# Minkowski Space

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Related to Minkowski Space: Minkowski metric, Minkowski inequality

## Minkowski Space

a four-dimensional space, combining the physical three-dimensional space and time; introduced by H. Minkowski in 1907–08. Points in Minkowski space correspond to “events” of the special theory of relativity.

The position of an event in Minkowski space is specified by four coordinates—three space coordinates and one time coordinate. The coordinates that are usually used are x = x, x2 = y, x3 = z, where x, y, and z are rectangular Cartesian coordinates of the event in a given inertial frame of reference, and the coordinate xθ = ct, where t is the time of the event and c is the velocity of light. The imaginary time coordinate x4 = ix0 = ict can be introduced instead of X0.

It follows from the special theory of relativity that space and time are not independent. In passing from one inertial frame of reference to another, the space coordinates and the time are transformed through each other by Lorentz transformations. The introduction of Minkowski space permits the Lorentz transformation to be represented as the transformation of the coordinates x1, x2, x3, x4 of an event in a rotation of the four-dimensional coordinate system in this space.

The chief invariant of Minkowski space is the square of the length of the four-dimensional vector that connects two points—events—and that remains invariant in rotations in Minkowski space and equal in magnitude (but opposite in sign) to the square of the four-dimensional interval (sAB2) of the special theory of relativity:

(x1Ax1B)2 + (x2Ax2B)2 + (x3Ax3B)2 + (x4Ax4B)2 = (xAxB)2 + (yAyB)2 + (zAzB)2 + c2(tAtB)2 = −sAB2

where the subscripts A and B indicate the space coordinates and time of events A and B, respectively. The uniqueness of the geometry of Minkowski space is that this expression contains the squares of the components of a four-dimensional vector along the time and space axes with different signs (such a geometry is said to be pseudo-Euclidean, in contrast to Euclidean geometry in which the square of the distance between two points is determined by the sum of the squares of the components, on the corresponding axes, of the vector that joins the points). As a result, a four-dimensional vector with nonzero components can have zero length. This is the case for the vector that joins two events connected by a light signal:

(xAxB)2 + (yAyB)2 + (zAzB)2 + c2(tAtB)2 = c2(tA - tB)

The geometry of Minkowski space makes it possible to give a lucid interpretation of the kinematic effects of the special theory of relativity (for example, the variation in length and rate of passage of time in passing over from one inertial frame of reference to another). It also serves as the basis for the modern mathematical apparatus of the theory of relativity.

G. A. ZISMAN

References in periodicals archive ?
Minkowski spacetime or Minkowski space can be thought a combination of time dimension and Euclidean space into a four-dimensional manifold.
Timelike, spacelike, and lightlike vectors are important for the Minkowski space [E.sup.3.sub.1].
where a is the amplitude of a displacement vector in Minkowski space. If we consider the Hubble diameter as the maximum dimension of the local patch of space then a = [r.sub.HS] where [r.sub.HS] is the Hubble radius.
Juttler, "C 1 Hermite interpolation by Pythagorean hodograph quintics in Minkowski space," Advances in Computational Mathematics, vol.
The flat spacetime of relativity, called Minkowski space, distinguishes vectors into three categories space-like, light-like, and time-like.
The flat case, [M.sup.3.sub.r]([rho]) = [E.sup.3.sub.r], [rho] = 0, r = 0,1, corresponds to either R or the Minkowski space [R.sup.3.sub.1] = [L.sup.3].
Let S be a surface having a pseudo null base curve a in the 3-dimensional Minkowski space with parametrization (6).
of California-San Diego) investigate the global in time regularity of the Yang-Mills equations on high dimensional Minkowski space with compact matrix gauge group G.
Let us suppose that [alpha]* = [alpha]* (t*) is another differentiable spacelike curve with arc-length and {[V*.sub.1], [V*.sub.2], [V*.sub.3] is Frenet frame of this curve in three dimensional Minkowski space [R.sup.3.sub.1].
In Minkowski space we have the following relations:
Subjects of special relativity are treated in the chapter on Minkowski space, and subjects of general relativity appear in the chapters on curved spaces and include Einstein's equation, the Schwarzschild metric, the precession of Mercury, the bending of light, etc.

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