Four-vector

From Wikipedia, the free encyclopedia

In relativity, a four-vector is a vector in a four-dimensional real vector space, called Minkowski space. The usage of the four-vector name tacitly assumes that its components refer to a standard basis. The components transform between these bases as the space and time coordinate differences, $(Δ t,Δ x,Δ y,Δ z)$ under spatial translations, rotations, and boosts (a change by a constant velocity to another inertial reference frame). The set of all such translations, rotations, and boosts (called Poincaré transformations) forms the Poincaré group. The set of rotations and boosts (Lorentz transformations, described by 4×4 matrices) forms the Lorentz group.

1 Mathematics of four-vectors
2 Examples of four-vectors in dynamics
3 Physics of four-vectors
- 3.1 Deriving E = mc2
- 3.2 Deriving E2 = p2c2 + m2c4
4 Examples of four-vectors in electromagnetism
5 See also
6 References

[edit] Mathematics of four-vectors

A point in Minkowski space is called an "event" and is described in a standard basis by a set of four coordinates such as

$\mathbf{x} := \left(ct, x, y, z \right)$

for $μ$ = 0, 1, 2, 3, where c is the speed of light. These coordinates are the components of the position four-vector for the event.

The displacement four-vector is defined to be an "arrow" linking two events:

$\Delta \mathbf{x}:= \left(\Delta ct, \Delta x, \Delta y, \Delta z \right)$

(Note that the position vector is the displacement vector when one of the two events is the origin of the coordinate system. Position vectors are relatively trivial; the general theory of four-vectors is concerned with displacement vectors.) The inner product of two four-vectors $u$ and $v$ is defined (using Einstein notation) as

$u \cdot v = u^{\mu} \eta_{\mu \nu} v^{\nu} = \left( \begin{matrix}u^0 & u^1 & u^2 & u^3 \end{matrix} \right) \left( \begin{matrix} 1 & 0 & 0 & 0 \\ 0 & -1 & 0 & 0 \\ 0 & 0 & -1 & 0 \\ 0 & 0 & 0 & -1 \end{matrix} \right) \left( \begin{matrix}v^0 \\ v^1 \\ v^2 \\ v^3 \end{matrix} \right) = u^0 v^0 - u^1 v^1 - u^2 v^2 - u^3 v^3$

where η is the Minkowski metric. Sometimes this inner product is called the Minkowski inner product.

The inner product is often expressed as the effect of the dual vector of one vector on the other:

$u \cdot v = u^*(v) = u{_\nu}v^{\nu}$

Here the $u ν$ -s are the components of the dual vector $u *$ of $u$ in the dual basis and called the covariant coordinates of $u$ , while the original $u ν$ components are called the contravariant coordinates. Lower and upper indices indicate always covariant and contravariant coordinates, respectively.

The relation between the covariant and contravariant coordinates is:

$u_{\mu} = u^{\nu} \eta_{\mu \nu} \,$ .

The four-vectors are arrows on the spacetime diagram or Minkowski diagram.

Four-vectors may be classified as either spacelike, timelike or null. In this article, four-vectors will be referred to simply as vectors. Spacelike, timelike, and null vectors are ones whose inner product with themselves is greater than, less than, and equal to zero respectively.

[edit] Examples of four-vectors in dynamics

When considering physical phenomena, differential equations arise naturally; however, when considering space and time derivatives of functions, it is unclear which reference frame these derivatives are taken with respect to. It is agreed that time derivatives are taken with respect to the proper time (τ) in the given reference frame. It is then important to find a relation between this time derivative and another time derivative (taken in another inertial reference frame). This relation is provided by the time transformation in the Lorentz transformations and is:

$\frac{d \tau}{dt}=\frac{1}{\gamma}$

where γ is the Lorentz factor. Important four-vectors in relativity theory can now be defined, such as the four-velocity of an $\mathbf{x}(\tau)$ world line is defined by:

$\mathbf{U} := \frac{d\mathbf{x}}{d \tau}= \frac{d\mathbf{x}}{dt}\frac{dt}{d \tau}= \left(\gamma c, \gamma \mathbf{u} \right)$

where

$u^i = \frac{dx^i}{dt}$

for i = 1, 2, 3. Notice that

$|| \mathbf{U} ||^2 = U^{\mu} U_{\mu} = c^2 \,$

The four-acceleration is given by:

$A =\frac{dU }{d \tau} = \left(\gamma \dot{\gamma} c, \gamma \dot{\gamma} \mathbf{u} + \gamma^2 \mathbf{\dot{u}} \right)$

Since the magnitude $\sqrt{ | U_\mu U^\mu | }$ of $\mathbf{U}$ is a constant, the four acceleration is (pseudo-)orthogonal to the four velocity, i.e. the Minkowski inner product of the four-acceleration and the four-velocity is zero:

$A_\mu U^\mu =\frac{1}{2} \frac{\partial (U^\mu U_\mu)}{\partial \tau } = 0 \,$

which is true for all world lines.

The four-momentum is for a massive particle is given by:

$p :=m U = \left(\gamma mc, \mathbf{p} \right)$

where m is the invariant mass of the particle.

The four-force is defined by:

$F := m A = \left(\gamma \dot{\gamma} mc, \gamma \mathbf{f} \right)$

where

$\mathbf{f} = \frac{d\mathbf{p}}{dt} = m \dot{\gamma} \mathbf{u} + m \gamma \mathbf{\dot{u}}$ .

[edit] Physics of four-vectors

The power and elegance of the four-vector formalism may be demonstrated by deriving some important relations between the physical quantities energy, mass and momentum.

[edit] Deriving E = mc²

Here, an expression for the total energy of a particle will be derived. The kinetic energy (K) of a particle is defined analogously to the classical definition, namely as

$\frac{dK}{dt}= \mathbf{f} \cdot \mathbf{u}$