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Poincare's lemma on a star-shaped domain: every closed C1 field is exact
Statement
Let be open and star-shaped with respect to . Every closed field is exact. A potential is
Facts & Assumptions
Given: The star-shaped domain, centre, and closed field in the Statement.
Star-shapedness gives for every and (Star-shaped open subsets of Euclidean space).
Closedness is the system , and exactness requires a function with gradient (Exact and closed C1 vector fields).
On a compact rectangle, a continuous parameter derivative may be passed through the integral when it is represented by a continuous function (Leibniz's rule on a compact rectangle: an interior parameter derivative with a continuous extension may be passed through a Riemann integral).
If a continuous function has an integrable interior derivative on a compact interval, the integral of that derivative is the endpoint increment (Newton–Leibniz needs only continuity on , differentiability on , and a Riemann-integrable extension of the interior derivative).
Continuous partial derivatives imply total differentiability, with derivative matrix equal to the Jacobian (If all partial derivatives exist on a neighbourhood and are continuous at a point, then the map is totally differentiable there with Jacobian derivative).
Proof
By [L1], the integrand defining is defined for every ; it is continuous, so the integral exists. Fix and a coordinate . Openness and [L1] provide a small closed coordinate interval about whose radial segments from remain in .
On that interval, [L3] differentiates the defining integral with respect to and gives where . The integrand and its parameter derivative are continuous because is .
By closedness in [L2], . Thus the integrand in step 2.1 is
Apply [L4] to step 3.1. The endpoint at is , and the endpoint at is , so .
Since this holds for every and , the partial derivatives of are the functions . In particular they are continuous, so [L5] gives , and their first partials are continuous; hence is .
By the definition in [L2], step 5.1 makes exact with the displayed potential.
Depends on
- Exact and closed C1 vector fields
- 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
Used by
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Sources
- J.-B. Campesato, Poincare Lemma, section 2 (standard reference, not scraped)