Sunday, 25 September 2011

Lorentz Transformation

Lorentz Transformation
A Lorentz transformation is a four-dimensional transformation
 x^('mu)=Lambda^mu_nux^nu,
(1)
satisfied by all four-vectors x^nu, where Lambda^mu_nu is a so-called Lorentz tensor. Lorentz tensors are restricted by the conditions
 Lambda^alpha_gammaLambda^beta_deltaeta_(alphabeta)=eta_(gammadelta),
(2)
with eta_(alphabeta) the Minkowski metric (Weinberg 1972, p. 26; Misner et al. 1973, p. 68).
Here, the tensor indices run over 0, 1, 2, 3, with x^0 being the time coordinate and (x^1,x^2,x^3) are space coordinates, and Einstein summation is used to sum over repeated indices. There are a number of conventions, but a common one used by Weinberg (1972) is to take the speed of light c=1 to simplify computations allow ct to be written simply as t for x^0. The group of Lorentz transformations in Minkowski space R^((3,1)) is known as the Lorentz group.
Note that while some authors (e.g., Weinberg 1972, p. 26) use the term "Lorentz transformation" to refer to the inhomogeneous transformation
 x^'^mu=Lambda^mu_nux^nu+a^mu,
(3)
where a^mu is a constant tensor, the preferred term for transformations of this form is Poincaré transformation (Misner et al. 1973, p. 68). The corresponding group of Poincaré transformations is known as the Poincaré group.
In the theory of special relativity, the Lorentz transformation replaces the Galilean transformation as the valid transformation law between reference frames moving with respect to one another at constant velocity. The Lorentz transformation serves this important role by virtue of the fact that it leaves the so-called proper time
dtau^2=dt^2-dx^2
(4)
=-eta_(alphabeta)dx^alphadx^beta
(5)
invariant. (Here, the convention c=1 is used.) To see this, note that
dtau^('2)=-eta_(alphabeta)dx^('alpha)dx^('beta)
(6)
=-eta_(alphabeta)Lambda^alpha_gammaLambda^beta_deltadx^gammadx^delta
(7)
=-eta_(gammadelta)dx^gammadx^delta
(8)
=dtau^2
(9)
(Weinberg 1972, p. 27).
The set of all Lorentz transformations is known as the inhomogeneous Lorentz group or the Poincaré group. Similarly, the set of Lorentz transformations with a^alpha=0 is known as the homogeneous Lorentz group. Restricting the transformations by the additional requirements
 Lambda^0_0>=1
(10)
and
 Tr(Lambda)=1,
(11)
where Tr(Lambda) denotes the tensor trace, give the proper inhomogeneous and proper homogeneous Lorentz groups.
Any proper homogeneous Lorentz transformation can be expressed as a product of a so-called boost and a rotation.

REFERENCES:
Fraundorf, P. "Accel-1D: Frame-Dependent Relativity at UM-StL." http://www.umsl.edu/~fraundor/a1toc.html.
Griffiths, D. J. Introduction to Electrodynamics. Englewood Cliffs, NJ: Prentice-Hall, pp. 412-414, 1981.
Misner, C. W.; Thorne, K. S.; and Wheeler, J. A. Gravitation. San Francisco: W. H. Freeman, 1973.
Morse, P. M. and Feshbach, H. "The Lorentz Transformation, Four-Vectors, Spinors." §1.7 in Methods of Theoretical Physics, Part I. New York: McGraw-Hill, pp. 93-107, 1953.
Weinberg, S. "Lorentz Transformations." §2.1 in Gravitation and Cosmology: Principles and Applications of the General Theory of Relativity. New York: Wiley, pp. 25-29, 1972.