is closed and bounded, and the proof by bisection uses no choice principle; the same holds on the real line).
If and are integrable between and and throughout the closed interval with those endpoints, then (Uniformly close integrable functions have integrals differing by at most the interval length times their uniform error); a continuous function on a closed bounded interval is Riemann integrable (A continuous function on is Riemann integrable, by Heine-Cantor and Riemann's criterion).
Proof
Take to be the map displayed in the Statement. By [F2] every with lies in when , so is defined there; by [L9] each coordinate of the integrand, being continuous in , is integrable on , so is defined for every .
By [F3] each coordinate of is a sum of terms . The map is continuous, so each such term is continuous in ; and since is , [L6], [L4] and [L5] give , which is again continuous in , while is if and otherwise. Hence each coordinate of the integrand has, in each coordinate of , a partial derivative that is continuous in .
Fix , choose a closed box with in its interior, and fix indices . Applying [L2] with the th edge of , the other coordinates of held at those of , and , using step 1.2 for the continuity of and and for the derivative hypothesis, gives that exists at with . The set is closed and bounded in , hence compact by [L8], so the integrand of that formula is uniformly continuous on it by [L8]; given this supplies such that points of within make the two integrands differ by at most at every , and [L9] then bounds the difference of the two integrals by . So is continuous on the interior of , and as was arbitrary, is on and is defined by [F4] and [F5].
Fix with and consider the two fields and on . For the first, step 1.2 gives , so by [F5] its Jacobian matrix is and by [F4] its divergence is . For the second, is if and otherwise, so its Jacobian matrix is the identity and its divergence is ; both fields are since these derivatives are continuous.
Applying [L1] to those two fields at a fixed , and multiplying by , gives where by step 2.2 the term contributes , the term contributes , the term contributes and the term contributes . At this reads in the second and fourth terms, since there.
By [F4] each coordinate of is a difference of two of the partial derivatives produced in step 2.1, and each of those is an integral over ; subtracting the two integrals and using step 3.1 for the resulting integrand gives again coordinatewise.
For fixed , put on . The map is differentiable with derivative , and is totally differentiable by [L6], so [L4] and [L5] give ; with [L7] applied to the product of and each coordinate of this yields , the integrand of step 4.1, which is continuous on and hence integrable by [L9].
By step 5.1 the function is continuous on and differentiable there, and its derivative is the integrand of step 4.1, so [L3] applied coordinate by coordinate on evaluates that integral as , using and the factor at .
Steps 4.1 and 6.1 give on , and step 2.1 gives that is on ; by [F1] the constructed is a vector potential for .
Remarks
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Where each hypothesis enters. Star-shapedness is used exactly once, in step 1.1, to know that the segment from the centre to stays in so that the integral is defined. The vanishing of is used exactly once, in step 2.2, to kill the term ; without it the curl of would carry an extra term and the integrand would not be an exact derivative in .
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The potential is not unique and the formula is not canonical. Adding the gradient of any function leaves the curl unchanged by The curl of the gradient of a function vanishes, so the displayed is one witness among many; it is the one that vanishes at the star centre.
Depends on
- Vector potentials of a continuous field on an open subset of $\mathbb R^3$
- Divergence and curl of a $C^1$ vector field
- The divergence and curl of a cross product
- Star-shaped open subsets of Euclidean space
- Leibniz's rule on a compact rectangle: an interior parameter derivative with a continuous extension may be passed through a Riemann integral
- Newton–Leibniz needs only continuity on $[a,b]$, differentiability on $(a,b)$, and a Riemann-integrable extension of the interior derivative
- If all partial derivatives exist on a neighbourhood and are continuous at a point, then the map is totally differentiable there with Jacobian derivative
- The cross product in $\mathbb R^3$
- The chain rule for total derivatives: $D(g\circ f)(a)=Dg(f(a))\circ Df(a)$
- A total derivative computes every directional derivative, and its matrix is the Jacobian
- The Jacobian matrix of partial derivatives and the gradient in the scalar-valued case
- Sums, scalar multiples, products and quotients: $(f+g)'(c) = f'(c) + g'(c)$, $(\alpha f)'(c) = \alpha f'(c)$, $(fg)'(c) = f'(c)g(c) + f(c)g'(c)$, and $(f/g)'(c) = \bigl(f'(c)g(c) - f(c)g'(c)\bigr)/g(c)^{2}$ when $g(c) \ne 0$
- Heine-Cantor: a continuous map from a compact metric space to any metric space is uniformly continuous
- Uniformly close integrable functions have integrals differing by at most the interval length times their uniform error
- Heine-Borel in $\mathbb{R}^n$: with the Euclidean metric a subset of $\mathbb{R}^n$ is compact if and only if it is closed and bounded, and the proof by bisection uses no choice principle; the same holds on the real line
- A continuous function on $[a,b]$ is Riemann integrable, by Heine-Cantor and Riemann's criterion
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Sources
- J. Feldman, A. Rechnitzer and E. Yeager, CLP-4 Vector Calculus (University of British Columbia), Theorem 4.1.16 (standard reference, not scraped)