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Introduction to special relativity
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In physics, special relativity is a theory about the relations between space and time, developed by Albert Einstein in 1905. (See "History of special relativity" for a detailed account and the contributions of Hendrik Lorentz and Henri Poincaré.) It abandoned the notion of absolute time, that is, that the temporal ordering of events and the duration of time intervals are independent from the observer.
The principle of relativity, or Galilean invariance, first described by Galileo Galilei in 1632, states that the fundamental laws of physics are the same in all inertial frames of reference: for example, an observer making experiments below the deck of a ship could not determine whether the ship is stationary or moving at any constant velocity.
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In physics, special relativity is a theory about the relations between space and time, developed by Albert Einstein in 1905. (See "History of special relativity" for a detailed account and the contributions of Hendrik Lorentz and Henri Poincaré.) It abandoned the notion of absolute time, that is, that the temporal ordering of events and the duration of time intervals are independent from the observer.
The principle of relativity, or Galilean invariance, first described by Galileo Galilei in 1632, states that the fundamental laws of physics are the same in all inertial frames of reference: for example, an observer making experiments below the deck of a ship could not determine whether the ship is stationary or moving at any constant velocity. Combined with the (implicit) assumption that time flows the same way for any observer, this implies that all velocities are relative: if one is walking with a velocity v on the ship, and the ship is moving through the sea with a velocity w, one's velocity relative to the sea is v + w. In the late 19th century, Maxwell's equations of electromagnetism were formulated. They predicted that the speed of light (and of electromagnetic waves in general) in a vacuum is c = 1/ (approximately 300 million metres per second, 1079 million kilometres per hour, or 671 million miles per hour), where e0 and µ0 are the electric permittivity and magnetic permeability of a vacuum. This was originally thought to apply only in the frame of reference of the luminiferous aether, the hypothetical substance then believed to be the medium of propagation of electromagnetic waves. The 1887 Michelson–Morley experiment aimed to measure differences in the relative speed of light due to the Earth's motion through the aether, but it yielded a null result.
In his 1905 paper "On the Electrodynamics of Moving Bodies", Albert Einstein dropped the requirement that time is absolute, acknowledged that "the same laws of electrodynamics and optics will be valid for all frames of reference for which the equations of mechanics hold good", and postulated "that light is always propagated in empty space with a definite velocity c which is independent of the state of motion of the emitting body". From this, some predictions can be derived which contradict common intuition and classical mechanics (although these effects are too small to be measured, except with speeds close to that of light or very accurate experiments). The first such prediction described by Einstein is the relativity of simultaneity: observers who are in motion with respect to each other may disagree on whether two events occurred at the same time or one occurred before the other. The other major predictions of special relativity are time dilation (a moving clock ticks more slowly than when it is at rest with respect to the observer), length contraction (a moving rod may be found to be shorter than when it is at rest with respect to the observer), and the equivalence of mass and energy (written as E = mc2). Special relativity predicts a non-linear velocity addition formula which prevents speeds greater than that of light from being observed. All these effects have been experimentally tested on numerous occasions since they were predicted, and were confirmed by those experiments. Just as Galilean relativity is today considered an approximation of special relativity, valid for low speeds, special relativity is nowadays considered an approximation of the theory of general relativity (developed by Einstein in 1915), valid for weak gravitational fields. General relativity postulates that physical laws should appear the same to all observers (an accelerating frame of reference being equivalent to one in which a gravitational field acts), and that gravitation is the effect of the curvature of space-time caused by energy (including mass).
In 1908, Hermann Minkowski reformulated the theory of special relativity based on different postulates of a more geometrical nature.
This approach considers space and time as being different components of a single entity, the spacetime, which is "divided" in different ways by observers in relative motion. Likewise, energy and momentum are the components of the four-momentum, and the electric and magnetic field are the components of the electromagnetic tensor. According to this approach, the speed of light is just a conversion factor stemming from the fact that we use different units to measure distances and durations. Since 1983, this conversion factor has been fixed to 299,792,458 metres per second exactly, by defining the metre as "the length of the path travelled by light in vacuum during a time interval of of a second."
History and background
With the advent of James Clerk Maxwell's equations, a consistent, unified theory of electromagnetism was realized by physicists of the late 19th and early 20th centuries. A consequence of this unification was that electromagnetic waves were discovered to travel at a speed
where is the magnetic permeability and is the electric permittivity. These quantities were properties of the material through which electric and magnetic fields propagated, and so had the property of gauge invariance (they are the same regardless of the velocity at which they are observed). Because of this, electromagnetic waves were also gauge invariant, meaning that all observers should see them traveling at the same speed.
This fact flew in the face of Galilean relativity, which demanded that no velocity could be gauge invariant. Solutions to this quandary were proposed by a number of physicists and mathematicians, including Hendrik Lorentz, who proposed a series of transformation laws that, while violating Galilean relativity, would preserve the results of Maxwell's Equations. Those transformations cause a modification of space-time coordinates when changing frames. Eventually, Henri Poincaré extended the principle of relativity to electrodynamics and argued that the main characteristic of the new mechanics is the impossibility of velocities greater than light. However, both Lorentz and Poincaré only tried to modify Newtonian mechanics, and continued to adhere to the Luminiferous aether and classical definitions of space and time.
Albert Einstein was considering the problem when in 1905 he founded special relativity on two postulates:
- The principle of relativity: that it is impossible to physically distinguish between inertial reference frames that are moving at a constant (or zero) velocity;
- The speed of light in free space is the same for all observers, regardless of their motion relative to the light source.
The final postulate directly contradicted the general understanding of the Galilean principle of relativity, a cornerstone of classical mechanics. Einstein's approach was based on thought experiments that assumed the validity of his two postulates while abandoning other concepts such as the invariance of length and time measurements in different reference frames. In 1908, Hermann Minkowski reformulated the theory based on different postulates of a more geometrical nature.
Special relativity associates the previously independent concepts of space and time as different components of a single entity, the spacetime, on which all 'events' take place. Different observers view these events differently because they use different coordinate systems on this spacetime. In this article the fundamentals of special relativity will be explored using this approach.
Special relativity predicts fundamental deviations from classical expectations in phenomena that involve large speeds. These have been experimentally tested on numerous occasions since its inception, and were confirmed by those experiments. The first such prediction described by Einstein is the relativity of simultaneity: observers who are in motion with respect to each other may disagree on whether two events occurred at the same time or one occurred before the other. The other major predictions of special relativity are time dilation (a moving clock ticks more slowly than when it is at rest with respect to the observer), length contraction (a moving rod may be found to be shorter than when it is at rest with respect to the observer), and the equivalence of mass and energy (written as E = mc2). Special relativity predicts a non-linear velocity addition formula which prevents speeds greater than that of light from being observed.
Today, special relativity (or its generalisation, general relativity) is a fundamental component of our understanding of nature, and the basic structure it provides underlies all modern theories of physics such as the Quantum field theories. In this sense, apart from being a dynamic theory itself, it provides a template to which all physical theories must adhere to. This is to be expected if relativity is indeed a theory about the fundamental structure of space and time.
Reference frames and Galilean relativity: a classical prelude
Galileo first suggested and later Isaac Newton mathematically defined the idea of a reference frame. Essentially, a reference frame is chosen by an observer as a selection of what constitutes the stationary (i.e., the inertial). By definition, choosing a reference frame is equivalent to choosing one particular velocity which is deemed "stationary" or "at rest". For mathematical convenience, we can define "at rest" to be a velocity of zero and the velocity of everything else in the universe can be measured relative to it.[There exists a more technical but mathematically convenient description of reference frames. A reference frame may be considered to be an identification of points in space at different times. That is, it is the identification of space points at different times as being the same point. This concept, particularly useful in making the transition to relativistic spacetime, is described in the language of affine space by VI Arnold in Mathematical Methods in Classical Mechanics, and in the language of fibre bundles by Roger Penrose in The Road to Reality.] Everything in the universe that has a non-zero velocity is in a different reference frame while everything that has zero velocity is in the chosen reference frame (and is, by definition, "at rest"). Another way of describing this can be done by considering a train moving at a constant 100 kilometre per hour velocity past a platform. If we choose the reference frame of the platform, then the train is moving at a speed of 100 kilometres per hour past the platform. Equivalently, we can choose the reference frame of the train and measure the 100 kilometre per second speed of the platform moving past it. To distinguish between the two reference frames physicists call each the "rest frame of the platform" and the "rest frame of the train" respectively. (Occasionally, the two frames will be called simply the "platform frame" and the "train frame".)
Different reference frames are distinguished through measuring relative velocities with respect to each other, but can different reference frames be distinguished through measurements that take place solely in one reference frame? Is there a physics experiment that exists that can tell us whether we are standing on a platform or standing on a train moving at 100 kilometres per hour, without making a comparison to the other reference frame? If such experiments existed, it would be possible to "know" one's velocity without measuring any other reference frame. This implies that there is some absolute standard of velocity that is defined by nature independent of the velocity differences measured between different reference frames. Such "absolute standards" would define an absolute stationary reference frame: nature would have to have a "preferred velocity", if this were the case.
Aristotle thought that all terrestrial objects tend to cease moving and come to rest if there are no forces acting on them. Thus Aristotle thought that there was an absolute standard: a preferred "at rest" reference frame associated with a stationary Earth sited at the center of the universe. To prove his point, Aristotle noted that massive terrestrial objects naturally come to rest when given the impetus to move at other velocities. Since all such objects seem to come to rest eventually, their natural state of rest is stationary.
Galileo challenged Aristotle's claim and argued that the concept of absolute motion is unreal. He proposed that the proofs that Aristotle offered for the existence of an absolute frame of rest were faulty, due to the fact that the reference frames being considered were not free of external influences. The reason that objects given the impetus to move eventually come to rest is that external friction connects them to the massive Earth. Isolating the reference frames and eliminating the friction would allow an object to continue to move forever.
If, as Galileo claimed, there is no absolute frame of rest, then all motion must be relative: that is we can only define a reference frame velocity by measuring it with respect to another velocity. An observer constrained to refer only to physical processes in one reference frame (if, say, the observer were imprisoned inside a windowless train traveling at 100 kilometres per hour) can never distinguish whether, according to some external observer, the train frame is at rest or moving with constant velocity. Any experiment conducted would give the same result in either case.
Isaac Newton accepted Galileo's claims and further extrapolated the ideas to more physically profound conclusions. According to Newton's Laws of Motion, as long as no external forces act on objects that are in the reference frame, the objects will stay in the reference frame indefinitely. Since all reference frames behave in the same fashion, there is no internal difference between one reference frame and another. Physics experiments performed in and observed from a reference frame that is associated with a velocity 100 kilometres per hour will yield the same results as those performed in a reference frame that is associated with a velocity of 0 kilometers per hour. This means that the two reference frames are physically indistinguishable.
In contrast, accelerated reference frames (that is, reference frames that are changing velocity) are experimentally distinguishable. For example, if an observer on a train saw that tea in a cup was sloping up the side of the cup rather than level (in seeming violation of Newton's laws of motion), an inference could be made that train is accelerating and, indeed, the value of the acceleration could be determined by measuring the effect. This experiment can be done without measuring with respect to any other reference frame and therefore there is an absolute frame of "zero acceleration" that can be defined. Reference frames that are not accelerating are all moving at constant uniform velocities with respect to each other, in all of which Newton's laws hold. These are called the inertial reference frames and are fundamental to both classical mechanics and special relativity.
Galilean relativity, a fundamental principle in classical physics, is the principle which defines the qualities of inertial reference frames. It implies that the laws of physics can not depend on velocity, they must stay the same in any inertial reference frame.
Mathematically, it says that if we transform all velocities to a different reference frame, the laws of physics must be unchanged. What is this transformation that must be applied to the velocities? Galileo gave the common-sense 'formula' for adding velocities: if
- particle P is moving at velocity v with respect to reference frame A and
- reference frame A is moving at velocity u with respect to reference frame B, then
- the velocity of P with respect to B is given by v + u.
The formula for transforming coordinates between different reference frames is called the Galilean transformation. The principle of Galilean relativity then demands that laws of physics be unchanged if the Galilean transformation is applied to them. Laws of classical mechanics, like Newton's second law, obey this principle because they have the same form after applying the transformation. As Newton's law involves the derivative of velocity, any constant velocity added in a Galilean transformation to a different reference frame contributes nothing (the derivative of a constant is zero). Addition of a time-varying velocity (corresponding to an accelerated reference frame) will however change the formula (see pseudo force), since Galilean relativity only applies to non-accelerated inertial reference frames.
Time is the same in all reference frames because it is absolute in classical mechanics. All observers measure exactly the same intervals of time and there is such a thing as an absolutely correct clock.
Invariance of length: the Euclidean picture
In special relativity, space and time are joined into a unified four-dimensional continuum called spacetime. To gain a sense of what spacetime is like, we must first look at the Euclidean space of Newtonian physics.
This approach to the theory of special relativity begins with the concept of "length". In everyday experience, it seems that the length of objects remains the same no matter how they are rotated or moved from place to place; as a result the simple length of an object doesn't appear to change or is "invariant". However, as is shown in the illustrations below, what is actually being suggested is that length seems to be invariant in a three-dimensional coordinate system.
The length of a line in a two-dimensional Cartesian coordinate system is given by Pythagoras' theorem:
One of the basic theorems of vector algebra is that the length of a vector does not change when it is rotated. However, a closer inspection tells us that this is only true if we consider rotations confined to the plane. If we introduce rotation in the third dimension, then we can tilt the line out of the plane. In this case the projection of the line on the plane will get shorter. Does this mean length is not invariant? Obviously not. The world is three-dimensional and in a 3D Cartesian coordinate system the length is given by the three-dimensional version of Pythagoras's theorem:
This is invariant under all rotations. The apparent violation of invariance of length only happened because we were 'missing' a dimension. It seems that, provided all the directions in which an object can be tilted or arranged are represented within a coordinate system, the length of an object does not change under rotations. A 3-dimensional coordinate system is enough in classical mechanics because time is assumed absolute and independent of space in that context. It can be considered separately.
Note that invariance of length is not ordinarily considered a dynamic principle, not even a theorem. It is simply a statement about the fundamental nature of space itself. Space as we ordinarily conceive it is called a three-dimensional Euclidean space, because its geometrical structure is described by the principles of Euclidean geometry. The formula for distance between two points is a fundamental property of a Euclidean space, it is called the Euclidean metric tensor (or simply the Euclidean metric). In general, distance formulas are called metric tensors.
Note that rotations are fundamentally related to the concept of length. In fact, one may define length or distance to be that which stays the same (is invariant) under rotations, or define rotations to be that which keep the length invariant. Given any one, it is possible to find the other. If we know the distance formula, we can find out the formula for transforming coordinates in a rotation. If, on the other hand, we have the formula for rotations then we can find out the distance formula.
The Minkowski formulation: introduction of spacetime
After Einstein derived special relativity formally from the (at first sight counter-intuitive) assumption that the speed of light is the same to all observers, Hermann Minkowski built on mathematical approaches used in non-euclidean geometry and on the mathematical work of Lorentz and Poincaré, and showed in 1908 that Einstein's new theory could also be explained by replacing the concept of a separate space and time with a four-dimensional continuum called spacetime. This was a groundbreaking concept, and Roger Penrose has said that relativity was not truly complete until Minkowski reformulated Einstein's work.
The concept of a four-dimensional space is hard to visualise. It may help at the beginning to think simply in terms of coordinates. In three-dimensional space, one needs three real numbers to refer to a point. In the Minkowski space, one needs four real numbers (three space coordinates and one time coordinate) to refer to a point at a particular instant of time. This point at a particular instant of time, specified by the four coordinates, is called an event. The distance between two different events is called the spacetime interval.
A path through the four-dimensional spacetime, usually called Minkowski space, is called a world line. Since it specifies both position and time, a particle having a known world line has a completely determined trajectory and velocity. This is just like graphing the displacement of a particle moving in a straight line against the time elapsed. The curve contains the complete motional information of the particle.
In the same way as the measurement of distance in 3D space needed all three coordinates we must include time as well as the three space coordinates when calculating the distance in Minkowski space (henceforth called M). In a sense, the spacetime interval provides a combined estimate of how far two events occur in space as well as the time that elapses between their occurrence.
But there is a problem. Time is related to the space coordinates, but they are not equivalent. Pythagoras's theorem treats all coordinates on an equal footing (see Euclidean space for more details). We can exchange two space coordinates without changing the length, but we can not simply exchange a space coordinate with time: they are fundamentally different. It is an entirely different thing for two events to be separated in space and to be separated in time. Minkowski proposed that the formula for distance needed a change. He found that the correct formula was actually quite simple, differing only by a sign from Pythagoras's theorem:
where c is a constant and t is the time coordinate.[Originally Minkowski tried to make his formula look like Pythagoras's theorem by introducing the concept of imaginary time and writing -1 as i2. But Wilson, Gilbert, Borel and others proposed that this was unnecessary and introduced real time with the assumption that, when comparing coordinate systems, the change of spatial displacements with displacements in time can be negative. This assumption is expressed in differential geometry using a metric tensor that has a negative coefficient. The different signature of the Minkowski metric means that the Minkowski space has hyperbolic rather than Euclidean geometry.]
Multiplication by c, which has the dimension , converts the time to units of length and this constant has the same value as the speed of light. So the spacetime interval between two distinct events is given by
There are two major points to be noted. Firstly, time is being measured in the same units as length by multiplying it by a constant conversion factor. Secondly, and more importantly, the time-coordinate has a different sign than the space coordinates. This means that in the four-dimensional spacetime, one coordinate is different from the others and influences the distance differently. This new 'distance' may be zero or even negative. This new distance formula, called the metric of the spacetime, is at the heart of relativity. This distance formula is called the metric tensor of M. This minus sign means that a lot of our intuition about distances can not be directly carried over into spacetime intervals. For example, the spacetime interval between two events separated both in time and space may be zero (see below). From now on, the terms distance formula and metric tensor will be used interchangeably, as will be the terms Minkowski metric and spacetime interval.
In Minkowski spacetime the spacetime interval is the invariant length, the ordinary 3D length is not required to be invariant. The spacetime interval must stay the same under rotations, but ordinary lengths can change. Just like before, we were missing a dimension. Note that everything thus far is merely definitions. We define a four-dimensional mathematical construct which has a special formula for distance, where distance means that which stays the same under rotations (alternatively, one may define a rotation to be that which keeps the distance unchanged).
Now comes the physical part. Rotations in Minkowski space have a different interpretation than ordinary rotations. These rotations correspond to transformations of reference frames. Passing from one reference frame to another corresponds to rotating the Minkowski space. An intuitive justification for this is given below, but mathematically this is a dynamical postulate just like assuming that physical laws must stay the same under Galilean transformations (which seems so intuitive that we don't usually recognise it to be a postulate).
Since by definition rotations must keep the distance same, passing to a different reference frame must keep the spacetime interval between two events unchanged. This requirement can be used to derive an explicit mathematical form for the transformation that must be applied to the laws of physics (compare with the application of Galilean transformations to classical laws) when shifting reference frames. These transformations are called the Lorentz transformations. Just like the Galilean transformations are the mathematical statement of the principle of Galilean relativity in classical mechanics, the Lorentz transformations are the mathematical form of Einstein's principle of relativity. Laws of physics must stay the same under Lorentz transformations. Maxwell's equations and Dirac's equation satisfy this property, and hence they are relativistically correct laws (but classically incorrect, since they don't transform correctly under Galilean transformations).
With the statement of the Minkowski metric, the common name for the distance formula given above, the theoretical foundation of special relativity is complete. The entire basis for special relativity can be summed up by the geometric statement "changes of reference frame correspond to rotations in the 4D Minkowski spacetime, which is defined to have the distance formula given above". The unique dynamical predictions of SR stem from this geometrical property of spacetime. Special relativity may be said to be the physics of Minkowski spacetime. In this case of spacetime, there are six independent rotations to be considered. Three of them are the standard rotations on a plane in two directions of space. The other three are rotations in a plane of both space and time: These rotations correspond to a change of velocity, and are described by the traditional Lorentz transformations.
As has been mentioned before, one can replace distance formulas with rotation formulas. Instead of starting with the invariance of the Minkowski metric as the fundamental property of spacetime, one may state (as was done in classical physics with Galilean relativity) the mathematical form of the Lorentz transformations and require that physical laws be invariant under these transformations. This makes no reference to the geometry of spacetime, but will produce the same result. This was in fact the traditional approach to SR, used originally by Einstein himself. However, this approach is often considered to offer less insight and be more cumbersome than the more natural Minkowski formalism.
Reference frames and Lorentz transformations: relativity revisited
We have already discussed that in classical mechanics coordinate frame changes correspond to Galilean transfomations of the coordinates. Is this adequate in the relativistic Minkowski picture?
Suppose there are two people, Bill and John, on separate planets that are moving away from each other. Bill and John are on separate planets so they both think that they are stationary. John draws a graph of Bill's motion through space and time and this is shown in the illustration below:
John sees that Bill is moving through space as well as time but Bill thinks he is moving through time alone. Bill would draw the same conclusion about John's motion. In fact, these two views, which would be classically considered a difference in reference frames, are related simply by a coordinate transformation in M. Bill's view of his own world line and John's view of Bill's world line are related to each other simply by a rotation of coordinates. One can be transformed into the other by a rotation of the time axis. Minkowski geometry handles transformations of reference frames in a very natural way.
Changes in reference frame, represented by velocity transformations in classical mechanics, are represented by rotations in Minkowski space. These rotations are called Lorentz transformations. They are different from the Galilean transformations because of the unique form of the Minkowski metric. The Lorentz transformations are the relativistic equivalent of Galilean transformations. Laws of physics, in order to be relativistically correct, must stay the same under Lorentz transformations. The physical statement that they must be same in all inertial reference frames remains unchanged, but the mathematical transformation between different reference frames changes. Newton's laws of motion are invariant under Galilean rather than Lorentz transformations, so they are immediately recognisable as non-relativistic laws and must be discarded in relativistic physics. Schrödinger's equation is also non-relativistic.
Maxwell's equations are trickier. They are written using vectors and at first glance appear to transform correctly under Galilean transformations. But on closer inspection, several questions are apparent that can not be satisfactorily resolved within classical mechanics (see History of special relativity). They are indeed invariant under Lorentz transformations and are relativistic, even though they were formulated before the discovery of special relativity. Classical electrodynamics can be said to be the first relativistic theory in physics. To make the relativistic character of equations apparent, they are written using 4-component vector-like quantities called 4-vectors. 4-vectors transform correctly under Lorentz transformations, so equations written using 4-vectors are inherently relativistic. This is called the manifestly covariant form of equations. 4-Vectors form a very important part of the formalism of special relativity.
Einstein's postulate: the constancy of the speed of light
Einstein's postulate of a constant speed of light is a natural consequence of the Minkowski formulation.
Proposition 1: When an object is travelling at c in a certain reference frame, the spacetime interval is zero.
Proof. The spacetime interval between the origin-event (0,0,0,0) and an event (x,y,z,t) is
- The distance travelled by an object moving at velocity v for t seconds is:
- giving
- Since the velocity v equals c we have
- Hence the spacetime interval between the events of departure and arrival is given by
Proposition 2: An object travelling at c in one reference frame is travelling at c in all reference frames.
Proof. Let the object move with velocity v when observed from a different reference frame. A change in reference frame corresponds to a rotation in M. Since the spacetime interval must be conserved under rotation, the spacetime interval must be the same in all reference frames. In proposition 1 we showed it to be zero in one reference frame, hence it must be zero in all other reference frames. Hence:
- which implies that
The paths of light rays have a zero spacetime interval, and hence all observers will obtain the same value for the speed of light. Therefore, when assuming that the universe has four dimensions related by Minkowski's formula, the speed of light can be proved constant. Hence Einstein's assumption of its constancy is unnecessary. For other approaches to this conclusion, see the references to Feigenbaum (2008).
Clock delays and rod contractions: more on Lorentz transformations
Another consequence of the invariance of the spacetime interval is that clocks will appear to go slower on objects that are moving relative to you. This is very similar to how the 2D projection of a line rotated into the third-dimension appears to get shorter. Length is not conserved simply because we are ignoring one of the dimensions. Let us return to the example of John and Bill.
John observes the length of Bill's spacetime interval as:
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whereas Bill doesn't think he has traveled in space, so writes:
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The spacetime interval, s2, is invariant. It has the same value for all observers, no matter who measures it or how they are moving in a straight line. This means that Bill's spacetime interval equals John's observation of Bill's spacetime interval so:
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and
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hence
- .
So, if John sees a clock that is at rest in Bill's frame record one second, John will find that his own clock measures between these same ticks an interval t, called coordinate time, which is greater than one second. It is said that clocks in motion slow down, relative to those on observers at rest. This is known as "relativistic time dilation of a moving clock". The time that is measured in the rest frame of the clock (in Bill's frame) is called the proper time of the clock.
In special relativity, therefore, changes in reference frame affect time also. Time is no longer absolute. There is no universally correct clock, time runs at different rates for different observers.
Similarly it can be shown that John will also observe measuring rods at rest on Bill's planet to be shorter in the direction of motion than his own measuring rods.[It should also be made clear that the length contraction result only applies to rods aligned in the direction of motion. At right angles to the direction of motion, there is no contraction.] This is a prediction known as "relativistic length contraction of a moving rod". If the length of a rod at rest on Bill's planet is , then we call this quantity the proper length of the rod. The length of that same rod as measured on John's planet, is called coordinate length, and given by
.
These two equations can be combined to obtain the general form of the Lorentz transformation in one spatial dimension:
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or equivalently:
-
where the Lorentz factor is given by
The above formulas for clock delays and length contractions are special cases of the general transformation.
Alternatively, these equations for time dilation and length contraction (here obtained from the invariance of the spacetime interval), can be obtained directly from the Lorentz transformation by setting X = 0 for time dilation, meaning that the clock is at rest in Bill's frame, or by setting t = 0 for length contraction, meaning that John must measure the distances to the end points of the moving rod at the same time.
A consequence of the Lorentz transformations is the modified velocity-addition formula:
Simultaneity and clock desynchronisation
The last consequence of Minkowski's spacetime is that clocks will appear to be out of phase with each other along the length of a moving object. This means that if one observer sets up a line of clocks that are all synchronised so they all read the same time, then another observer who is moving along the line at high speed will see the clocks all reading different times. This means that observers who are moving relative to each other see different events as simultaneous. This effect is known as "Relativistic Phase" or the "Relativity of Simultaneity". Relativistic phase is often overlooked by students of special relativity, but if it is understood, then phenomena such as the twin paradox are easier to understand.
Observers have a set of simultaneous events around them that they regard as composing the present instant. The relativity of simultaneity results in observers who are moving relative to each other having different sets of events in their present instant.
The net effect of the four-dimensional universe is that observers who are in motion relative to you seem to have time coordinates that lean over in the direction of motion, and consider things to be simultaneous that are not simultaneous for you. Spatial lengths in the direction of travel are shortened, because they tip upwards and downwards, relative to the time axis in the direction of travel, akin to a rotation out of three-dimensional space.
Great care is needed when interpreting spacetime diagrams. Diagrams present data in two dimensions, and cannot show faithfully how, for instance, a zero length spacetime interval appears.
General relativity: a peek forward
Unlike Newton's laws of motion, relativity is not based upon dynamical postulates. It does not assume anything about motion or forces. Rather, it deals with the fundamental nature of spacetime. It is concerned with describing the geometry of the backdrop on which all dynamical phenomena take place. In a sense therefore, it is a meta-theory, a theory that lays out a structure that all other theories must follow. In truth, Special relativity is only a special case. It assumes that spacetime is flat. That is, it assumes that the structure of Minkowski space and the Minkowski metric tensor is constant throughout. In General relativity, Einstein showed that this is not true. The structure of spacetime is modified by the presence of matter. Specifically, the distance formula given above is no longer generally valid except in space free from mass. However, just like a curved surface can be considered flat in the infinitesimal limit of calculus, a curved spacetime can be considered flat at a small scale. This means that the Minkowski metric written in the differential form is generally valid.
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One says that the Minkowski metric is valid locally, but it fails to give a measure of distance over extended distances. It is not valid globally. In fact, in general relativity the global metric itself becomes dependent on the mass distribution and varies through space. The central problem of general relativity is to solve the famous Einstein field equations for a given mass distribution and find the distance formula that applies in that particular case. Minkowski's spacetime formulation was the conceptual stepping stone to general relativity. His fundamentally new outlook allowed not only the development of general relativity, but also to some extent quantum field theories.
Mass-energy equivalence: sunlight and atom bombs
Einstein showed that mass is simply another form of energy. The energy equivalent of rest mass m is . This equivalence implies that mass should be interconvertible with other forms of energy. This is the basic principle behind atom bombs and production of energy in nuclear reactors and stars (like the Sun).
Applications
There is a common perception that relativistic physics is not needed in everyday life. This is not true. Many technologies are critically dependent on relativistic physics:
The postulates of Special Relativity
Einstein developed Special Relativity on the basis of two postulates:
- First postulate - Special principle of relativity - The laws of physics are the same in all inertial frames of reference. In other words, there are no privileged inertial frames of reference.
- Second postulate - Invariance of c - The speed of light in a vacuum is independent of the motion of the light source.
Special Relativity can be derived from these postulates, as was done by Einstein in 1905. Einstein's postulates are still applicable in the modern theory but the origin of the postulates is more explicit. It was shown above how the existence of a universally constant velocity (the speed of light) is a consequence of modeling the universe as a particular four dimensional space having certain specific properties. The principle of relativity is a result of Minkowski structure being preserved under Lorentz transformations, which are postulated to be the physical transformations of inertial reference frames.
External links
Special relativity for a general audience (no math knowledge required)
- An -winning, non-technical introduction (film clips and demonstrations) supported by dozens of pages of further explanations and animations, at levels with or without mathematics.
- Introduction to relativity theory, from the Max Planck Institute for Gravitational Physics.
Special relativity explained (using simple or more advanced math)
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- on Special and General Relativity
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- A basic introduction to concepts of Special and General Relativity, requiring only a knowledge of basic geometry.
- from the University of New South Wales.
- Mathematics of special relativity presented in as simple and comprehensive manner possible within philosophical and historical contexts.
- .
- (1964), by Robert Katz; an introduction ... accessible to any student who has had an introduction to general physics and some slight acquaintance with the calculus."(130 pp; pdf format)
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from John de Pillis. Flash animations of clocks, frames, EM waves, various paradoxes, etc.
See also
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