In mathematical functional analysis a partial isometry is a linear map between Hilbert spaces such that it is an isometry on the orthogonal complement of its kernel.
The orthogonal complement of its kernel is called the initial subspace and its range is called the final subspace.
Partial isometries appear in the polar decomposition.
General definition
The concept of partial isometry can be defined in other equivalent ways. If U is an isometric map defined on a closed subset H1 of a Hilbert space H then we can define an extension W of U to all of H by the condition that W be zero on the orthogonal complement of H1. Thus a partial isometry is also sometimes defined as a closed partially defined isometric map.
Partial isometries (and projections) can be defined in the more abstract setting of a semigroup with involution; the definition coincides with the one herein.
Characterization in finite dimensions
In finite-dimensional vector spaces, a matrix
is a partial isometry if and only if
is the projection onto its support. Contrast this with the more demanding definition of isometry: a matrix
is an isometry if and only if
. In other words, an isometry is an injective partial isometry.
Any finite-dimensional partial isometry can be represented, in some choice of basis, as a matrix of the form
, that is, as a matrix whose first
columns form an isometry, while all the other columns are identically 0.
Note that for any isometry
, the Hermitian conjugate
is a partial isometry, although not every partial isometry has this form, as shown explicitly in the given examples.
Operator Algebras
For operator algebras one introduces the initial and final subspaces:
![{\displaystyle {\mathcal {I}}W:={\mathcal {R}}W^{*}W,\,{\mathcal {F}}W:={\mathcal {R}}WW^{*}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/39354ba010dd3f106196c99aef8cb9b48d8d4451)
C*-Algebras
For C*-algebras one has the chain of equivalences due to the C*-property:
![{\displaystyle (W^{*}W)^{2}=W^{*}W\iff WW^{*}W=W\iff W^{*}WW^{*}=W^{*}\iff (WW^{*})^{2}=WW^{*}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/9e1df0abc6398de43d2332f63f263b875ba20d04)
So one defines partial isometries by either of the above and declares the initial resp. final projection to be W*W resp. WW*.
A pair of projections are partitioned by the equivalence relation:
![{\displaystyle P=W^{*}W,\,Q=WW^{*}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/e64505e750fb0ab56a1d06eb6dfb8dfa0dcffd93)
It plays an important role in K-theory for C*-algebras and in the Murray-von Neumann theory of projections in a von Neumann algebra.
Special Classes
Projections
Any orthogonal projection is one with common initial and final subspace:
![{\displaystyle P:{\mathcal {H}}\rightarrow {\mathcal {H}}:\quad {\mathcal {I}}P={\mathcal {F}}P}](https://wikimedia.org/api/rest_v1/media/math/render/svg/16f21dafc573077f335cdce69dae20e989306616)
Embeddings
Any isometric embedding is one with full initial subspace:
![{\displaystyle J:{\mathcal {H}}\hookrightarrow {\mathcal {K}}:\quad {\mathcal {I}}J={\mathcal {H}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/e15a451f500617b3094bf456fe47a09a27891244)
Unitaries
Any unitary operator is one with full initial and final subspace:
![{\displaystyle U:{\mathcal {H}}\leftrightarrow {\mathcal {K}}:\quad {\mathcal {I}}U={\mathcal {H}},\,{\mathcal {F}}U={\mathcal {K}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/a220edd0b005192f038cb386ec8f4bb2c38ade63)
(Apart from these there are far more partial isometries.)
Examples
Nilpotents
On the two-dimensional complex Hilbert space the matrix
![{\displaystyle {\begin{pmatrix}0&1\\0&0\end{pmatrix}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/3f2c2adffe3e1a938568783836cd8125f9b407c8)
is a partial isometry with initial subspace
![{\displaystyle \{0\}\oplus \mathbb {C} }](https://wikimedia.org/api/rest_v1/media/math/render/svg/f8c652cf4479defde4c3f6df110cc61013dbae92)
and final subspace
![{\displaystyle \mathbb {C} \oplus \{0\}.}](https://wikimedia.org/api/rest_v1/media/math/render/svg/47d396c6f7d799f78cfb26c32873f6df446b5a84)
Generic finite-dimensional examples
Other possible examples in finite dimensions are
![{\displaystyle A\equiv {\begin{pmatrix}1&0&0\\0&{\frac {1}{\sqrt {2}}}&{\frac {1}{\sqrt {2}}}\\0&0&0\end{pmatrix}}.}](https://wikimedia.org/api/rest_v1/media/math/render/svg/52d5cf844af8671c31ca6b993d7beb95e1edca60)
This is clearly not an isometry, because the columns are not orthonormal. However, its support is the span of
![{\displaystyle \mathbf {e} _{1}\equiv (1,0,0)}](https://wikimedia.org/api/rest_v1/media/math/render/svg/9b50f2a92be6581b626f13119baf529f8718929f)
and
![{\displaystyle {\frac {1}{\sqrt {2}}}(\mathbf {e} _{2}+\mathbf {e} _{3})\equiv (0,1/{\sqrt {2}},1/{\sqrt {2}})}](https://wikimedia.org/api/rest_v1/media/math/render/svg/ddd71e04d06704e07e4d1ce47a15566bf5f07431)
, and restricting the action of
![{\displaystyle A}](https://wikimedia.org/api/rest_v1/media/math/render/svg/7daff47fa58cdfd29dc333def748ff5fa4c923e3)
on this space, it becomes an isometry (and in particular, a unitary). One can similarly verify that
![{\displaystyle A^{*}A=\Pi _{\operatorname {supp} (A)}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/d218b3e32d4d2aa34ead3eab216269a953a3d700)
, that is, that
![{\displaystyle A^{*}A}](https://wikimedia.org/api/rest_v1/media/math/render/svg/e11e97df5a2c7e9c34416af7209e20c55db10ace)
is the projection onto its support.
Partial isometries do not necessarily correspond to squared matrices. Consider for example,
![{\displaystyle A\equiv {\begin{pmatrix}1&0&0\\0&{\frac {1}{2}}&{\frac {1}{2}}\\0&0&0\\0&{\frac {1}{2}}&{\frac {1}{2}}\end{pmatrix}}.}](https://wikimedia.org/api/rest_v1/media/math/render/svg/cd208b3c3625da8c10a210e7aca93f469d9ae9ac)
This matrix has support the span of
![{\displaystyle \mathbf {e} _{1}\equiv (1,0,0)}](https://wikimedia.org/api/rest_v1/media/math/render/svg/9b50f2a92be6581b626f13119baf529f8718929f)
and
![{\displaystyle \mathbf {e} _{2}+\mathbf {e} _{3}\equiv (0,1,1)}](https://wikimedia.org/api/rest_v1/media/math/render/svg/90c15314f4f7c59625911737d5d348e1e3845034)
, and acts as an isometry (and in particular, as the identity) on this space.
Yet another example, in which this time
acts like a non-trivial isometry on its support, is
![{\displaystyle A={\begin{pmatrix}0&{\frac {1}{\sqrt {2}}}&{\frac {1}{\sqrt {2}}}\\1&0&0\\0&0&0\end{pmatrix}}.}](https://wikimedia.org/api/rest_v1/media/math/render/svg/afe2929efae49aff51213031fb5ad7cc06735feb)
One can readily verify that
![{\displaystyle A\mathbf {e} _{1}=\mathbf {e} _{2}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/8e01ac49ea42efd8f63dc556024dd794541982ea)
, and
![{\displaystyle A\left({\frac {\mathbf {e} _{2}+\mathbf {e} _{3}}{\sqrt {2}}}\right)=\mathbf {e} _{1}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/3b89d5b649717568cc92ea8e55146e8a68117c36)
, showing the isometric behavior of
![{\displaystyle A}](https://wikimedia.org/api/rest_v1/media/math/render/svg/7daff47fa58cdfd29dc333def748ff5fa4c923e3)
between its support
![{\displaystyle \operatorname {span} (\{\mathbf {e} _{1},\mathbf {e} _{2}+\mathbf {e} _{3}\})}](https://wikimedia.org/api/rest_v1/media/math/render/svg/2b64383f9f13574555248bd3e3a573483cf025ae)
and its range
![{\displaystyle \operatorname {span} (\{\mathbf {e} _{1},\mathbf {e} _{2}\})}](https://wikimedia.org/api/rest_v1/media/math/render/svg/d84e6a3356cda7d4a5c25bcf3f504fba1b2b3c5d)
.
Leftshift and Rightshift
On the square summable sequences the operators
![{\displaystyle R:\ell ^{2}(\mathbb {N} )\to \ell ^{2}(\mathbb {N} ):(x_{1},x_{2},\ldots )\mapsto (0,x_{1},x_{2},\ldots )}](https://wikimedia.org/api/rest_v1/media/math/render/svg/881e7ac9535226e1a8d1157631f17b2af38ca17f)
![{\displaystyle L:\ell ^{2}(\mathbb {N} )\to \ell ^{2}(\mathbb {N} ):(x_{1},x_{2},\ldots )\mapsto (x_{2},x_{3},\ldots )}](https://wikimedia.org/api/rest_v1/media/math/render/svg/c694f70486f7004def0477eb7a701e586ecb0bf4)
which are related by
![{\displaystyle R^{*}=L}](https://wikimedia.org/api/rest_v1/media/math/render/svg/ae57c4ddaa4aaa94ee5c0021fd9f91a41e80896f)
are partial isometries with initial subspace
![{\displaystyle LR(x_{1},x_{2},\ldots )=(x_{1},x_{2},\ldots )}](https://wikimedia.org/api/rest_v1/media/math/render/svg/f6f447fa015df6acc10b52f92c44894c413531a9)
and final subspace:
.
References
External links