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Hilbert projection theorem
Encyclopedia
In mathematics, the Hilbert projection theorem is a famous result of convex analysis
that says that for every point
in a Hilbert space
and every closed convex
, there exists a unique point
for which
is minimized over
.
This is, in particular, true for any closed subspace M of
. In that case, a necessary and sufficient condition for
is that the vector
be orthogonal to
.
Let δ be the distance between x and C, (yn) a sequence in C such that the distance squarred between x and yn is below or equal to δ2 + 1/n. Let n and m be two integers, then the following equalities are true:
and
We have therefore:
By giving an upper bound to the first to terms of the equality and by noticing that the middle of yn and ym belong to C and has therefore a distance greater than or equal to δ from x, one gets :
The last inequality proves that (yn) is a Cauchy sequence
. Since C is complete, the sequence is therefore convergent to a point y in C, whose distance from x is minimal.
Let y1 and y2 be two minimizer. Then:
Since
belongs to C, we have
and therefore
Hence
, which proves unicity.
The condition is necessary:
Let
such that
for all
.
which proves that
is a minimizer.
The condition is necessary:
Let
be the minimizer. Let
and
.
is always positive. Therefore,![](http://image.absoluteastronomy.com/images/formulas/3/6/3367561-29.gif)
QED
Convex analysis
Convex analysis is the branch of mathematics devoted to the study of properties of convex functions and convex sets, often with applications in convex minimization, a subdomain of optimization theory....
that says that for every point
![](http://image.absoluteastronomy.com/images/formulas/3/6/3367561-1.gif)
Hilbert space
The mathematical concept of a Hilbert space, named after David Hilbert, generalizes the notion of Euclidean space. It extends the methods of vector algebra and calculus from the two-dimensional Euclidean plane and three-dimensional space to spaces with any finite or infinite number of dimensions...
![](http://image.absoluteastronomy.com/images/formulas/3/6/3367561-2.gif)
![](http://image.absoluteastronomy.com/images/formulas/3/6/3367561-3.gif)
![](http://image.absoluteastronomy.com/images/formulas/3/6/3367561-4.gif)
![](http://image.absoluteastronomy.com/images/formulas/3/6/3367561-5.gif)
![](http://image.absoluteastronomy.com/images/formulas/3/6/3367561-6.gif)
This is, in particular, true for any closed subspace M of
![](http://image.absoluteastronomy.com/images/formulas/3/6/3367561-7.gif)
![](http://image.absoluteastronomy.com/images/formulas/3/6/3367561-8.gif)
![](http://image.absoluteastronomy.com/images/formulas/3/6/3367561-9.gif)
![](http://image.absoluteastronomy.com/images/formulas/3/6/3367561-10.gif)
Proof
- Let us show the existence of y:
Let δ be the distance between x and C, (yn) a sequence in C such that the distance squarred between x and yn is below or equal to δ2 + 1/n. Let n and m be two integers, then the following equalities are true:
and
We have therefore:
By giving an upper bound to the first to terms of the equality and by noticing that the middle of yn and ym belong to C and has therefore a distance greater than or equal to δ from x, one gets :
The last inequality proves that (yn) is a Cauchy sequence
Cauchy sequence
In mathematics, a Cauchy sequence , named after Augustin-Louis Cauchy, is a sequence whose elements become arbitrarily close to each other as the sequence progresses...
. Since C is complete, the sequence is therefore convergent to a point y in C, whose distance from x is minimal.
- Let us show the uniqueness of y :
Let y1 and y2 be two minimizer. Then:
Since
![](http://image.absoluteastronomy.com/images/formulas/3/6/3367561-16.gif)
![](http://image.absoluteastronomy.com/images/formulas/3/6/3367561-17.gif)
Hence
![](http://image.absoluteastronomy.com/images/formulas/3/6/3367561-19.gif)
- Let us show the equivalent condition on y when C = M is a closed subspace.
The condition is necessary:
Let
![](http://image.absoluteastronomy.com/images/formulas/3/6/3367561-20.gif)
![](http://image.absoluteastronomy.com/images/formulas/3/6/3367561-21.gif)
![](http://image.absoluteastronomy.com/images/formulas/3/6/3367561-22.gif)
![](http://image.absoluteastronomy.com/images/formulas/3/6/3367561-23.gif)
![](http://image.absoluteastronomy.com/images/formulas/3/6/3367561-24.gif)
The condition is necessary:
Let
![](http://image.absoluteastronomy.com/images/formulas/3/6/3367561-25.gif)
![](http://image.absoluteastronomy.com/images/formulas/3/6/3367561-26.gif)
![](http://image.absoluteastronomy.com/images/formulas/3/6/3367561-27.gif)
is always positive. Therefore,
![](http://image.absoluteastronomy.com/images/formulas/3/6/3367561-29.gif)
QED