Tensor
From Wikipedia, the free encyclopedia
Cauchy stress tensor, a second-order tensor. The tensor's components, in a three-dimensional Cartesian coordinate system, form the matrix
whose columns are the stresses (forces per unit area) acting on the e1, e2, and e3 faces of the cube.
Tensors are
geometric objects that describe
linear relations between
vectors,
scalars, and other tensors. Elementary examples of such relations include the
dot product, the
cross product, and
linear maps. Vectors and scalars themselves are also tensors. A tensor can be represented as a
multi-dimensional array of numerical values. The
order (also
degree)
of a tensor is the dimensionality of the array needed to represent it,
or equivalently, the number of indices needed to label a component of
that array. For example, a linear map can be represented by a matrix (a
2-dimensional array) and therefore is a 2nd-order tensor. A vector can
be represented as a 1-dimensional array and is a 1st-order tensor.
Scalars are single numbers and are thus 0th-order tensors. It is very
important not to confuse dimensions of the array with dimensions of the
underlying vector space.
Tensors are used to represent correspondences between sets of
geometric vectors; for applications in engineering and Newtonian physics these are normally
Euclidean vectors. For example, the
Cauchy stress tensor T takes a direction
v as input and produces the stress
T(v)
on the surface normal to this vector for output thus expressing a
relationship between these two vectors, shown in the figure (right).
Because they express a relationship between vectors, tensors themselves must be
independent of a particular choice of
coordinate system. Finding the representation of a tensor in terms of a coordinate
basis results in an organized multidimensional array representing the tensor in that basis or
frame of reference. The coordinate independence of a tensor then takes the form of a
"covariant" transformation law
that relates the array computed in one coordinate system to that
computed in another one. The precise form of the transformation law
determines the
type (or
valence) of the tensor. The tensor type is a pair of natural numbers
(n, m) where
n is the number of
contravariant indices and
m is the number of
covariant indices. The total order of a tensor is the sum of these two numbers.
Tensors are important in physics because they provide a concise
mathematical framework for formulating and solving physics problems in
areas such as elasticity, fluid mechanics, and general relativity.
Tensors were first conceived by
Tullio Levi-Civita and
Gregorio Ricci-Curbastro, who continued the earlier work of
Bernhard Riemann and
Elwin Bruno Christoffel and others, as part of the
absolute differential calculus. The concept enabled an alternative formulation of the intrinsic
differential geometry of a
manifold in the form of the
Riemann curvature tensor.
[1]
Definition
There are several approaches to defining tensors. Although seemingly
different, the approaches just describe the same geometric concept using
different languages and at different levels of abstraction.
As multidimensional arrays
Just as a
vector with respect to a given
basis
is represented by an array of one dimension, any tensor with respect to
a basis is represented by a multidimensional array. The numbers in the
array are known as the
scalar components of the tensor or simply its
components. They are denoted by indices giving their position in the array, as
subscripts and superscripts,
after the symbolic name of the tensor. In most cases, the indices of a
tensor are either covariant or contravariant, designated by subscript or
superscript, respectively. The total number of indices required to
uniquely select each component is equal to the
dimension of the array, and is called the
order,
degree or
rank of the tensor.
[Note 1] For example, the entries of an order 2 tensor
T would be denoted
Tij,
Ti j,
Tij, or
Tij, where
i and
j are indices running from 1 to the
dimension of the related vector space.
[Note 2] When the basis and its
dual coincide (i.e. for an
orthonormal basis), the distinction between contravariant and covariant indices may be ignored; in these cases
Tij or
Tij could be used interchangeably.
[Note 3]
Just as the components of a vector change when we change the
basis of the vector space, the entries of a tensor also change under such a transformation. Each tensor comes equipped with a
transformation law that details how the components of the tensor respond to a
change of basis. The components of a vector can respond in two distinct ways to a
change of basis (see
covariance and contravariance of vectors), where the new basis vectors
are expressed in terms of the old basis vectors
as,
where
Ri j is a matrix and in the second expression the summation sign was suppressed (
a notational convenience introduced by Einstein that will be used throughout this article).
[Note 4] The components,
vi, of a regular (or column) vector,
v, transform with the
inverse of the matrix
R,
where the hat denotes the components in the new basis. While the components,
wi, of a covector (or row vector),
w transform with the matrix R itself,
The components of a tensor transform in a similar manner with a
transformation matrix for each index. If an index transforms like a
vector with the inverse of the basis transformation, it is called
contravariant
and is traditionally denoted with an upper index, while an index that
transforms with the basis transformation itself is called
covariant and is denoted with a lower index. The transformation law for an order-
m tensor with
n contravariant indices and
m − n covariant indices is thus given as,
Such a tensor is said to be of order or
type (n, m−n).
[Note 5] This discussion motivates the following formal definition:
[2]
Definition. A tensor of type (n, m − n) is an assignment of a multidimensional array
![T^{i_1\dots i_n}_{i_{n+1}\dots i_m}[\mathbf{f}]](https://lh3.googleusercontent.com/blogger_img_proxy/AEn0k_t2m_J70TZQYGMwgWWdsOHLTWjR-Hf7UciIC9X-wpyc9NucITV8PaYmjLN-2x8G3BRd-1JmZ5Varx_MQ_YS2VuQ5pNIQRqiX4xPWjzYQl5DKeTMDienYRQxm3RqFiDDtfTeiEnnrGcKXYdISc1YIQ=s0-d)
to each basis f = (e1,...,eN) such that, if we apply the change of basis
then the multidimensional array obeys the transformation law
![T^{i_1\dots i_n}_{i_{n+1}\dots i_m}[\mathbf{f}\cdot R] = (R^{-1})^{i_1}_{j_1}\cdots(R^{-1})^{i_n}_{j_n} R^{j_{n+1}}_{i_{n+1}}\cdots R^{j_{m}}_{i_{m}}T^{j_1,\ldots,j_n}_{j_{n+1},\ldots,j_m}[\mathbf{f}].](https://lh3.googleusercontent.com/blogger_img_proxy/AEn0k_tI5VHmgLueLXj2FpBLClYVCrDPD6v4AVkXTNIR8XkfUPPOk6WfIXT7hYUdhx_VDXTN2I3wR0kR3YZA7yZgVAMlJt21jh5jlrfLLgJ2LLFoKPTJDayCVZ2N6NZUeWHLWPklvJ1mMc_5wGAI1TYn=s0-d)
The definition of a tensor as a multidimensional array satisfying a transformation law traces back to the work of Ricci.
[1] Nowadays, this definition is still used in some physics and engineering text books.
[3][4]
Tensor fields
In many applications, especially in differential geometry and
physics, it is natural to consider a tensor with components that are
functions of the point in a space. This was the setting of Ricci's
original work. In modern mathematical terminology such an object is
called a
tensor field, often referred to simply as a tensor.
[1]
In this context, a
coordinate basis is often chosen for the tangent vector space. The transformation law may then be expressed in terms of
partial derivatives of the coordinate functions,
, defining a coordinate transformation,
[1]
As multilinear maps
A downside to the definition of a tensor using the multidimensional
array approach is that it is not apparent from the definition that the
defined object is indeed basis independent, as is expected from an
intrinsically geometric object. Although it is possible to show that
transformation laws indeed ensure independence from the basis, sometimes
a more intrinsic definition is preferred. One approach is to define a
tensor as a
multilinear map. In that approach a type
(n, m) tensor
T is defined as a map,
where
V is a
vector space and
V* is the corresponding
dual space of covectors, which is linear in each of its arguments.
By applying a multilinear map
T of type
(n, m) to a basis {
ej} for
V and a canonical cobasis {
εi} for
V*,
an (
n+
m)-dimensional array of components can be obtained. A different choice of basis will yield different components. But, because
T
is linear in all of its arguments, the components satisfy the tensor
transformation law used in the multilinear array definition. The
multidimensional array of components of
T thus form a tensor
according to that definition. Moreover, such an array can be realised as
the components of some multilinear map
T. This motivates viewing multilinear maps as the intrinsic objects underlying tensors.
Using tensor products
For some mathematical applications, a more abstract approach is
sometimes useful. This can be achieved by defining tensors in terms of
elements of
tensor products of vector spaces, which in turn are defined through a
universal property. A type
(n, m) tensor is defined in this context as an element of the tensor product of vector spaces,
[5]
If
vi is a basis of
V and
wj is a basis of
W, then the tensor product
has a natural basis
. The components of a tensor
T are the coefficients of the tensor with respect to the basis obtained from a basis {
ei} for
V and its dual {
εj}, i.e.
Using the properties of the tensor product, it can be shown that these components satisfy the transformation law for a type
(m, n) tensor. Moreover, the universal property of the tensor product gives a
1-to-1 correspondence between tensors defined in this way and tensors defined as multilinear maps.
Examples
This table shows important examples of tensors, including both
tensors on vector spaces and tensor fields on manifolds. The tensors are
classified according to their type
(n, m), where
n is the number of contravariant indices,
m is the number of covariant indices, and
n + m gives the total order of the tensor. For example, a
bilinear form is the same thing as a
(0, 2)-tensor; an
inner product is an example of a
(0, 2)-tensor, but not all
(0, 2)-tensors are inner products. In the
(0, M)-entry of the table,
M
denotes the dimensionality of the underlying vector space or manifold
because for each dimension of the space, a separate index is needed to
select that dimension to get a maximally covariant antisymmetric tensor.
-
| n, m |
n = 0 |
n = 1 |
n = 2 |
... |
n |
... |
| m = 0 |
scalar, e.g. scalar curvature |
vector (e.g. direction vector) |
bivector, e.g. inverse metric tensor |
|
n-vector, a sum of n-blades |
|
| m = 1 |
covector, linear functional, 1-form (e.g. gradient of a scalar field) |
linear transformation, Kronecker delta |
|
|
|
|
| m = 2 |
bilinear form, e.g. inner product, metric tensor, Ricci curvature, 2-form, symplectic form |
e.g. cross product in three dimensions |
e.g. elasticity tensor |
|
|
|
| m = 3 |
e.g. 3-form |
e.g. Riemann curvature tensor |
|
|
|
|
| ... |
|
|
|
|
|
|
| m = M |
e.g. M-form i.e. volume form |
|
|
|
|
|
| ... |
|
|
|
|
|
|
Raising an index on an
(n, m)-tensor produces an
(n + 1, m − 1)-tensor;
this can be visualized as moving diagonally up and to the right on the
table. Symmetrically, lowering an index can be visualized as moving
diagonally down and to the left on the table.
Contraction of an upper with a lower index of an
(n, m)-tensor produces an
(n − 1, m − 1)-tensor; this can be visualized as moving diagonally up and to the left on the table.
Orientation defined by an ordered set of vectors.
Reversed orientation corresponds to negating the exterior product.
Geometric interpretation of grade
n elements in a real
exterior algebra for
n = 0 (signed point), 1 (directed line segment, or vector), 2 (oriented plane element), 3 (oriented volume). The exterior product of
n vectors can be visualized as any
n-dimensional shape (e.g.
n-
parallelotope,
n-
ellipsoid); with magnitude (
hypervolume), and
orientation defined by that on its
n − 1-dimensional boundary and on which side the interior is.
[6][7]
Notation
Ricci calculus
Ricci calculus is the modern formalism and notation for tensor indices: indicating
inner and
outer products,
covariance and contravariance,
summations of tensor components,
symmetry and
antisymmetry, and
partial and
covariant derivatives.
Einstein summation convention
The
Einstein summation convention dispenses with writing
summation signs, leaving the summation implicit. Any repeated index symbol is summed over: if the index
i is used twice in a given term of a tensor expression, it means that the term is to be summed for all
i. Several distinct pairs of indices may be summed this way.
Penrose graphical notation
Penrose graphical notation
is a diagrammatic notation which replaces the symbols for tensors with
shapes, and their indices by lines and curves. It is independent of
basis elements, and requires no symbols for the indices.
Abstract index notation
The
abstract index notation is a way to write tensors such that the indices are no longer thought of as numerical, but rather are
indeterminates. This notation captures the expressiveness of indices and the basis-independence of index-free notation.
Component-free notation
A
component-free treatment of tensors uses notation that emphasises that tensors do not rely on any basis, and is defined in terms of the
tensor product of vector spaces.
Operations
There are a number of basic operations that may be conducted on
tensors that again produce a tensor.
The linear nature of tensor implies
that two tensors of the same type may be added together, and that
tensors may be multiplied by a scalar with results analogous to the
scaling of a vector.
On components, these operations are simply performed component for
component. These operations do not change the type of the tensor,
however there also exist operations that change the type of the tensors.
Tensor product
The
tensor product takes two tensors,
S and
T, and produces a new tensor,
S ⊗ T,
whose order is the sum of the orders of the original tensors. When
described as multilinear maps, the tensor product simply multiplies the
two tensors, i.e.
which again produces a map that is linear in all its arguments. On
components the effect similarly is to multiply the components of the two
input tensors, i.e.
If
S is of type (
l,
k) and
T is of type (
n,
m), then the tensor product
S ⊗ T has type
(l+n,k+m).
Contraction
Tensor contraction is an operation that reduces the total order of a tensor by two. More precisely, it reduces a type
(n, m) tensor to a type
(n − 1, m − 1)
tensor. In terms of components, the operation is achieved by summing
over one contravariant and one covariant index of tensor. For example, a
(1, 1)-tensor
can be contracted to a scalar through
.
Where the summation is again implied. When the
(1, 1)-tensor is interpreted as a linear map, this operation is known as the
trace.
The contraction is often used in conjunction with the tensor product to contract an index from each tensor.
The contraction can also be understood in terms of the definition of a
tensor as an element of a tensor product of copies of the space
V with the space
V* by first decomposing the tensor into a linear combination of simple tensors, and then applying a factor from
V* to a factor from
V. For example, a tensor
can be written as a linear combination
The contraction of
T on the first and last slots is then the vector
Raising or lowering an index
When a vector space is equipped with a
nondegenerate bilinear form (or
metric tensor
as it is often called in this context), operations can be defined that
convert a contravariant (upper) index into a covariant (lower) index and
vice versa. A metric tensor is a (symmetric) (
0, 2)-tensor,
it is thus possible to contract an upper index of a tensor with one of
lower indices of the metric tensor in the product. This produces a new
tensor with the same index structure as the previous, but with lower
index in the position of the contracted upper index. This operation is
quite graphically known as
lowering an index.
Conversely, the inverse operation can be defined, and is called
raising an index. This is equivalent to a similar contraction on the product with a
(2, 0)-tensor. This
inverse metric tensor has components that are the matrix inverse of those if the metric tensor.
Applications
Continuum mechanics
Important examples are provided by continuum mechanics. The stresses inside a
solid body or
fluid are described by a tensor. The
stress tensor and
strain tensor are both second-order tensors, and are related in a general linear elastic material by a fourth-order
elasticity tensor.
In detail, the tensor quantifying stress in a 3-dimensional solid
object has components that can be conveniently represented as a 3 × 3
array. The three faces of a cube-shaped infinitesimal volume segment of
the solid are each subject to some given force. The force's vector
components are also three in number.
Thus, 3 × 3, or 9 components are
required to describe the stress at this cube-shaped infinitesimal
segment. Within the bounds of this solid is a whole mass of varying
stress quantities, each requiring 9 quantities to describe. Thus, a
second-order tensor is needed.
If a particular
surface element
inside the material is singled out, the material on one side of the
surface will apply a force on the other side. In general, this force
will not be orthogonal to the surface, but it will depend on the
orientation of the surface in a linear manner. This is described by a
tensor of
type (2, 0), in
linear elasticity, or more precisely by a tensor field of type
(2, 0), since the stresses may vary from point to point.
Other examples from physics
Common applications include
Applications of tensors of order > 2
The concept of a tensor of order two is often conflated with that of a
matrix. Tensors of higher order do however capture ideas important in
science and engineering, as has been shown successively in numerous
areas as they develop. This happens, for instance, in the field of
computer vision, with the
trifocal tensor generalizing the
fundamental matrix.
The field of
nonlinear optics studies the changes to material
polarization density under extreme electric fields. The polarization waves generated are related to the generating
electric fields through the nonlinear susceptibility tensor. If the polarization
P is not linearly proportional to the electric field
E, the medium is termed
nonlinear. To a good approximation (for sufficiently weak fields, assuming no permanent dipole moments are present),
P is given by a
Taylor series in
E whose coefficients are the nonlinear susceptibilities:
Here
is the linear susceptibility,
gives the
Pockels effect and
second harmonic generation, and
gives the
Kerr effect. This expansion shows the way higher-order tensors arise naturally in the subject matter.
Generalizations
Tensors in infinite dimensions
The notion of a tensor can be generalized in a variety of ways to
infinite dimensions. One, for instance, is via the
tensor product of
Hilbert spaces.
[8] Another way of generalizing the idea of tensor, common in
nonlinear analysis, is via the
multilinear maps definition where instead of using finite-dimensional vector spaces and their
algebraic duals, one uses infinite-dimensional
Banach spaces and their
continuous dual.
[9] Tensors thus live naturally on
Banach manifolds.
[10]
Tensor densities
The concept of a
tensor field
can be generalized by considering objects that transform differently.
An object that transforms as an ordinary tensor field under coordinate
transformations, except that it is also multiplied by the determinant of
the
Jacobian of the inverse coordinate transformation to the
power, is called a tensor density with weight
.
[11] Invariantly, in the language of multilinear algebra, one can think of tensor densities as
multilinear maps taking their values in a
density bundle such as the (1-dimensional) space of
n-forms (where
n is the dimension of the space), as opposed to taking their values in just
R. Higher "weights" then just correspond to taking additional tensor products with this space in the range.
A special case are the scalar densities. Scalar 1-densities are
especially important because it makes sense to define their integral
over a manifold. They appear, for instance, in the
Einstein–Hilbert action in general relativity. The most common example of a scalar 1-density is the
volume element, which in the presence of a metric tensor
g is the square root of its
determinant in coordinates, denoted
. The metric tensor is a covariant tensor of order 2, and so its determinant scales by the square of the coordinate transition:
which is the transformation law for a scalar density of weight +2.
More generally, any tensor density is the product of an ordinary
tensor with a scalar density of the appropriate weight. In the language
of
vector bundles, the determinant bundle of the
tangent bundle is a
line bundle that can be used to 'twist' other bundles
w
times. While locally the more general transformation law can indeed be
used to recognise these tensors, there is a global question that arises,
reflecting that in the transformation law one may write either the
Jacobian determinant, or its absolute value. Non-integral powers of the
(positive) transition functions of the bundle of densities make sense,
so that the weight of a density, in that sense, is not restricted to
integer values. Restricting to changes of coordinates with positive
Jacobian determinant is possible on
orientable manifolds,
because there is a consistent global way to eliminate the minus signs;
but otherwise the line bundle of densities and the line bundle of
n-forms are distinct. For more on the intrinsic meaning, see
density on a manifold.
Spinors
When changing from one
orthonormal basis (called a
frame)
to another by a rotation, the components of a tensor transform by that
same rotation. This transformation does not depend on the path taken
through the space of frames. However, the space of frames is not
simply connected (see
orientation entanglement and
plate trick):
there are continuous paths in the space of frames with the same
beginning and ending configurations that are not deformable one into the
other. It is possible to attach an additional discrete invariant to
each frame called the "spin" that incorporates this path dependence, and
which turns out to have values of ±1. A
spinor
is an object that transforms like a tensor under rotations in the
frame, apart from a possible sign that is determined by the spin.
History
The concepts of later tensor analysis arose from the work of
Carl Friedrich Gauss in differential geometry, and the formulation was much influenced by the theory of
algebraic forms and invariants developed during the middle of the nineteenth century.
[12] The word "tensor" itself was introduced in 1846 by
William Rowan Hamilton[13] to describe something different from what is now meant by a tensor.
[Note 6] The contemporary usage was introduced by
Woldemar Voigt in 1898.
[14]
Tensor calculus was developed around 1890 by
Gregorio Ricci-Curbastro under the title
absolute differential calculus, and originally presented by Ricci in 1892.
[15] It was made accessible to many mathematicians by the publication of Ricci and
Tullio Levi-Civita's 1900 classic text
Méthodes de calcul différentiel absolu et leurs applications (Methods of absolute differential calculus and their applications).
[16]
In the 20th century, the subject came to be known as
tensor analysis, and achieved broader acceptance with the introduction of
Einstein's theory of
general relativity,
around 1915. General relativity is formulated completely in the
language of tensors. Einstein had learned about them, with great
difficulty, from the geometer
Marcel Grossmann.
[17]
Levi-Civita then initiated a correspondence with Einstein to correct
mistakes Einstein had made in his use of tensor analysis. The
correspondence lasted 1915–17, and was characterized by mutual respect:
I admire the elegance of your method of computation; it must be nice
to ride through these fields upon the horse of true mathematics while
the like of us have to make our way laboriously on foot.
—Albert Einstein,
The Italian Mathematicians of Relativity[18]
Tensors were also found to be useful in other fields such as
continuum mechanics. Some well-known examples of tensors in
differential geometry are
quadratic forms such as
metric tensors, and the
Riemann curvature tensor. The
exterior algebra of
Hermann Grassmann,
from the middle of the nineteenth century, is itself a tensor theory,
and highly geometric, but it was some time before it was seen, with the
theory of
differential forms, as naturally unified with tensor calculus. The work of
Élie Cartan made differential forms one of the basic kinds of tensors used in mathematics.
From about the 1920s onwards, it was realised that tensors play a basic role in
algebraic topology (for example in the
Künneth theorem).
[19] Correspondingly there are types of tensors at work in many branches of
abstract algebra, particularly in
homological algebra and
representation theory. Multilinear algebra can be developed in greater generality than for scalars coming from a
field. For example, scalars can come from a
ring. But the theory is then less geometric and computations more technical and less algorithmic.
[20] Tensors are generalized within
category theory by means of the concept of
monoidal category, from the 1960s.
[21]
results in a molecule indistinguishable from the original. This is also called an n-fold rotational axis and abbreviated Cn. Examples are the C2 in water and the C3 in ammonia. A molecule can have more than one symmetry axis; the one with the highest n is called the principal axis, and by convention is assigned the z-axis in a Cartesian coordinate system.
is a differential operator defined over a vector field
