In a given coordinate system , the spacetime interval between two Events and with coordinates and ( respectively is given by:
:
and is an Invariant .:
:
i.e.,
where is the Minkowski Metric
:
and the Einstein Summation Convention is being used. From this relation follows the linearity of the coordinate transformation:
:
where and satisfy:
:
:
:
Such a transformation is called a Poincaré Transformation . The represents a space-time translation; when , the transformation is a Lorentz transformation.
Taking the determinant of the first equation gives
Lorentz transformations with are called and consist of spatial rotations and boosts. Those with are called '''improper Lorentz transformations''' and consist of (discrete) space and time reflections.
A quantity invariant under Lorentz transformations is known as a Lorentz Scalar .
Given two observers and , each using a Cartesian coordinate system to measure space and time intervals, and , assume that the coordinate systems are oriented so that the relative velocity of and is ''v'' along the common - axis with parallel (but not common) and axes (same for the and axes). Also, assume that their origins meet at the common time ==0. Then the frames are said to be in (SC). The Lorentz transformation for frames in SC Can Be Shown to be:
:
:
:
:
:::where
:::: is the X Component (in ) of the position of a point (or object) stationary relative to ''observer '',
:::: is the ''x component'' (in ) of the position of the same point (or object) that is stationary relative to ''observer '' (moving with respect to ),
:::: is the time since time zero (in ) of ''observer '',
:::: is the time since time zero (in ) of ''observer '' (as seen by ''observer ''),
:::: and are both the ''y component'' of the position of a point in both reference frames (same with and ),
:::: is called the Lorentz Factor ,
:::: is the Speed Of Light in a vacuum, and
:::: is the relative velocity between the two observers.
This Lorentz transformation is called a ''boost in the x-direction'' and is often expressed in Matrix form as
:
where the coordinate is replaced by (and similarly for ).
The Lorentz transformations in SC may be cast into a more useful form by introducing a parameter called the or '''hyperbolic parameter''' through the equation:
:
The Lorentz transformations in SC are then:
:
:
:
:
|
:
These equations can be expressed in matrix form as
:
,
where
is the identity matrix.
The composition of two Lorentz transformations is a Lorentz transformation and the set of all Lorentz transformations with the operation of composition forms a group called the
Lorentz Group .
Under the
Erlangen Program ,
Minkowski Space can be viewed as the
Geometry defined by the
Poincaré Group , which combines Lorentz transformations with translations.
One of the most astounding predictions of special relativity was the idea that time is relative. In essence, each observer's frame of reference is associated with a unique clock, the result being that time passes at different rates for different observers. This was a direct prediction from the Lorentz transformations and is called
Time Dilation . Time dilation was also used to prove that
Simultaneity varies between
Reference Frame s.
Lorentz transformations can also be used to prove that magnetic and electric fields are the same force. The reason they are interpreted differently is due to Lorentz transformations done on the charges moving relative to the observer. Changing reference frames shows that an electric field will look like both a magnetic and electric field to a moving observer. There also exist frames in which a magnetic and electric field can be observed as a single magnetic, or electric field.
For relative speeds much less than the speed of light, the Lorentz transformations reduce to the
Galilean Transformation in accordance with the
Correspondence Principle . The correspondence limit is usually stated mathematically as
.
The transformations were first discovered and published by
Joseph Larmor in 1897, although
Woldemar Voigt had published a slightly different version of them in 1887, for which he showed that Maxwell's equations were invariant. In 1905,
Henri Poincaré named them after the
Dutch Physicist and
Mathematician Hendrik Antoon Lorentz (
1853 -
1928 ) who had published a first order version of these transformations in the 1890s and the final version in 1899 and 1904. The development of these transformations was encouraged by the null result of the
Michelson-Morley Experiment .
The Lorentz transformations were published in 1897 and 1900 by
Joseph Larmor and by
Hendrik Lorentz in 1899 and 1904. Voigt (1887) had published a form of the equations
:
which incorporated
Relativity Of Simultaneity ("local time") and
Time Dilation . For Voigt, clocks ran slower by the factor
which is greater than the now accepted value of
predicted by Larmor (1897). Note that Voigt equations have a length expansion in the transverse direction. Voigt derived these transformations as those which would make the speed of light the same in all reference frames. Lorentz believed Voigt's transformations were equivalent to his (apparently not seeing the significance of the different time dilation) and wrote
:"In a paper which to my regret has escaped my notice all these years, Voigt has applied a transformation equivalent to
Lorentz treansformation . The idea of the transformations used above might therefore have been borrowed form Voigt and the proof that it does not alter the form of the equations for the free ether is contained in his paper" (Lorentz 1913)
In a similar vein, Larmor and Lorentz, who believed the
Luminiferous Aether hypothesis,
were seeking the transformations under which Maxwell's equations were invariant when transformed from the ether to a moving frame.
Henri Poincaré in 1900 attributed the invention of local time to Lorentz and showed how Lorentz's first version of it (which applies to invariant clock rates) arose when clocks were sychronised by exchanging light signals which were assumed to travel at the same speed against and with the motion of the reference frame (see
Relativity Of Simultaneity ).
Larmor's (1897) and Lorentz's (1899, 1904) final equations were not in the modern notation and form, but were algebraically equivalent to those published (1905) by
Henri Poincaré , the French
Mathematician , who revised the form to make the four equations into the coherent, self-consistent whole we know today. Both Larmor and Lorentz discovered that the transformation preserved
Maxwell's Equations . Paul Langevin (1911) said of the transformation
:"It is the great merit of H. A. Lorentz to have seen that the fundamental equations of electromagnetism admit a group of transformations which enables them to have the same form when one passes from one frame of reference to another; this new transformation has the most profound implications for the transformations of space and time".
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