HOME

TheInfoList



OR:

In
physics Physics is the scientific study of matter, its Elementary particle, fundamental constituents, its motion and behavior through space and time, and the related entities of energy and force. "Physical science is that department of knowledge whi ...
, the Lorentz transformations are a six-parameter family of
linear In mathematics, the term ''linear'' is used in two distinct senses for two different properties: * linearity of a '' function'' (or '' mapping''); * linearity of a '' polynomial''. An example of a linear function is the function defined by f(x) ...
transformations from a coordinate frame in
spacetime In physics, spacetime, also called the space-time continuum, is a mathematical model that fuses the three dimensions of space and the one dimension of time into a single four-dimensional continuum. Spacetime diagrams are useful in visualiz ...
to another frame that moves at a constant
velocity Velocity is a measurement of speed in a certain direction of motion. It is a fundamental concept in kinematics, the branch of classical mechanics that describes the motion of physical objects. Velocity is a vector (geometry), vector Physical q ...
relative to the former. The respective inverse transformation is then parameterized by the negative of this velocity. The transformations are named after the Dutch
physicist A physicist is a scientist who specializes in the field of physics, which encompasses the interactions of matter and energy at all length and time scales in the physical universe. Physicists generally are interested in the root or ultimate cau ...
Hendrik Lorentz. The most common form of the transformation, parametrized by the real constant v, representing a velocity confined to the -direction, is expressed as \begin t' &= \gamma \left( t - \frac \right) \\ x' &= \gamma \left( x - v t \right)\\ y' &= y \\ z' &= z \end where and are the coordinates of an event in two frames with the spatial origins coinciding at , where the primed frame is seen from the unprimed frame as moving with speed along the -axis, where is the
speed of light The speed of light in vacuum, commonly denoted , is a universal physical constant exactly equal to ). It is exact because, by international agreement, a metre is defined as the length of the path travelled by light in vacuum during a time i ...
, and \gamma = \frac is the
Lorentz factor The Lorentz factor or Lorentz term (also known as the gamma factor) is a dimensionless quantity expressing how much the measurements of time, length, and other physical properties change for an object while it moves. The expression appears in sev ...
. When speed is much smaller than , the Lorentz factor is negligibly different from 1, but as approaches , \gamma grows without bound. The value of must be smaller than for the transformation to make sense. Expressing the speed as a fraction of the speed of light, \beta = v/c, an equivalent form of the transformation is \begin ct' &= \gamma \left( c t - \beta x \right) \\ x' &= \gamma \left( x - \beta ct \right) \\ y' &= y \\ z' &= z. \end Frames of reference can be divided into two groups: inertial (relative motion with constant velocity) and non-inertial (accelerating, moving in curved paths, rotational motion with constant
angular velocity In physics, angular velocity (symbol or \vec, the lowercase Greek letter omega), also known as the angular frequency vector,(UP1) is a pseudovector representation of how the angular position or orientation of an object changes with time, i ...
, etc.). The term "Lorentz transformations" only refers to transformations between ''inertial'' frames, usually in the context of special relativity. In each reference frame, an observer can use a local coordinate system (usually
Cartesian coordinates In geometry, a Cartesian coordinate system (, ) in a plane is a coordinate system that specifies each point uniquely by a pair of real numbers called ''coordinates'', which are the signed distances to the point from two fixed perpendicular o ...
in this context) to measure lengths, and a clock to measure time intervals. An event is something that happens at a point in space at an instant of time, or more formally a point in
spacetime In physics, spacetime, also called the space-time continuum, is a mathematical model that fuses the three dimensions of space and the one dimension of time into a single four-dimensional continuum. Spacetime diagrams are useful in visualiz ...
. The transformations connect the space and time coordinates of an event as measured by an observer in each frame.One can imagine that in each inertial frame there are observers positioned throughout space, each with a synchronized clock and at rest in the particular inertial frame. These observers then report to a central office, where all reports are collected. When one speaks of a ''particular'' observer, one refers to someone having, at least in principle, a copy of this report. See, e.g., . They supersede the Galilean transformation of
Newtonian physics Classical mechanics is a physical theory describing the motion of objects such as projectiles, parts of machinery, spacecraft, planets, stars, and galaxies. The development of classical mechanics involved substantial change in the methods ...
, which assumes an
absolute space and time Absolute space and time is a concept in physics and philosophy about the properties of the universe. In physics, absolute space and time may be a preferred frame. Early concept A version of the concept of absolute space (in the sense of a prefe ...
(see Galilean relativity). The Galilean transformation is a good approximation only at relative speeds much less than the speed of light. Lorentz transformations have a number of unintuitive features that do not appear in Galilean transformations. For example, they reflect the fact that observers moving at different velocities may measure different distances, elapsed times, and even different orderings of events, but always such that the
speed of light The speed of light in vacuum, commonly denoted , is a universal physical constant exactly equal to ). It is exact because, by international agreement, a metre is defined as the length of the path travelled by light in vacuum during a time i ...
is the same in all inertial reference frames. The invariance of light speed is one of the postulates of special relativity. Historically, the transformations were the result of attempts by Lorentz and others to explain how the speed of
light Light, visible light, or visible radiation is electromagnetic radiation that can be visual perception, perceived by the human eye. Visible light spans the visible spectrum and is usually defined as having wavelengths in the range of 400– ...
was observed to be independent of the reference frame, and to understand the symmetries of the laws of
electromagnetism In physics, electromagnetism is an interaction that occurs between particles with electric charge via electromagnetic fields. The electromagnetic force is one of the four fundamental forces of nature. It is the dominant force in the interacti ...
. The transformations later became a cornerstone for
special relativity In physics, the special theory of relativity, or special relativity for short, is a scientific theory of the relationship between Spacetime, space and time. In Albert Einstein's 1905 paper, Annus Mirabilis papers#Special relativity, "On the Ele ...
. The Lorentz transformation is a
linear transformation In mathematics, and more specifically in linear algebra, a linear map (also called a linear mapping, linear transformation, vector space homomorphism, or in some contexts linear function) is a mapping V \to W between two vector spaces that pr ...
. It may include a rotation of space; a rotation-free Lorentz transformation is called a Lorentz boost. In
Minkowski space In physics, Minkowski space (or Minkowski spacetime) () is the main mathematical description of spacetime in the absence of gravitation. It combines inertial space and time manifolds into a four-dimensional model. The model helps show how a ...
—the mathematical model of spacetime in special relativity—the Lorentz transformations preserve the spacetime interval between any two events. They describe only the transformations in which the spacetime event at the origin is left fixed. They can be considered as a hyperbolic rotation of Minkowski space. The more general set of transformations that also includes translations is known as the Poincaré group where initial time and initial origin coordinates of the two reference frames may differ, the two frames may have axes oriented differently and the direction of the speed between frames is arbitrary.


History

Many physicists—including Woldemar Voigt, George FitzGerald, Joseph Larmor, and Hendrik Lorentz himself—had been discussing the physics implied by these equations since 1887. Early in 1889, Oliver Heaviside had shown from
Maxwell's equations Maxwell's equations, or Maxwell–Heaviside equations, are a set of coupled partial differential equations that, together with the Lorentz force law, form the foundation of classical electromagnetism, classical optics, Electrical network, electr ...
that the
electric field An electric field (sometimes called E-field) is a field (physics), physical field that surrounds electrically charged particles such as electrons. In classical electromagnetism, the electric field of a single charge (or group of charges) descri ...
surrounding a spherical distribution of charge should cease to have
spherical symmetry In geometry, circular symmetry is a type of continuous symmetry for a planar object that can be rotated by any arbitrary angle and map onto itself. Rotational circular symmetry is isomorphic with the circle group in the complex plane, or the ...
once the charge is in motion relative to the
luminiferous aether Luminiferous aether or ether (''luminiferous'' meaning 'light-bearing') was the postulated Transmission medium, medium for the propagation of light. It was invoked to explain the ability of the apparently wave-based light to propagate through empt ...
. FitzGerald then conjectured that Heaviside's distortion result might be applied to a theory of intermolecular forces. Some months later, FitzGerald published the conjecture that bodies in motion are being contracted, in order to explain the baffling outcome of the 1887 aether-wind experiment of Michelson and Morley. In 1892, Lorentz independently presented the same idea in a more detailed manner, which was subsequently called FitzGerald–Lorentz contraction hypothesis. Their explanation was widely known before 1905. Lorentz (1892–1904) and Larmor (1897–1900), who believed the luminiferous aether hypothesis, also looked for the transformation under which
Maxwell's equations Maxwell's equations, or Maxwell–Heaviside equations, are a set of coupled partial differential equations that, together with the Lorentz force law, form the foundation of classical electromagnetism, classical optics, Electrical network, electr ...
are invariant when transformed from the aether to a moving frame. They extended the FitzGerald–Lorentz contraction hypothesis and found out that the time coordinate has to be modified as well (" local time").
Henri Poincaré Jules Henri Poincaré (, ; ; 29 April 185417 July 1912) was a French mathematician, Theoretical physics, theoretical physicist, engineer, and philosophy of science, philosopher of science. He is often described as a polymath, and in mathemati ...
gave a physical interpretation to local time (to first order in , the relative velocity of the two reference frames normalized to the speed of light) as the consequence of clock synchronization, under the assumption that the speed of light is constant in moving frames. Larmor is credited to have been the first to understand the crucial
time dilation Time dilation is the difference in elapsed time as measured by two clocks, either because of a relative velocity between them (special relativity), or a difference in gravitational potential between their locations (general relativity). When unsp ...
property inherent in his equations. In 1905, Poincaré was the first to recognize that the transformation has the properties of a mathematical group, and he named it after Lorentz. Later in the same year
Albert Einstein Albert Einstein (14 March 187918 April 1955) was a German-born theoretical physicist who is best known for developing the theory of relativity. Einstein also made important contributions to quantum mechanics. His mass–energy equivalence f ...
published what is now called
special relativity In physics, the special theory of relativity, or special relativity for short, is a scientific theory of the relationship between Spacetime, space and time. In Albert Einstein's 1905 paper, Annus Mirabilis papers#Special relativity, "On the Ele ...
, by deriving the Lorentz transformation under the assumptions of the
principle of relativity In physics, the principle of relativity is the requirement that the equations describing the laws of physics have the same form in all admissible frames of reference. For example, in the framework of special relativity, the Maxwell equations ...
and the constancy of the speed of light in any inertial reference frame, and by abandoning the mechanistic aether as unnecessary.


Derivation of the group of Lorentz transformations

An '' event'' is something that happens at a certain point in spacetime, or more generally, the point in spacetime itself. In any inertial frame an event is specified by a time coordinate and a set of Cartesian coordinates , , to specify position in space in that frame. Subscripts label individual events. From Einstein's second postulate of relativity (invariance of ) it follows that: in all inertial frames for events connected by ''light signals''. The quantity on the left is called the ''spacetime interval'' between events and . The interval between ''any two'' events, not necessarily separated by light signals, is in fact invariant, i.e., independent of the state of relative motion of observers in different inertial frames, as is shown using homogeneity and isotropy of space. The transformation sought after thus must possess the property that: where are the spacetime coordinates used to define events in one frame, and are the coordinates in another frame. First one observes that () is satisfied if an arbitrary -tuple of numbers are added to events and . Such transformations are called ''spacetime translations'' and are not dealt with further here. Then one observes that a ''linear'' solution preserving the origin of the simpler problem solves the general problem too: (a solution satisfying the first formula automatically satisfies the second one as well; see polarization identity). Finding the solution to the simpler problem is just a matter of look-up in the theory of
classical group In mathematics, the classical groups are defined as the special linear groups over the reals \mathbb, the complex numbers \mathbb and the quaternions \mathbb together with special automorphism groups of Bilinear form#Symmetric, skew-symmetric an ...
s that preserve
bilinear form In mathematics, a bilinear form is a bilinear map on a vector space (the elements of which are called '' vectors'') over a field ''K'' (the elements of which are called '' scalars''). In other words, a bilinear form is a function that is linea ...
s of various signature.The separate requirements of the three equations lead to three different groups. The second equation is satisfied for spacetime translations in addition to Lorentz transformations leading to the Poincaré group or the ''inhomogeneous Lorentz group''. The first equation (or the second restricted to lightlike separation) leads to a yet larger group, the
conformal group In mathematics, the conformal group of an inner product space is the group (mathematics), group of transformations from the space to itself that preserve angles. More formally, it is the group of transformations that preserve the conformal geometr ...
of spacetime.
First equation in () can be written more compactly as: where refers to the bilinear form of
signature A signature (; from , "to sign") is a depiction of someone's name, nickname, or even a simple "X" or other mark that a person writes on documents as a proof of identity and intent. Signatures are often, but not always, Handwriting, handwritt ...
on exposed by the right hand side formula in (). The alternative notation defined on the right is referred to as the ''relativistic dot product''. Spacetime mathematically viewed as endowed with this bilinear form is known as
Minkowski space In physics, Minkowski space (or Minkowski spacetime) () is the main mathematical description of spacetime in the absence of gravitation. It combines inertial space and time manifolds into a four-dimensional model. The model helps show how a ...
. The Lorentz transformation is thus an element of the group , the Lorentz group or, for those that prefer the other metric signature, (also called the Lorentz group).The groups and are isomorphic. It is widely believed that the choice between the two metric signatures has no physical relevance, even though some objects related to and respectively, e.g., the
Clifford algebra In mathematics, a Clifford algebra is an algebra generated by a vector space with a quadratic form, and is a unital associative algebra with the additional structure of a distinguished subspace. As -algebras, they generalize the real number ...
s corresponding to the different signatures of the bilinear form associated to the two groups, are non-isomorphic.
One has: which is precisely preservation of the bilinear form () which implies (by linearity of and bilinearity of the form) that () is satisfied. The elements of the Lorentz group are rotations and ''boosts'' and mixes thereof. If the spacetime translations are included, then one obtains the ''inhomogeneous Lorentz group'' or the Poincaré group.


Generalities

The relations between the primed and unprimed spacetime coordinates are the Lorentz transformations, each coordinate in one frame is a
linear function In mathematics, the term linear function refers to two distinct but related notions: * In calculus and related areas, a linear function is a function whose graph is a straight line, that is, a polynomial function of degree zero or one. For di ...
of all the coordinates in the other frame, and the
inverse function In mathematics, the inverse function of a function (also called the inverse of ) is a function that undoes the operation of . The inverse of exists if and only if is bijective, and if it exists, is denoted by f^ . For a function f\colon ...
s are the inverse transformation. Depending on how the frames move relative to each other, and how they are oriented in space relative to each other, other parameters that describe direction, speed, and orientation enter the transformation equations. Transformations describing relative motion with constant (uniform) velocity and without rotation of the space coordinate axes are called Lorentz boosts or simply ''boosts'', and the relative velocity between the frames is the parameter of the transformation. The other basic type of Lorentz transformation is rotation in the spatial coordinates only, these like boosts are inertial transformations since there is no relative motion, the frames are simply tilted (and not continuously rotating), and in this case quantities defining the rotation are the parameters of the transformation (e.g., axis–angle representation, or Euler angles, etc.). A combination of a rotation and boost is a ''homogeneous transformation'', which transforms the origin back to the origin. The full Lorentz group also contains special transformations that are neither rotations nor boosts, but rather reflections in a plane through the origin. Two of these can be singled out; spatial inversion in which the spatial coordinates of all events are reversed in sign and temporal inversion in which the time coordinate for each event gets its sign reversed. Boosts should not be conflated with mere displacements in spacetime; in this case, the coordinate systems are simply shifted and there is no relative motion. However, these also count as symmetries forced by special relativity since they leave the spacetime interval invariant. A combination of a rotation with a boost, followed by a shift in spacetime, is an ''inhomogeneous Lorentz transformation'', an element of the Poincaré group, which is also called the inhomogeneous Lorentz group.


Physical formulation of Lorentz boosts


Coordinate transformation

A "stationary" observer in frame defines events with coordinates , , , . Another frame moves with velocity relative to , and an observer in this "moving" frame defines events using the coordinates , , , . The coordinate axes in each frame are parallel (the and axes are parallel, the and axes are parallel, and the and axes are parallel), remain mutually perpendicular, and relative motion is along the coincident axes. At , the origins of both coordinate systems are the same, . In other words, the times and positions are coincident at this event. If all these hold, then the coordinate systems are said to be in standard configuration, or synchronized. If an observer in records an event , , , , then an observer in records the ''same'' event with coordinates where is the relative velocity between frames in the -direction, is the
speed of light The speed of light in vacuum, commonly denoted , is a universal physical constant exactly equal to ). It is exact because, by international agreement, a metre is defined as the length of the path travelled by light in vacuum during a time i ...
, and \gamma = \frac (lowercase
gamma Gamma (; uppercase , lowercase ; ) is the third letter of the Greek alphabet. In the system of Greek numerals it has a value of 3. In Ancient Greek, the letter gamma represented a voiced velar stop . In Modern Greek, this letter normally repr ...
) is the
Lorentz factor The Lorentz factor or Lorentz term (also known as the gamma factor) is a dimensionless quantity expressing how much the measurements of time, length, and other physical properties change for an object while it moves. The expression appears in sev ...
. Here, is the ''
parameter A parameter (), generally, is any characteristic that can help in defining or classifying a particular system (meaning an event, project, object, situation, etc.). That is, a parameter is an element of a system that is useful, or critical, when ...
'' of the transformation, for a given boost it is a constant number, but can take a continuous range of values. In the setup used here, positive relative velocity is motion along the positive directions of the axes, zero relative velocity is no relative motion, while negative relative velocity is relative motion along the negative directions of the axes. The magnitude of relative velocity cannot equal or exceed , so only subluminal speeds are allowed. The corresponding range of is . The transformations are not defined if is outside these limits. At the speed of light () is infinite, and
faster than light Faster-than-light (superluminal or supercausal) travel and communication are the conjectural propagation of matter or information faster than the speed of light in vacuum (). The special theory of relativity implies that only particles with zero ...
() is a
complex number In mathematics, a complex number is an element of a number system that extends the real numbers with a specific element denoted , called the imaginary unit and satisfying the equation i^= -1; every complex number can be expressed in the for ...
, each of which make the transformations unphysical. The space and time coordinates are measurable quantities and numerically must be real numbers. As an active transformation, an observer in notices the coordinates of the event to be "boosted" in the negative directions of the axes, because of the in the transformations. This has the equivalent effect of the ''coordinate system'' boosted in the positive directions of the axes, while the event does not change and is simply represented in another coordinate system, a passive transformation. The inverse relations (, , , in terms of , , , ) can be found by algebraically solving the original set of equations. A more efficient way is to use physical principles. Here is the "stationary" frame while is the "moving" frame. According to the principle of relativity, there is no privileged frame of reference, so the transformations from to must take exactly the same form as the transformations from to . The only difference is moves with velocity relative to (i.e., the relative velocity has the same magnitude but is oppositely directed). Thus if an observer in notes an event , , , , then an observer in notes the ''same'' event with coordinates and the value of remains unchanged. This "trick" of simply reversing the direction of relative velocity while preserving its magnitude, and exchanging primed and unprimed variables, always applies to finding the inverse transformation of every boost in any direction. Sometimes it is more convenient to use (lowercase
beta Beta (, ; uppercase , lowercase , or cursive ; or ) is the second letter of the Greek alphabet. In the system of Greek numerals, it has a value of 2. In Ancient Greek, beta represented the voiced bilabial plosive . In Modern Greek, it represe ...
) instead of , so that \begin ct' &= \gamma \left( ct - \beta x \right) \,, \\ x' &= \gamma \left( x - \beta ct \right) \,, \\ \end which shows much more clearly the symmetry in the transformation. From the allowed ranges of and the definition of , it follows . The use of and is standard throughout the literature. In the case of three spatial dimensions 'ct'',''x'',''y'',''z'' where the boost \beta is in the ''x'' direction, the eigenstates of the transformation are with eigenvalue \sqrt, with eigenvalue \sqrt, and and , the latter two with eigenvalue 1.  When the boost velocity \boldsymbol is in an arbitrary vector direction with the boost vector \boldsymbol=\boldsymbol/c, then the transformation from an unprimed spacetime coordinate system to a primed coordinate system is given by \begin ct' \vphantom \\ x' \vphantom \\ y' \vphantom \\ z' \vphantom \end = \begin \gamma & -\gamma\beta _x & -\gamma\beta _y & -\gamma\beta _z \\ -\gamma\beta _x & 1+\frac\beta _x^2 & \frac\beta _x \beta _y& \frac\beta _x\beta _z \\ -\gamma\beta _y & \frac\beta _x \beta _y & 1+\frac\beta _y^2 & \frac\beta _y\beta _z \\ -\gamma\beta _z & \frac\beta _x\beta _z & \frac\beta _y\beta _z & 1+\frac\beta _z^2 \\ \end \begin ct \vphantom \\ x \vphantom \\ y \vphantom \\ z \vphantom \end, where the
Lorentz factor The Lorentz factor or Lorentz term (also known as the gamma factor) is a dimensionless quantity expressing how much the measurements of time, length, and other physical properties change for an object while it moves. The expression appears in sev ...
is \gamma =1/\sqrt . The
determinant In mathematics, the determinant is a Scalar (mathematics), scalar-valued function (mathematics), function of the entries of a square matrix. The determinant of a matrix is commonly denoted , , or . Its value characterizes some properties of the ...
of the transformation matrix is +1 and its trace is 2(1+\gamma). The inverse of the transformation is given by reversing the sign of \boldsymbol. The quantity c^2t^2-x^2-y^2-z^2 is invariant under the transformation: namely (ct'^2-x'^2-y'^2-z'^2)=(ct^2-x^2-y^2-z^2). The Lorentz transformations can also be derived in a way that resembles circular rotations in 3-dimensional space using the hyperbolic functions. For the boost in the direction, the results are where (lowercase
zeta Zeta (, ; uppercase Ζ, lowercase ζ; , , classical or ''zē̂ta''; ''zíta'') is the sixth letter of the Greek alphabet. In the system of Greek numerals, it has a value of 7. It was derived from the Phoenician alphabet, Phoenician letter zay ...
) is a parameter called ''
rapidity In special relativity, the classical concept of velocity is converted to rapidity to accommodate the limit determined by the speed of light. Velocities must be combined by Einstein's velocity-addition formula. For low speeds, rapidity and velo ...
'' (many other symbols are used, including , , , , , ). Given the strong resemblance to rotations of spatial coordinates in 3-dimensional space in the Cartesian , , and planes, a Lorentz boost can be thought of as a hyperbolic rotation of spacetime coordinates in the xt, yt, and zt Cartesian-time planes of 4-dimensional
Minkowski space In physics, Minkowski space (or Minkowski spacetime) () is the main mathematical description of spacetime in the absence of gravitation. It combines inertial space and time manifolds into a four-dimensional model. The model helps show how a ...
. The parameter is the hyperbolic angle of rotation, analogous to the ordinary angle for circular rotations. This transformation can be illustrated with a Minkowski diagram. The hyperbolic functions arise from the ''difference'' between the squares of the time and spatial coordinates in the spacetime interval, rather than a sum. The geometric significance of the hyperbolic functions can be visualized by taking or in the transformations. Squaring and subtracting the results, one can derive hyperbolic curves of constant coordinate values but varying , which parametrizes the curves according to the identity \cosh^2\zeta - \sinh^2\zeta = 1 \,. Conversely the and axes can be constructed for varying coordinates but constant . The definition \tanh\zeta = \frac \,, provides the link between a constant value of rapidity, and the
slope In mathematics, the slope or gradient of a Line (mathematics), line is a number that describes the direction (geometry), direction of the line on a plane (geometry), plane. Often denoted by the letter ''m'', slope is calculated as the ratio of t ...
of the axis in spacetime. A consequence these two hyperbolic formulae is an identity that matches the Lorentz factor \cosh\zeta = \frac \,. Comparing the Lorentz transformations in terms of the relative velocity and rapidity, or using the above formulae, the connections between , , and are \begin \beta &= \tanh\zeta \,, \\ \gamma &= \cosh\zeta \,, \\ \beta \gamma &= \sinh\zeta \,. \end Taking the inverse hyperbolic tangent gives the rapidity \zeta = \tanh^\beta \,. Since , it follows . From the relation between and , positive rapidity is motion along the positive directions of the axes, zero rapidity is no relative motion, while negative rapidity is relative motion along the negative directions of the axes. The inverse transformations are obtained by exchanging primed and unprimed quantities to switch the coordinate frames, and negating rapidity since this is equivalent to negating the relative velocity. Therefore, The inverse transformations can be similarly visualized by considering the cases when and . So far the Lorentz transformations have been applied to ''one event''. If there are two events, there is a spatial separation and time interval between them. It follows from the
linearity In mathematics, the term ''linear'' is used in two distinct senses for two different properties: * linearity of a '' function'' (or '' mapping''); * linearity of a '' polynomial''. An example of a linear function is the function defined by f(x) ...
of the Lorentz transformations that two values of space and time coordinates can be chosen, the Lorentz transformations can be applied to each, then subtracted to get the Lorentz transformations of the differences; \begin \Delta t' &= \gamma \left( \Delta t - \frac \right) \,, \\ \Delta x' &= \gamma \left( \Delta x - v \, \Delta t \right) \,, \end with inverse relations \begin \Delta t &= \gamma \left( \Delta t' + \frac \right) \,, \\ \Delta x &= \gamma \left( \Delta x' + v \, \Delta t' \right) \,. \end where (uppercase
delta Delta commonly refers to: * Delta (letter) (Δ or δ), the fourth letter of the Greek alphabet * D (NATO phonetic alphabet: "Delta"), the fourth letter in the Latin alphabet * River delta, at a river mouth * Delta Air Lines, a major US carrier ...
) indicates a difference of quantities; e.g., for two values of coordinates, and so on. These transformations on ''differences'' rather than spatial points or instants of time are useful for a number of reasons: * in calculations and experiments, it is lengths between two points or time intervals that are measured or of interest (e.g., the length of a moving vehicle, or time duration it takes to travel from one place to another), * the transformations of velocity can be readily derived by making the difference infinitesimally small and dividing the equations, and the process repeated for the transformation of acceleration, * if the coordinate systems are never coincident (i.e., not in standard configuration), and if both observers can agree on an event in and in , then they can use that event as the origin, and the spacetime coordinate differences are the differences between their coordinates and this origin, e.g., , , etc.


Physical implications

A critical requirement of the Lorentz transformations is the invariance of the speed of light, a fact used in their derivation, and contained in the transformations themselves. If in the equation for a pulse of light along the direction is , then in the Lorentz transformations give , and vice versa, for any . For relative speeds much less than the speed of light, the Lorentz transformations reduce to the Galilean transformation: \begin t' &\approx t \\ x' &\approx x - vt \end in accordance with the
correspondence principle In physics, a correspondence principle is any one of several premises or assertions about the relationship between classical and quantum mechanics. The physicist Niels Bohr coined the term in 1920 during the early development of quantum theory; ...
. It is sometimes said that nonrelativistic physics is a physics of "instantaneous action at a distance". Three counterintuitive, but correct, predictions of the transformations are: ;
Relativity of simultaneity In physics, the relativity of simultaneity is the concept that ''distant simultaneity'' – whether two spatially separated events occur at the same time – is not absolute, but depends on the observer's reference frame. This poss ...
: Suppose two events occur along the x axis simultaneously () in , but separated by a nonzero displacement . Then in , we find that \Delta t' = \gamma \frac , so the events are no longer simultaneous according to a moving observer. ;
Time dilation Time dilation is the difference in elapsed time as measured by two clocks, either because of a relative velocity between them (special relativity), or a difference in gravitational potential between their locations (general relativity). When unsp ...
: Suppose there is a clock at rest in . If a time interval is measured at the same point in that frame, so that , then the transformations give this interval in by . Conversely, suppose there is a clock at rest in . If an interval is measured at the same point in that frame, so that , then the transformations give this interval in by . Either way, each observer measures the time interval between ticks of a moving clock to be longer by a factor than the time interval between ticks of his own clock. ;
Length contraction Length contraction is the phenomenon that a moving object's length is measured to be shorter than its proper length, which is the length as measured in the object's own rest frame. It is also known as Lorentz contraction or Lorentz–FitzGerald ...
: Suppose there is a rod at rest in aligned along the axis, with length . In , the rod moves with velocity , so its length must be measured by taking two simultaneous () measurements at opposite ends. Under these conditions, the inverse Lorentz transform shows that . In the two measurements are no longer simultaneous, but this does not matter because the rod is at rest in . So each observer measures the distance between the end points of a moving rod to be shorter by a factor than the end points of an identical rod at rest in his own frame. Length contraction affects any geometric quantity related to lengths, so from the perspective of a moving observer, areas and volumes will also appear to shrink along the direction of motion.


Vector transformations

The use of vectors allows positions and velocities to be expressed in arbitrary directions compactly. A single boost in any direction depends on the full relative velocity vector with a magnitude that cannot equal or exceed , so that . Only time and the coordinates parallel to the direction of relative motion change, while those coordinates perpendicular do not. With this in mind, split the spatial
position vector In geometry, a position or position vector, also known as location vector or radius vector, is a Euclidean vector that represents a point ''P'' in space. Its length represents the distance in relation to an arbitrary reference origin ''O'', and ...
as measured in , and as measured in , each into components perpendicular (⊥) and parallel ( ‖ ) to , \mathbf=\mathbf_\perp+\mathbf_\, \,,\quad \mathbf' = \mathbf_\perp' + \mathbf_\, ' \,, then the transformations are \begin t' &= \gamma \left(t - \frac \right) \\ \mathbf_\, ' &= \gamma (\mathbf_\, - \mathbf t) \\ \mathbf_\perp' &= \mathbf_\perp \end where is the
dot product In mathematics, the dot product or scalar productThe term ''scalar product'' means literally "product with a Scalar (mathematics), scalar as a result". It is also used for other symmetric bilinear forms, for example in a pseudo-Euclidean space. N ...
. The Lorentz factor retains its definition for a boost in any direction, since it depends only on the magnitude of the relative velocity. The definition with magnitude is also used by some authors. Introducing a
unit vector In mathematics, a unit vector in a normed vector space is a Vector (mathematics and physics), vector (often a vector (geometry), spatial vector) of Norm (mathematics), length 1. A unit vector is often denoted by a lowercase letter with a circumfle ...
in the direction of relative motion, the relative velocity is with magnitude and direction , and vector projection and rejection give respectively \mathbf_\parallel = (\mathbf\cdot\mathbf)\mathbf\,,\quad \mathbf_\perp = \mathbf - (\mathbf\cdot\mathbf)\mathbf Accumulating the results gives the full transformations, The projection and rejection also applies to . For the inverse transformations, exchange and to switch observed coordinates, and negate the relative velocity (or simply the unit vector since the magnitude is always positive) to obtain The unit vector has the advantage of simplifying equations for a single boost, allows either or to be reinstated when convenient, and the rapidity parametrization is immediately obtained by replacing and . It is not convenient for multiple boosts. The vectorial relation between relative velocity and rapidity is \boldsymbol = \beta \mathbf = \mathbf \tanh\zeta \,, and the "rapidity vector" can be defined as \boldsymbol = \zeta\mathbf = \mathbf\tanh^\beta \,, each of which serves as a useful abbreviation in some contexts. The magnitude of is the absolute value of the rapidity scalar confined to , which agrees with the range .


Transformation of velocities

Defining the coordinate velocities and Lorentz factor by :\mathbf = \frac \,,\quad \mathbf' = \frac \,,\quad \gamma_\mathbf = \frac taking the differentials in the coordinates and time of the vector transformations, then dividing equations, leads to :\mathbf' = \frac\left frac - \mathbf + \frac\frac\left(\mathbf\cdot\mathbf\right)\mathbf\right The velocities and are the velocity of some massive object. They can also be for a third inertial frame (say ), in which case they must be ''constant''. Denote either entity by . Then moves with velocity relative to , or equivalently with velocity relative to , in turn moves with velocity relative to . The inverse transformations can be obtained in a similar way, or as with position coordinates exchange and , and change to . The transformation of velocity is useful in
stellar aberration In astronomy, aberration (also referred to as astronomical aberration, stellar aberration, or velocity aberration) is a phenomenon where celestial objects exhibit an apparent motion about their true positions based on the velocity of the obser ...
, the Fizeau experiment, and the relativistic Doppler effect. The Lorentz transformations of acceleration can be similarly obtained by taking differentials in the velocity vectors, and dividing these by the time differential.


Transformation of other quantities

In general, given four quantities and and their Lorentz-boosted counterparts and , a relation of the form A^2 - \mathbf\cdot\mathbf = ^2 - \mathbf'\cdot\mathbf' implies the quantities transform under Lorentz transformations similar to the transformation of spacetime coordinates; \begin A' &= \gamma \left(A - \frac \right) \,, \\ \mathbf' &= \mathbf + (\gamma-1)(\mathbf\cdot\mathbf)\mathbf - \frac \,. \end The decomposition of (and ) into components perpendicular and parallel to is exactly the same as for the position vector, as is the process of obtaining the inverse transformations (exchange and to switch observed quantities, and reverse the direction of relative motion by the substitution ). The quantities collectively make up a ''
four-vector In special relativity, a four-vector (or 4-vector, sometimes Lorentz vector) is an object with four components, which transform in a specific way under Lorentz transformations. Specifically, a four-vector is an element of a four-dimensional vect ...
'', where is the "timelike component", and the "spacelike component". Examples of and are the following: For a given object (e.g., particle, fluid, field, material), if or correspond to properties specific to the object like its charge density,
mass density Density (volumetric mass density or specific mass) is the ratio of a substance's mass to its volume. The symbol most often used for density is ''ρ'' (the lower case Greek language, Greek letter rho), although the Latin letter ''D'' (or ''d'') ...
, spin, etc., its properties can be fixed in the rest frame of that object. Then the Lorentz transformations give the corresponding properties in a frame moving relative to the object with constant velocity. This breaks some notions taken for granted in non-relativistic physics. For example, the energy of an object is a scalar in non-relativistic mechanics, but not in relativistic mechanics because energy changes under Lorentz transformations; its value is different for various inertial frames. In the rest frame of an object, it has a rest energy and zero momentum. In a boosted frame its energy is different and it appears to have a momentum. Similarly, in non-relativistic quantum mechanics the spin of a particle is a constant vector, but in relativistic quantum mechanics spin depends on relative motion. In the rest frame of the particle, the spin pseudovector can be fixed to be its ordinary non-relativistic spin with a zero timelike quantity , however a boosted observer will perceive a nonzero timelike component and an altered spin. Not all quantities are invariant in the form as shown above, for example orbital
angular momentum Angular momentum (sometimes called moment of momentum or rotational momentum) is the rotational analog of Momentum, linear momentum. It is an important physical quantity because it is a Conservation law, conserved quantity – the total ang ...
does not have a timelike quantity, and neither does the
electric field An electric field (sometimes called E-field) is a field (physics), physical field that surrounds electrically charged particles such as electrons. In classical electromagnetism, the electric field of a single charge (or group of charges) descri ...
nor the
magnetic field A magnetic field (sometimes called B-field) is a physical field that describes the magnetic influence on moving electric charges, electric currents, and magnetic materials. A moving charge in a magnetic field experiences a force perpendicular ...
. The definition of angular momentum is , and in a boosted frame the altered angular momentum is . Applying this definition using the transformations of coordinates and momentum leads to the transformation of angular momentum. It turns out transforms with another vector quantity related to boosts, see relativistic angular momentum for details. For the case of the and fields, the transformations cannot be obtained as directly using vector algebra. The Lorentz force is the definition of these fields, and in it is while in it is . A method of deriving the EM field transformations in an efficient way which also illustrates the unit of the electromagnetic field uses tensor algebra, given below.


Mathematical formulation

Throughout, italic non-bold capital letters are matrices, while non-italic bold letters are matrices.


Homogeneous Lorentz group

Writing the coordinates in column vectors and the
Minkowski metric In physics, Minkowski space (or Minkowski spacetime) () is the main mathematical description of spacetime in the absence of general_relativity, gravitation. It combines inertial space and time manifolds into a four-dimensional model. The model ...
as a square matrix X' = \begin c\,t' \\ x' \\ y' \\ z' \end \,, \quad \eta = \begin -1&0&0&0\\ 0&1&0&0 \\ 0&0&1&0 \\ 0&0&0&1 \end \,, \quad X = \begin c\,t \\ x \\ y \\ z \end the spacetime interval takes the form (superscript denotes
transpose In linear algebra, the transpose of a Matrix (mathematics), matrix is an operator which flips a matrix over its diagonal; that is, it switches the row and column indices of the matrix by producing another matrix, often denoted by (among other ...
) X \cdot X = X^\mathrm \eta X = ^\mathrm \eta and is invariant under a Lorentz transformation X' = \Lambda X where is a square matrix which can depend on parameters. The
set Set, The Set, SET or SETS may refer to: Science, technology, and mathematics Mathematics *Set (mathematics), a collection of elements *Category of sets, the category whose objects and morphisms are sets and total functions, respectively Electro ...
of all Lorentz transformations \Lambda in this article is denoted \mathcal. This set together with matrix multiplication forms a group, in this context known as the '' Lorentz group''. Also, the above expression is a
quadratic form In mathematics, a quadratic form is a polynomial with terms all of degree two (" form" is another name for a homogeneous polynomial). For example, 4x^2 + 2xy - 3y^2 is a quadratic form in the variables and . The coefficients usually belong t ...
of signature (3,1) on spacetime, and the group of transformations which leaves this quadratic form invariant is the
indefinite orthogonal group In mathematics, the indefinite orthogonal group, is the Lie group of all linear transformations of an ''n''-dimension (vector space), dimensional real number, real vector space that leave invariant a nondegenerate form, nondegenerate, symmetric bi ...
O(3,1), a
Lie group In mathematics, a Lie group (pronounced ) is a group (mathematics), group that is also a differentiable manifold, such that group multiplication and taking inverses are both differentiable. A manifold is a space that locally resembles Eucli ...
. In other words, the Lorentz group is O(3,1). As presented in this article, any Lie groups mentioned are matrix Lie groups. In this context the operation of composition amounts to
matrix multiplication In mathematics, specifically in linear algebra, matrix multiplication is a binary operation that produces a matrix (mathematics), matrix from two matrices. For matrix multiplication, the number of columns in the first matrix must be equal to the n ...
. From the invariance of the spacetime interval it follows \eta = \Lambda^\mathrm \eta \Lambda and this matrix equation contains the general conditions on the Lorentz transformation to ensure invariance of the spacetime interval. Taking the
determinant In mathematics, the determinant is a Scalar (mathematics), scalar-valued function (mathematics), function of the entries of a square matrix. The determinant of a matrix is commonly denoted , , or . Its value characterizes some properties of the ...
of the equation using the product ruleFor two square matrices and , gives immediately \left det (\Lambda)\right2 = 1 \quad \Rightarrow \quad \det(\Lambda) = \pm 1 Writing the Minkowski metric as a block matrix, and the Lorentz transformation in the most general form, \eta = \begin-1 & 0 \\ 0 & \mathbf\end \,, \quad \Lambda=\begin\Gamma & -\mathbf^\mathrm\\-\mathbf & \mathbf\end \,, carrying out the block matrix multiplications obtains general conditions on to ensure relativistic invariance. Not much information can be directly extracted from all the conditions, however one of the results \Gamma^2 = 1 + \mathbf^\mathrm\mathbf is useful; always so it follows that \Gamma^2 \geq 1 \quad \Rightarrow \quad \Gamma \leq - 1 \,,\quad \Gamma \geq 1 The negative inequality may be unexpected, because multiplies the time coordinate and this has an effect on time symmetry. If the positive equality holds, then is the Lorentz factor. The determinant and inequality provide four ways to classify Lorentz Transformations (''herein LTs for brevity''). Any particular LT has only one determinant sign ''and'' only one inequality. There are four sets which include every possible pair given by the
intersection In mathematics, the intersection of two or more objects is another object consisting of everything that is contained in all of the objects simultaneously. For example, in Euclidean geometry, when two lines in a plane are not parallel, their ...
s ("n"-shaped symbol meaning "and") of these classifying sets. where "+" and "−" indicate the determinant sign, while "↑" for ≥ and "↓" for ≤ denote the inequalities. The full Lorentz group splits into the union ("u"-shaped symbol meaning "or") of four disjoint sets \mathcal = \mathcal_^\uparrow \cup \mathcal_^\uparrow \cup \mathcal_^\downarrow \cup \mathcal_^\downarrow A
subgroup In group theory, a branch of mathematics, a subset of a group G is a subgroup of G if the members of that subset form a group with respect to the group operation in G. Formally, given a group (mathematics), group under a binary operation  ...
of a group must be closed under the same operation of the group (here matrix multiplication). In other words, for two Lorentz transformations and from a particular subgroup, the composite Lorentz transformations and must be in the same subgroup as and . This is not always the case: the composition of two antichronous Lorentz transformations is orthochronous, and the composition of two improper Lorentz transformations is proper. In other words, while the sets \mathcal_+^\uparrow , \mathcal_+, \mathcal^\uparrow, and \mathcal_0 = \mathcal_+^\uparrow \cup \mathcal_^\downarrow all form subgroups, the sets containing improper and/or antichronous transformations without enough proper orthochronous transformations (e.g. \mathcal_+^\downarrow , \mathcal_^\downarrow , \mathcal_^\uparrow ) do not form subgroups.


Proper transformations

If a Lorentz covariant 4-vector is measured in one inertial frame with result X, and the same measurement made in another inertial frame (with the same orientation and origin) gives result X', the two results will be related by X' = B(\mathbf)X where the boost matrix B(\mathbf) represents the rotation-free Lorentz transformation between the unprimed and primed frames and \mathbf is the velocity of the primed frame as seen from the unprimed frame. The matrix is given by B(\mathbf) = \begin \gamma &-\gamma v_x/c &-\gamma v_y/c &-\gamma v_z/c \\ -\gamma v_x/c&1+(\gamma-1)\dfrac & (\gamma-1)\dfrac& (\gamma-1)\dfrac \\ -\gamma v_y/c& (\gamma-1)\dfrac&1+(\gamma-1)\dfrac & (\gamma-1)\dfrac \\ -\gamma v_z/c& (\gamma-1)\dfrac& (\gamma-1)\dfrac&1+(\gamma-1)\dfrac \end = \begin \gamma & -\gamma \vec^T \\ -\gamma \vec & I + (\gamma-1)\dfrac \end, where v=\sqrt is the magnitude of the velocity and \gamma=\frac is the Lorentz factor. This formula represents a passive transformation, as it describes how the coordinates of the measured quantity changes from the unprimed frame to the primed frame. The active transformation is given by B(-\mathbf). If a frame is boosted with velocity relative to frame , and another frame is boosted with velocity relative to , the separate boosts are X'' = B(\mathbf)X' \,, \quad X' = B(\mathbf)X and the composition of the two boosts connects the coordinates in and , X'' = B(\mathbf)B(\mathbf)X \,. Successive transformations act on the left. If and are
collinear In geometry, collinearity of a set of Point (geometry), points is the property of their lying on a single Line (geometry), line. A set of points with this property is said to be collinear (sometimes spelled as colinear). In greater generality, t ...
(parallel or antiparallel along the same line of relative motion), the boost matrices commute: . This composite transformation happens to be another boost, , where is collinear with and . If and are not collinear but in different directions, the situation is considerably more complicated. Lorentz boosts along different directions do not commute: and are not equal. Although each of these compositions is ''not'' a single boost, each composition is still a Lorentz transformation as it preserves the spacetime interval. It turns out the composition of any two Lorentz boosts is equivalent to a boost followed or preceded by a rotation on the spatial coordinates, in the form of or . The and are composite velocities, while and are rotation parameters (e.g. axis-angle variables,
Euler angles The Euler angles are three angles introduced by Leonhard Euler to describe the Orientation (geometry), orientation of a rigid body with respect to a fixed coordinate system.Novi Commentarii academiae scientiarum Petropolitanae 20, 1776, pp. 189� ...
, etc.). The rotation in block matrix form is simply \quad R(\boldsymbol) = \begin 1 & 0 \\ 0 & \mathbf(\boldsymbol) \end \,, where is a
rotation matrix In linear algebra, a rotation matrix is a transformation matrix that is used to perform a rotation (mathematics), rotation in Euclidean space. For example, using the convention below, the matrix :R = \begin \cos \theta & -\sin \theta \\ \sin \t ...
, which rotates any 3-dimensional vector in one sense (active transformation), or equivalently the coordinate frame in the opposite sense (passive transformation). It is ''not'' simple to connect and (or and ) to the original boost parameters and . In a composition of boosts, the matrix is named the Wigner rotation, and gives rise to the Thomas precession. These articles give the explicit formulae for the composite transformation matrices, including expressions for . In this article the axis-angle representation is used for . The rotation is about an axis in the direction of a
unit vector In mathematics, a unit vector in a normed vector space is a Vector (mathematics and physics), vector (often a vector (geometry), spatial vector) of Norm (mathematics), length 1. A unit vector is often denoted by a lowercase letter with a circumfle ...
, through angle (positive anticlockwise, negative clockwise, according to the
right-hand rule In mathematics and physics, the right-hand rule is a Convention (norm), convention and a mnemonic, utilized to define the orientation (vector space), orientation of Cartesian coordinate system, axes in three-dimensional space and to determine the ...
). The "axis-angle vector" \boldsymbol = \theta \mathbf will serve as a useful abbreviation. Spatial rotations alone are also Lorentz transformations since they leave the spacetime interval invariant. Like boosts, successive rotations about different axes do not commute. Unlike boosts, the composition of any two rotations is equivalent to a single rotation. Some other similarities and differences between the boost and rotation matrices include: * inverses: (relative motion in the opposite direction), and (rotation in the opposite sense about the same axis) *
identity transformation Graph of the identity function on the real numbers In mathematics, an identity function, also called an identity relation, identity map or identity transformation, is a function that always returns the value that was used as its argument, unc ...
for no relative motion/rotation: * unit
determinant In mathematics, the determinant is a Scalar (mathematics), scalar-valued function (mathematics), function of the entries of a square matrix. The determinant of a matrix is commonly denoted , , or . Its value characterizes some properties of the ...
: . This property makes them proper transformations. * matrix symmetry: is symmetric (equals
transpose In linear algebra, the transpose of a Matrix (mathematics), matrix is an operator which flips a matrix over its diagonal; that is, it switches the row and column indices of the matrix by producing another matrix, often denoted by (among other ...
), while is nonsymmetric but
orthogonal In mathematics, orthogonality (mathematics), orthogonality is the generalization of the geometric notion of ''perpendicularity''. Although many authors use the two terms ''perpendicular'' and ''orthogonal'' interchangeably, the term ''perpendic ...
(transpose equals inverse, ). The most general proper Lorentz transformation includes a boost and rotation together, and is a nonsymmetric matrix. As special cases, and . An explicit form of the general Lorentz transformation is cumbersome to write down and will not be given here. Nevertheless, closed form expressions for the transformation matrices will be given below using group theoretical arguments. It will be easier to use the rapidity parametrization for boosts, in which case one writes and .


The Lie group SO(3,1)

The set of transformations \ with matrix multiplication as the operation of composition forms a group, called the "restricted Lorentz group", and is the special indefinite orthogonal group SO(3,1). (The plus sign indicates that it preserves the orientation of the temporal dimension). For simplicity, look at the infinitesimal Lorentz boost in the direction (examining a boost in any other direction, or rotation about any axis, follows an identical procedure). The infinitesimal boost is a small boost away from the identity, obtained by the Taylor expansion of the boost matrix to first order about , B_x = I + \zeta \left. \frac \_ + \cdots where the higher order terms not shown are negligible because is small, and is simply the boost matrix in the ''x'' direction. The derivative of the matrix is the matrix of derivatives (of the entries, with respect to the same variable), and it is understood the derivatives are found first then evaluated at , \left. \frac \_ = - K_x \,. For now, is defined by this result (its significance will be explained shortly). In the limit of an infinite number of infinitely small steps, the finite boost transformation in the form of a
matrix exponential In mathematics, the matrix exponential is a matrix function on square matrix, square matrices analogous to the ordinary exponential function. It is used to solve systems of linear differential equations. In the theory of Lie groups, the matrix exp ...
is obtained B_x =\lim_\left(I-\fracK_x\right)^ = e^ where the limit definition of the exponential has been used (see also characterizations of the exponential function). More generallyExplicitly, \boldsymbol \cdot\mathbf = \zeta_x K_x + \zeta_y K_y + \zeta_z K_z \boldsymbol \cdot\mathbf = \theta_x J_x + \theta_y J_y + \theta_z J_z B(\boldsymbol) = e^ \, , \quad R(\boldsymbol) = e^ \,. The axis-angle vector and rapidity vector are altogether six continuous variables which make up the group parameters (in this particular representation), and the generators of the group are and , each vectors of matrices with the explicit formsIn
quantum mechanics Quantum mechanics is the fundamental physical Scientific theory, theory that describes the behavior of matter and of light; its unusual characteristics typically occur at and below the scale of atoms. Reprinted, Addison-Wesley, 1989, It is ...
, relativistic quantum mechanics, and
quantum field theory In theoretical physics, quantum field theory (QFT) is a theoretical framework that combines Field theory (physics), field theory and the principle of relativity with ideas behind quantum mechanics. QFT is used in particle physics to construct phy ...
, a different convention is used for these matrices; the right hand sides are all multiplied by a factor of the imaginary unit .
\begin K_x &= \begin 0 & 1 & 0 & 0 \\ 1 & 0 & 0 & 0 \\ 0 & 0 & 0 & 0 \\ 0 & 0 & 0 & 0 \\ \end\,,\quad & K_y &= \begin 0 & 0 & 1 & 0\\ 0 & 0 & 0 & 0\\ 1 & 0 & 0 & 0\\ 0 & 0 & 0 & 0 \end\,,\quad & K_z &= \begin 0 & 0 & 0 & 1\\ 0 & 0 & 0 & 0\\ 0 & 0 & 0 & 0\\ 1 & 0 & 0 & 0 \end \\ 0mu J_x &= \begin 0 & 0 & 0 & 0 \\ 0 & 0 & 0 & 0 \\ 0 & 0 & 0 & -1 \\ 0 & 0 & 1 & 0 \\ \end\,,\quad & J_y &= \begin 0 & 0 & 0 & 0 \\ 0 & 0 & 0 & 1 \\ 0 & 0 & 0 & 0 \\ 0 & -1 & 0 & 0 \end\,,\quad & J_z &= \begin 0 & 0 & 0 & 0 \\ 0 & 0 & -1 & 0 \\ 0 & 1 & 0 & 0 \\ 0 & 0 & 0 & 0 \end \end These are all defined in an analogous way to above, although the minus signs in the boost generators are conventional. Physically, the generators of the Lorentz group correspond to important symmetries in spacetime: are the ''rotation generators'' which correspond to
angular momentum Angular momentum (sometimes called moment of momentum or rotational momentum) is the rotational analog of Momentum, linear momentum. It is an important physical quantity because it is a Conservation law, conserved quantity – the total ang ...
, and are the ''boost generators'' which correspond to the motion of the system in spacetime. The derivative of any smooth curve with in the group depending on some group parameter with respect to that group parameter, evaluated at , serves as a definition of a corresponding group generator , and this reflects an infinitesimal transformation away from the identity. The smooth curve can always be taken as an exponential as the exponential will always map smoothly back into the group via for all ; this curve will yield again when differentiated at . Expanding the exponentials in their Taylor series obtains B()=I-\sinh \zeta (\mathbf \cdot \mathbf )+(\cosh \zeta -1)(\mathbf \cdot \mathbf )^2 R(\boldsymbol )=I+\sin \theta (\mathbf \cdot \mathbf )+(1-\cos \theta )(\mathbf \cdot \mathbf )^2\,. which compactly reproduce the boost and rotation matrices as given in the previous section. It has been stated that the general proper Lorentz transformation is a product of a boost and rotation. At the ''infinitesimal'' level the product \begin \Lambda &= (I - \boldsymbol \cdot \mathbf + \cdots )(I + \boldsymbol \cdot \mathbf + \cdots ) \\ &= (I + \boldsymbol \cdot \mathbf + \cdots )(I - \boldsymbol \cdot \mathbf + \cdots ) \\ &= I - \boldsymbol \cdot \mathbf + \boldsymbol \cdot \mathbf + \cdots \end is commutative because only linear terms are required (products like and count as higher order terms and are negligible). Taking the limit as before leads to the finite transformation in the form of an exponential \Lambda (\boldsymbol, \boldsymbol) = e^. The converse is also true, but the decomposition of a finite general Lorentz transformation into such factors is nontrivial. In particular, e^ \ne e^ e^, because the generators do not commute. For a description of how to find the factors of a general Lorentz transformation in terms of a boost and a rotation ''in principle'' (this usually does not yield an intelligible expression in terms of generators and ), see Wigner rotation. If, on the other hand, ''the decomposition is given'' in terms of the generators, and one wants to find the product in terms of the generators, then the
Baker–Campbell–Hausdorff formula In mathematics, the Baker–Campbell–Hausdorff formula gives the value of Z that solves the equation e^X e^Y = e^Z for possibly noncommutative and in the Lie algebra of a Lie group. There are various ways of writing the formula, but all ultima ...
applies.


The Lie algebra so(3,1)

Lorentz generators can be added together, or multiplied by real numbers, to obtain more Lorentz generators. In other words, the
set Set, The Set, SET or SETS may refer to: Science, technology, and mathematics Mathematics *Set (mathematics), a collection of elements *Category of sets, the category whose objects and morphisms are sets and total functions, respectively Electro ...
of all Lorentz generators V = \ together with the operations of ordinary
matrix addition In mathematics, matrix addition is the operation of adding two matrices by adding the corresponding entries together. For a vector, \vec\!, adding two matrices would have the geometric effect of applying each matrix transformation separately ...
and multiplication of a matrix by a number, forms a
vector space In mathematics and physics, a vector space (also called a linear space) is a set (mathematics), set whose elements, often called vector (mathematics and physics), ''vectors'', can be added together and multiplied ("scaled") by numbers called sc ...
over the real numbers.Until now the term "vector" has exclusively referred to "
Euclidean vector In mathematics, physics, and engineering, a Euclidean vector or simply a vector (sometimes called a geometric vector or spatial vector) is a geometric object that has magnitude (or length) and direction. Euclidean vectors can be added and scal ...
", examples are position , velocity , etc. The term "vector" applies much more broadly than Euclidean vectors, row or column vectors, etc., see
linear algebra Linear algebra is the branch of mathematics concerning linear equations such as :a_1x_1+\cdots +a_nx_n=b, linear maps such as :(x_1, \ldots, x_n) \mapsto a_1x_1+\cdots +a_nx_n, and their representations in vector spaces and through matrix (mathemat ...
and
vector space In mathematics and physics, a vector space (also called a linear space) is a set (mathematics), set whose elements, often called vector (mathematics and physics), ''vectors'', can be added together and multiplied ("scaled") by numbers called sc ...
for details. The generators of a Lie group also form a vector space over a field of numbers (e.g.
real number In mathematics, a real number is a number that can be used to measure a continuous one- dimensional quantity such as a duration or temperature. Here, ''continuous'' means that pairs of values can have arbitrarily small differences. Every re ...
s,
complex number In mathematics, a complex number is an element of a number system that extends the real numbers with a specific element denoted , called the imaginary unit and satisfying the equation i^= -1; every complex number can be expressed in the for ...
s), since a
linear combination In mathematics, a linear combination or superposition is an Expression (mathematics), expression constructed from a Set (mathematics), set of terms by multiplying each term by a constant and adding the results (e.g. a linear combination of ''x'' a ...
of the generators is also a generator. They just live in a different space to the position vectors in ordinary 3-dimensional space.
The generators form a basis set of ''V'', and the components of the axis-angle and rapidity vectors, , are the coordinates of a Lorentz generator with respect to this basis.In ordinary 3-dimensional position space, the position vector is expressed as a linear combination of the Cartesian unit vectors which form a basis, and the Cartesian coordinates are coordinates with respect to this basis. Three of the commutation relations of the Lorentz generators are J_x, J_y = J_z \,,\quad K_x, K_y = -J_z \,,\quad J_x, K_y = K_z \,, where the bracket is known as the ''
commutator In mathematics, the commutator gives an indication of the extent to which a certain binary operation fails to be commutative. There are different definitions used in group theory and ring theory. Group theory The commutator of two elements, ...
'', and the other relations can be found by taking
cyclic permutation In mathematics, and in particular in group theory, a cyclic permutation is a permutation consisting of a single cycle. In some cases, cyclic permutations are referred to as cycles; if a cyclic permutation has ''k'' elements, it may be called a ''k ...
s of , , components (i.e. change to , to , and to , repeat). These commutation relations, and the vector space of generators, fulfill the definition of the
Lie algebra In mathematics, a Lie algebra (pronounced ) is a vector space \mathfrak g together with an operation called the Lie bracket, an alternating bilinear map \mathfrak g \times \mathfrak g \rightarrow \mathfrak g, that satisfies the Jacobi ident ...
\mathfrak(3, 1). In summary, a Lie algebra is defined as a
vector space In mathematics and physics, a vector space (also called a linear space) is a set (mathematics), set whose elements, often called vector (mathematics and physics), ''vectors'', can be added together and multiplied ("scaled") by numbers called sc ...
''V'' over a field of numbers, and with a
binary operation In mathematics, a binary operation or dyadic operation is a rule for combining two elements (called operands) to produce another element. More formally, a binary operation is an operation of arity two. More specifically, a binary operation ...
, (called a Lie bracket in this context) on the elements of the vector space, satisfying the axioms of bilinearity, alternatization, and the Jacobi identity. Here the operation , is the commutator which satisfies all of these axioms, the vector space is the set of Lorentz generators ''V'' as given previously, and the field is the set of real numbers. Linking terminology used in mathematics and physics: A group generator is any element of the Lie algebra. A group parameter is a component of a coordinate vector representing an arbitrary element of the Lie algebra with respect to some basis. A basis, then, is a set of generators being a basis of the Lie algebra in the usual vector space sense. The exponential map from the Lie algebra to the Lie group, \exp \, : \, \mathfrak(3,1) \to \mathrm(3,1), provides a one-to-one correspondence between small enough neighborhoods of the origin of the Lie algebra and neighborhoods of the identity element of the Lie group. In the case of the Lorentz group, the exponential map is just the
matrix exponential In mathematics, the matrix exponential is a matrix function on square matrix, square matrices analogous to the ordinary exponential function. It is used to solve systems of linear differential equations. In the theory of Lie groups, the matrix exp ...
. Globally, the exponential map is not one-to-one, but in the case of the Lorentz group, it is
surjective In mathematics, a surjective function (also known as surjection, or onto function ) is a function such that, for every element of the function's codomain, there exists one element in the function's domain such that . In other words, for a f ...
(onto). Hence any group element in the connected component of the identity can be expressed as an exponential of an element of the Lie algebra.


Improper transformations

Lorentz transformations also include parity inversion P = \begin 1 & 0 \\ 0 & - \mathbf \end which negates all the spatial coordinates only, and time reversal T = \begin - 1 & 0 \\ 0 & \mathbf \end which negates the time coordinate only, because these transformations leave the spacetime interval invariant. Here is the
identity matrix In linear algebra, the identity matrix of size n is the n\times n square matrix with ones on the main diagonal and zeros elsewhere. It has unique properties, for example when the identity matrix represents a geometric transformation, the obje ...
. These are both symmetric, they are their own inverses (see
involution (mathematics) In mathematics, an involution, involutory function, or self-inverse function is a function that is its own inverse, : for all in the domain of . Equivalently, applying twice produces the original value. General properties Any involution ...
), and each have determinant −1. This latter property makes them improper transformations. If is a proper orthochronous Lorentz transformation, then is improper antichronous, is improper orthochronous, and is proper antichronous.


Inhomogeneous Lorentz group

Two other spacetime symmetries have not been accounted for. In order for the spacetime interval to be invariant, it can be shown that it is necessary and sufficient for the coordinate transformation to be of the form X' = \Lambda X + C where ''C'' is a constant column containing translations in time and space. If ''C'' ≠ 0, this is an inhomogeneous Lorentz transformation or Poincaré transformation. If ''C'' = 0, this is a homogeneous Lorentz transformation. Poincaré transformations are not dealt further in this article.


Tensor formulation


Contravariant vectors

Writing the general matrix transformation of coordinates as the matrix equation \begin ^0 \\ ^1 \\ ^2 \\ ^3 \end = \begin _0 & _1 & _2 & _3 \vphantom \\ _0 & _1 & _2 & _3 \vphantom \\ _0 & _1 & _2 & _3 \vphantom \\ _0 & _1 & _2 & _3 \vphantom \\ \end \begin x^0 \vphantom \\ x^1 \vphantom \\ x^2 \vphantom \\ x^3 \vphantom \end allows the transformation of other physical quantities that cannot be expressed as four-vectors; e.g.,
tensor In mathematics, a tensor is an algebraic object that describes a multilinear relationship between sets of algebraic objects associated with a vector space. Tensors may map between different objects such as vectors, scalars, and even other ...
s or spinors of any order in 4-dimensional spacetime, to be defined. In the corresponding tensor index notation, the above matrix expression is ^\nu = _\mu x^\mu, where lower and upper indices label covariant and contravariant components respectively, and the summation convention is applied. It is a standard convention to use Greek indices that take the value 0 for time components, and 1, 2, 3 for space components, while
Latin Latin ( or ) is a classical language belonging to the Italic languages, Italic branch of the Indo-European languages. Latin was originally spoken by the Latins (Italic tribe), Latins in Latium (now known as Lazio), the lower Tiber area aroun ...
indices simply take the values 1, 2, 3, for spatial components (the opposite for Landau and Lifshitz). Note that the first index (reading left to right) corresponds in the matrix notation to a ''row index''. The second index corresponds to the column index. The transformation matrix is universal for all
four-vector In special relativity, a four-vector (or 4-vector, sometimes Lorentz vector) is an object with four components, which transform in a specific way under Lorentz transformations. Specifically, a four-vector is an element of a four-dimensional vect ...
s, not just 4-dimensional spacetime coordinates. If is any four-vector, then in tensor index notation ^\nu = _\mu A^\mu \,. Alternatively, one writes A^ = _\mu A^\mu \,. in which the primed indices denote the indices of A in the primed frame. For a general -component object one may write ^\alpha = _\beta X^\beta \,, where is the appropriate representation of the Lorentz group, an matrix for every . In this case, the indices should ''not'' be thought of as spacetime indices (sometimes called Lorentz indices), and they run from to . E.g., if is a bispinor, then the indices are called ''Dirac indices''.


Covariant vectors

There are also vector quantities with covariant indices. They are generally obtained from their corresponding objects with contravariant indices by the operation of ''lowering an index''; e.g., x_\nu = \eta_x^\mu, where is the
metric tensor In the mathematical field of differential geometry, a metric tensor (or simply metric) is an additional structure on a manifold (such as a surface) that allows defining distances and angles, just as the inner product on a Euclidean space allows ...
. (The linked article also provides more information about what the operation of raising and lowering indices really is mathematically.) The inverse of this transformation is given by x^\mu = \eta^x_\nu, where, when viewed as matrices, is the inverse of . As it happens, . This is referred to as ''raising an index''. To transform a covariant vector , first raise its index, then transform it according to the same rule as for contravariant -vectors, then finally lower the index; _\nu = \eta_ _\sigma \eta^A_\mu. But \eta_ _\sigma \eta^ = _\nu, That is, it is the -component of the ''inverse'' Lorentz transformation. One defines (as a matter of notation), ^\mu \equiv _\nu, and may in this notation write _\nu = ^\mu A_\mu. Now for a subtlety. The implied summation on the right hand side of _\nu = ^\mu A_\mu = _\nu A_\mu is running over ''a row index'' of the matrix representing . Thus, in terms of matrices, this transformation should be thought of as the ''inverse transpose'' of acting on the column vector . That is, in pure matrix notation, A' = \left(\Lambda^\right)^\mathrm A. This means exactly that covariant vectors (thought of as column matrices) transform according to the dual representation of the standard representation of the Lorentz group. This notion generalizes to general representations, simply replace with .


Tensors

If and are linear operators on vector spaces and , then a linear operator may be defined on the
tensor product In mathematics, the tensor product V \otimes W of two vector spaces V and W (over the same field) is a vector space to which is associated a bilinear map V\times W \rightarrow V\otimes W that maps a pair (v,w),\ v\in V, w\in W to an element of ...
of and , denoted according to From this it is immediately clear that if and are a four-vectors in , then transforms as The second step uses the bilinearity of the tensor product and the last step defines a 2-tensor on component form, or rather, it just renames the tensor . These observations generalize in an obvious way to more factors, and using the fact that a general tensor on a vector space can be written as a sum of a coefficient (component!) times tensor products of basis vectors and basis covectors, one arrives at the transformation law for any
tensor In mathematics, a tensor is an algebraic object that describes a multilinear relationship between sets of algebraic objects associated with a vector space. Tensors may map between different objects such as vectors, scalars, and even other ...
quantity . It is given by where is defined above. This form can generally be reduced to the form for general -component objects given above with a single matrix () operating on column vectors. This latter form is sometimes preferred; e.g., for the electromagnetic field tensor.


Transformation of the electromagnetic field

Lorentz transformations can also be used to illustrate that the
magnetic field A magnetic field (sometimes called B-field) is a physical field that describes the magnetic influence on moving electric charges, electric currents, and magnetic materials. A moving charge in a magnetic field experiences a force perpendicular ...
and
electric field An electric field (sometimes called E-field) is a field (physics), physical field that surrounds electrically charged particles such as electrons. In classical electromagnetism, the electric field of a single charge (or group of charges) descri ...
are simply different aspects of the same force — the
electromagnetic force In physics, electromagnetism is an interaction that occurs between particles with electric charge via electromagnetic fields. The electromagnetic force is one of the four fundamental forces of nature. It is the dominant force in the interac ...
, as a consequence of relative motion between
electric charge Electric charge (symbol ''q'', sometimes ''Q'') is a physical property of matter that causes it to experience a force when placed in an electromagnetic field. Electric charge can be ''positive'' or ''negative''. Like charges repel each other and ...
s and observers. The fact that the electromagnetic field shows relativistic effects becomes clear by carrying out a simple thought experiment. * An observer measures a charge at rest in frame . The observer will detect a static electric field. As the charge is stationary in this frame, there is no electric current, so the observer does not observe any magnetic field. * The other observer in frame moves at velocity relative to and the charge. ''This'' observer sees a different electric field because the charge moves at velocity in their rest frame. The motion of the charge corresponds to an
electric current An electric current is a flow of charged particles, such as electrons or ions, moving through an electrical conductor or space. It is defined as the net rate of flow of electric charge through a surface. The moving particles are called charge c ...
, and thus the observer in frame also sees a magnetic field. The electric and magnetic fields transform differently from space and time, but exactly the same way as relativistic angular momentum and the boost vector. The electromagnetic field strength tensor is given by F^ = \begin 0 & -\fracE_x & -\fracE_y & -\fracE_z \\ \fracE_x & 0 & -B_z & B_y \\ \fracE_y & B_z & 0 & -B_x \\ \fracE_z & -B_y & B_x & 0 \end \text(+,-,-,-)\text. in
SI units The International System of Units, internationally known by the abbreviation SI (from French ), is the modern form of the metric system and the world's most widely used system of measurement. It is the only system of measurement with official st ...
. In relativity, the Gaussian system of units is often preferred over SI units, even in texts whose main choice of units is SI units, because in it the electric field and the magnetic induction have the same units making the appearance of the
electromagnetic field tensor In electromagnetism, the electromagnetic tensor or electromagnetic field tensor (sometimes called the field strength tensor, Faraday tensor or Maxwell bivector) is a mathematical object that describes the electromagnetic field in spacetime. T ...
more natural. Consider a Lorentz boost in the -direction. It is given by _\nu = \begin \gamma & -\gamma\beta & 0 & 0\\ -\gamma\beta & \gamma & 0 & 0\\ 0 & 0 & 1 & 0\\ 0 & 0 & 0 & 1\\ \end, \qquad F^ = \begin 0 & E_x & E_y & E_z \\ -E_x & 0 & B_z & -B_y \\ -E_y & -B_z & 0 & B_x \\ -E_z & B_y & -B_x & 0 \end \text(-,+,+,+)\text, where the field tensor is displayed side by side for easiest possible reference in the manipulations below. The general transformation law becomes F^ = _\mu _\nu F^. For the magnetic field one obtains \begin B_ &= F^ = _\mu _\nu F^ = _2 _3 F^ = 1 \times 1 \times B_x \\ &= B_x, \\ B_ &= F^ = _\mu _\nu F^ = _3 _\nu F^ = _3 _0 F^ + _3 _1 F^ \\ &= 1 \times (-\beta\gamma) (-E_z) + 1 \times \gamma B_y = \gamma B_y + \beta\gamma E_z \\ &= \gamma\left(\mathbf - \boldsymbol \times \mathbf\right)_y \\ B_ &= F^ = _\mu _\nu F^ = _\mu _2 F^ = _0 _2 F^ + _1 _2 F^ \\ &= (-\gamma\beta) \times 1\times E_y + \gamma \times 1 \times B_z = \gamma B_z - \beta\gamma E_y \\ &= \gamma\left(\mathbf - \boldsymbol \times \mathbf\right)_z \end For the electric field results \begin E_ &= F^ = _\mu _\nu F^ = _1 _0 F^ + _0 _1 F^ \\ &= (-\gamma\beta)(-\gamma\beta)(-E_x) + \gamma\gamma E_x = -\gamma^2\beta^2(E_x) + \gamma^2 E_x = E_x(1 - \beta^2)\gamma^2 \\ &= E_x, \\ E_ &= F^ = _\mu _\nu F^ = _\mu _2 F^ = _0 _2 F^ + _1 _2 F^ \\ &= \gamma \times 1 \times E_y + (-\beta\gamma) \times 1 \times B_z = \gamma E_y - \beta\gamma B_z \\ &= \gamma\left(\mathbf + \boldsymbol \times \mathbf\right)_y \\ E_ &= F^ = _\mu _\nu F^ = _\mu _3 F^ = _0 _3 F^ + _1 _3 F^ \\ &= \gamma \times 1 \times E_z - \beta\gamma \times 1 \times (-B_y) = \gamma E_z + \beta\gamma B_y \\ &= \gamma\left(\mathbf + \boldsymbol \times \mathbf\right)_z. \end Here, is used. These results can be summarized by \begin \mathbf_ &= \mathbf_\parallel \\ \mathbf_ &= \mathbf_\parallel \\ \mathbf_ &= \gamma \left( \mathbf_\bot + \boldsymbol \times \mathbf_\bot \right) = \gamma \left( \mathbf + \boldsymbol \times \mathbf \right)_\bot,\\ \mathbf_ &= \gamma \left( \mathbf_\bot - \boldsymbol \times \mathbf_\bot \right) = \gamma \left( \mathbf - \boldsymbol \times \mathbf \right)_\bot, \end and are independent of the metric signature. For SI units, substitute . refer to this last form as the view as opposed to the ''geometric view'' represented by the tensor expression F^ = _\mu _\nu F^, and make a strong point of the ease with which results that are difficult to achieve using the view can be obtained and understood. Only objects that have well defined Lorentz transformation properties (in fact under ''any'' smooth coordinate transformation) are geometric objects. In the geometric view, the electromagnetic field is a six-dimensional geometric object in ''spacetime'' as opposed to two interdependent, but separate, 3-vector fields in ''space'' and ''time''. The fields (alone) and (alone) do not have well defined Lorentz transformation properties. The mathematical underpinnings are equations and that immediately yield . One should note that the primed and unprimed tensors refer to the ''same event in spacetime''. Thus the complete equation with spacetime dependence is F^\left(x'\right) = _\mu _\nu F^\left(\Lambda^ x'\right) = _\mu _\nu F^(x). Length contraction has an effect on charge density and current density , and time dilation has an effect on the rate of flow of charge (current), so charge and current distributions must transform in a related way under a boost. It turns out they transform exactly like the space-time and energy-momentum four-vectors, \begin \mathbf' &= \mathbf - \gamma\rho v\mathbf + \left( \gamma - 1 \right)(\mathbf \cdot \mathbf)\mathbf \\ \rho' &= \gamma \left(\rho - \mathbf \cdot \frac\right), \end or, in the simpler geometric view, j^ = _\mu j^\mu. Charge density transforms as the time component of a four-vector. It is a rotational scalar. The current density is a 3-vector. The Maxwell equations are invariant under Lorentz transformations.


Spinors

Equation hold unmodified for any representation of the Lorentz group, including the bispinor representation. In one simply replaces all occurrences of by the bispinor representation , The above equation could, for instance, be the transformation of a state in Fock space describing two free electrons.


Transformation of general fields

A general ''noninteracting'' multi-particle state (Fock space state) in
quantum field theory In theoretical physics, quantum field theory (QFT) is a theoretical framework that combines Field theory (physics), field theory and the principle of relativity with ideas behind quantum mechanics. QFT is used in particle physics to construct phy ...
transforms according to the rule where is the Wigner's little group and is the representation of .


See also


Footnotes


Notes


References


Websites

* *


Papers

* * * * * * * . See also
English translation
* * * eqn (55). * * * * *


Books

* * * * * * * * * * * * * * * * * * * * * * * * * * * * *


Further reading

* * *


External links


Derivation of the Lorentz transformations
This web page contains a more detailed derivation of the Lorentz transformation with special emphasis on group properties.

This webpage poses a problem, the solution of which is the Lorentz transformation, which is presented graphically in its next page.

– a chapter from an online textbook
Warp Special Relativity Simulator
A computer program demonstrating the Lorentz transformations on everyday objects. * visualizing the Lorentz transformation.
MinutePhysics video
on
YouTube YouTube is an American social media and online video sharing platform owned by Google. YouTube was founded on February 14, 2005, by Steve Chen, Chad Hurley, and Jawed Karim who were three former employees of PayPal. Headquartered in ...
explaining and visualizing the Lorentz transformation with a mechanical Minkowski diagram
Interactive graph
on Desmos (graphing) showing Lorentz transformations with a virtual Minkowski diagram
Interactive graph
on Desmos showing Lorentz transformations with points and hyperbolas

''from John de Pillis.'' Online Flash animations of Galilean and Lorentz frames, various paradoxes, EM wave phenomena, ''etc''. {{Authority control Special relativity Mathematical physics Spacetime Coordinate systems Hendrik Lorentz