Four-tensor

In special relativity, one of the simplest non-trivial examples of a four-tensor is the four-displacement

${\displaystyle x^{\mu }=(x^{0},x^{1},x^{2},x^{3})\,,}$

a four-tensor with contravariant rank 1 and covariant rank 0. Four-tensors of this kind are usually known as four-vectors. Here the component x⁰ = ct gives the displacement of a body in time (coordinate time t is multiplied by the speed of light c so that x⁰ has dimensions of length). The remaining components of the four-displacement form the spatial displacement vector x = (x¹, x², x³).[1]

The four-momentum for massive or massless particles is

${\displaystyle p^{\mu }=\left(E/c,p_{x},p_{y},p_{z}\right)}$

combines its energy (divided by c) p⁰ = E/c and 3-momentum p = (p¹, p², p³).[1]

For a particle with relativistic mass m, four momentum is defined by

${\displaystyle p^{\mu }=m{\frac {dx^{\mu }}{d\tau }}}$

with τ the proper time of the particle.

The Minkowski metric tensor with an orthonormal basis for the (−+++) convention is

${\displaystyle \eta ^{\mu \nu }={\begin{pmatrix}-1&0&0&0\\0&1&0&0\\0&0&1&0\\0&0&0&1\end{pmatrix}}\,}$

used for calculating the line element and raising and lowering indices. The above applies to Cartesian coordinates. In general relativity, the metric tensor is given by much more general expressions for curvilinear coordinates.

The angular momentum L = x ∧ p of a particle with relativistic mass m and relativistic momentum p (as measured by an observer in a lab frame) combines with another vector quantity N = mx − pt (without a standard name) in the relativistic angular momentum tensor[2][3]

${\displaystyle M^{\mu \nu }={\begin{pmatrix}0&-N^{1}c&-N^{2}c&-N^{3}c\\N^{1}c&0&L^{12}&-L^{31}\\N^{2}c&-L^{12}&0&L^{23}\\N^{3}c&L^{31}&-L^{23}&0\end{pmatrix}}}$

with components

${\displaystyle M^{\alpha \beta }=X^{\alpha }P^{\beta }-X^{\beta }P^{\alpha }}$

The stress–energy tensor of a continuum or field generally takes the form of a second order tensor, and usually denoted by T. The timelike component corresponds to energy density (energy per unit volume), the mixed spacetime components to momentum density (momentum per unit volume), and the purely spacelike parts to 3d stress tensors.

The electromagnetic field tensor combines the electric field and E and magnetic field B[4]

${\displaystyle F^{\mu \nu }={\begin{pmatrix}0&-E_{x}/c&-E_{y}/c&-E_{z}/c\\E_{x}/c&0&-B_{z}&B_{y}\\E_{y}/c&B_{z}&0&-B_{x}\\E_{z}/c&-B_{y}&B_{x}&0\end{pmatrix}}}$

The electromagnetic displacement tensor combines the electric displacement field D and magnetic field intensity H as follows[5]

${\displaystyle {\mathcal {D}}^{\mu \nu }={\begin{pmatrix}0&-D_{x}c&-D_{y}c&-D_{z}c\\D_{x}c&0&-H_{z}&H_{y}\\D_{y}c&H_{z}&0&-H_{x}\\D_{z}c&-H_{y}&H_{x}&0\end{pmatrix}}.}$

The magnetization-polarization tensor combines the P and M fields[4]

${\displaystyle {\mathcal {M}}^{\mu \nu }={\begin{pmatrix}0&P_{x}c&P_{y}c&P_{z}c\\-P_{x}c&0&-M_{z}&M_{y}\\-P_{y}c&M_{z}&0&-M_{x}\\-P_{z}c&-M_{y}&M_{x}&0\end{pmatrix}},}$

The three field tensors are related by

${\displaystyle {\mathcal {D}}^{\mu \nu }={\frac {1}{\mu _{0}}}F^{\mu \nu }-{\mathcal {M}}^{\mu \nu }\,}$

which is equivalent to the definitions of the D and H fields.

The electric dipole moment d and magnetic dipole moment μ of a particle are unified into a single tensor[6]

${\displaystyle \sigma ^{\mu \nu }={\begin{pmatrix}0&d_{x}&d_{y}&d_{z}\\-d_{x}&0&\mu _{z}/c&-\mu _{y}/c\\-d_{y}&-\mu _{z}/c&0&\mu _{x}/c\\-d_{z}&\mu _{y}/c&-\mu _{x}/c&0\end{pmatrix}},}$

The Ricci curvature tensor is another second order tensor.

In general relativity, there are curvature tensors which tend to be higher order, such as the Riemann curvature tensor and Weyl curvature tensor which are both fourth order tensors.