Status of special relativity


Status of special relativity

Special relativity (SR) is usually concerned with the behaviour of objects and "observers" (inertial reference systems) which remain at rest or are moving at a constant velocity. In this case, the observer is said to be "in an inertial frame of reference". Comparison of the position and time of events as recorded by different inertial observers can be done by using the Lorentz transformation equations. A common misstatement is that SR cannot be used to handle the case of objects and observers who are undergoing acceleration ("non-inertial reference frames"), but this is incorrect. For an example, see the relativistic rocket problem.

SR can correctly predict the behaviour of accelerating bodies in the presence of a constant or zero gravitational field, or those in a rotating reference frame. It is not capable of accurately describing motion in varying gravitational fields; in that case it must be replaced by general relativity. At very small scales, such as at the Planck length and below, it is also possible that special relativity breaks down, due to the effects of quantum gravity. However, at macroscopic scales and in the absence of strong gravitational fields, special relativity is now universally accepted by the physics community and experimental results.

Dependence on definition of units

Because of the freedom one has to select how one defines units of length and time in physics, it is possible to make one of the two postulates of relativity a tautological consequence of the definitions, but one cannot do this for both postulates simultaneously because when combined they have consequences which are independent of one's choice of definition of length and time. For instance, if one defines units of length and time in terms of a physical object (e.g. by defining units of time in terms of transitions of a caesium atom, or length in terms of wavelengths of a krypton atom) then it becomes tautological that the law determining that unit of length or time will be the same in all reference frames, but then theinvariance of "c" is non-trivial. Conversely, if one defines units of length and time in such a way that "c" is necessarily constant, then the second postulate becomes tautological, but the first one does not; for instance, if the length unit is defined in terms of the time unit and a predetermined fixed value of "c", then there is no "a priori" reason why the number of wavelengths of krypton in a unit of length will be the same in all reference frames (or even in all orientations).

Experimental evidence

A number of experiments support special relativity when compared against other theories. These include:

* The Michelson-Morley experiment - round trip speed of light variations (as a function of angle with "aether velocity"), no effect found
* The Hammar experiment - obstruction of ether flow by mass, no effect found
* The Trouton-Noble experiment - torque on a capacitor (as a function of angle with "aether velocity"), no effect found
* The Trouton-Rankine experiment - change in resistance of a coil of wire (as a function of angle with "aether velocity"), no effect found
* The Kennedy-Thorndike experiment - like the Michelson-Morley experiment except with unequal length interferometer arms (again no variation in the round trip speed of light was detected)
* The Ives-Stilwell experiment - transverse doppler shift was confirmed
* Experiments to test emitter theory demonstrated that the speed of light is independent of the speed of the emitter.

The Sagnac effect, a phenomenon that is taken in to account in GPS synchronisation procedures, is predicted by both special relativity and Galilean relativity and is thus neutral evidence as far as special relativity is concerned.

In addition, experimental Tests of general relativity for the most part also verify special relativity, since the laws of special relativity are included as part of General Relativity.

Mathematical consistency

Mathematically, special relativity is internally consistent, being nothing more than the geometry of rotationally symmetric (=isotropic) Minkowski space, together with a requirement that all laws of nature be inertial frame invariant. To date, efforts of many amateur physicists to create thought-experiments within special relativity with genuine logical paradoxes have gone in vain, unless one assumes the existence of objects which do not seem to exist in special relativity (see below). However, it is certainly possible to create thought-experiments which have unintuitive consequences, and which contradict some other theories.

Theories incompatible with relativity

Special relativity is not compatible with the physical existence of the following objects, forces, or laws (except in the "nonrelativistic limit" in which all speeds are much less than "c"):

# Infinitely rigid rods, or any other object which transmits forces at infinite speeds. Note that this would require the existence of a new force which is not currently explained by any of the laws of physics.
# Tachyon particles, unless these particles cannot transmit any information at superluminal speeds, or are somehow not subject to the laws of cause and effect.
# Rulers which are immune to Lorentz contraction. Again, this would require a new force not currently explained by the laws of physics.
# Devices which can record absolute position. Note that the existence of such devices would also contradict Galilean relativity.
# Clocks that are immune to time dilation. Again, this would require a new force not currently explained by the laws of physics.
# Clocks which can record absolute time. Indeed, the concept of absolute time is philosophically inconsistent with Einstein's interpretation of special relativity.
# Forces which can act instantaneously at a distance; this includes Newton's law of gravity and Coulomb's law of electrostatics. Note however that these two laws can be modified (to general relativity and Maxwell's equations respectively) in a manner consistent with or generalizing the theory of special relativity. There are also some laws of physics which act non-locally but do not transmit information at superluminal speeds, and which are thus technically (if not philosophically) consistent with special relativity; the primary example here is the collapse of the wave function.
# Laws of nature which are Galilean invariant instead of Lorentz invariant, or which are not invariant under either of these two transformations.
# The Newtonian velocity addition law v = v_1 + v_2; this law is replaced by the relativistic addition law.
# Conservation of Newtonian momentum defined as p = mv and Newtonian kinetic energy defined as E = egin{matrix}frac{1}{2}end{matrix} mv^2. The equivalent conserved quantities are p = E v / c^2 and E^2 = m^2 c^4 + p^2 c^2 (which reduce to the Newtonian ones in the low-velocity limit). Similarly, Newton's second law in the form F=ma is no longer valid, but must be replaced by F = dp/dt (which is in fact closer to Newton's original formulation of this law).
# The Schrödinger equation, which is the quantization of non-relativistic equation E = p^2 / 2m + V from Newtonian mechanics. This can be replaced by the Dirac equation, Klein-Gordon equation, or quantum field theory.
# Nonrelativistic fluid equations such as the Euler equations and Navier-Stokes equations; these must be replaced by relativistic fluid equations such as the Relativistic Euler equations.
# Additivity of mass; the total mass of a system (as determined by solving the equation E^2 = m^2 c^4 + p^2 c^2, where "E" is the total energy and "p" is the total momentum) is not necessarily equal to the sum of the masses of its components, just as the length of a sum of vectors is not necessarily equal to the sum of the lengths of the individual vectors. Indeed there is a triangle inequality which says that the total mass is always "greater than" or equal to the sum of the individual masses. However, the total mass of a system remains conserved (this is a consequence of conservation of energy and momentum).
# Conservation of particle number is compatible with relativity, but once quantum mechanics is also added, it is possible that this conservation law breaks down, leading to spontaneous particle creation and annihilation. This phenomenon is usually studied within the framework of quantum field theory.
# Wormholes or other objects which affect the topology of spacetime. However, these objects can be compatible with general relativity.

Theories compatible with relativity

Special relativity "is" compatible with

# Translation invariance, rotation invariance, time reversal symmetry, and reflection symmetry of the laws of physics. Indeed, special relativity generalizes and unifies these symmetries via the principle of Lorentz invariance.
# The non-relativistic Doppler shift law, which works fine if time dilation is accounted for; the combination equals "relativistic Doppler".
# Maxwell's equations of electromagnetism. In fact Maxwell's equations combined with the first postulate of special relativity can be used to deduce the second postulate. Actually electromagnetism is greatly simplified by relativity, as "magnetism" is simply the relativistic effect obtained when the simple law of electrostatics is put into a relativistic Universe.
# The Lorentz force law in electromagnetism, subject to the caveats concerning Newton's second law mentioned earlier. Maxwell's equations, combined with the Lorentz force law, can also be used to demonstrate mathematically several consequences of special relativity, such as Lorentz contraction and time dilation, at least for rulers and clocks which operate via electromagnetic forces.
# and are still compatible with special relativity, though as mentioned earlier all forces must now act locally instead of at a distance (and are most likely mediated via fields with finite speed of propagation).
# Classical Yang-Mills theory, which generalizes Maxwell's equations and which govern the classical theory of the weak and strong nuclear forces. Indeed, as with Maxwell's equations, one could use the Yang-Mills equations to deduce the second postulate of special relativity from the first, and can also demonstrate relativistic effects such as Lorentz contraction and time dilation for rulers and clocks that operate via nuclear forces (e.g. atomic clocks). Quantum Yang-Mills theory is a special case of quantum field theory.
# In addition to Maxwell's equations and Yang-Mills equations, related equations such as the wave equation, Dirac equation, Klein-Gordon equation, and Yang-Mills-Higgs equation are also compatible with special relativity. See Relativistic wave equations for further discussion.
# Quantum mechanics, though as mentioned above Schrödinger's equation must now be replaced by another equation. One can view quantum field theory as the natural unification of special relativity with quantum mechanics. However, if one assumes both special relativity and quantum mechanics then one is forced to abandon local hidden variable theories, unless one is willing to adopt interpretations of quantum mechanics such as the many-worlds interpretation; see Bell's theorem for more discussion. For similar reasons the concept of the collapse of a wave function becomes problematic in relativity, though the difficulties are more aesthetic than fundamental in nature. The unification of general relativity and quantum mechanics is a notoriously difficult problem which has not yet been resolved satisfactorily; see quantum gravity.
# General relativity collapses to special relativity in the limit when the strength of the gravitational field tends to zero.
# Hamiltonian mechanics, though the Hamiltonian system often has to incorporate not only point particles, but also the fields which mediate the forces between these particles.
# Conservation laws, such as conservation of mass, energy, momentum, angular momentum and charge. (See however the earlier note about failure of additivity of mass). This can be viewed as a consequence of Noether's theorem from Hamiltonian mechanics. Conservation of particle number is not covered by Noether's theorem and can break down in relativity.
# Lagrangian mechanics (the principle of least action), although as with Hamiltonian mechanics, the Lagrangian system often needs to incorporate fields as well as particles. Also, the Lagrangian of a point particle often needs to be written using proper time instead of absolute time or time in a co-ordinate frame.
# Relativistic quantum chemistry

As these examples show, special relativity affects all aspects of physics, and is not purely concerned with light. Indeed, in a very literal sense, light is merely the most visible phenomenon in physics which involves the constant "c".

Alternatives to special relativity

# emitter theory: largely abandoned nowadays. Any theory that proposes that the velocity of light should depend on the speed of the object emitting the light is inconsistent with observations of binary stars, since the light from these stars would vary in arrival time depending on where the stars were in their orbits.
# "Absolute" aether: largely abandoned, due to null results such as the Michelson-Morley experiment
# ether drag theories: also largely abandoned, due to the range of dragging theories using apparently "ad hoc" hypotheses and coefficients, and the lack of a deeper guiding principle or law (but see quantum gravity and frame-dragging).
# Lorentz ether theory: This theory gives the same predictions in any experimental setting as special relativity. However, the two theories are ontologically and philosophically very different. As a result, they suggest different ways to extend or modify the theory (e.g., ways of understanding gravity).

See also

*Tests of general relativity


Wikimedia Foundation. 2010.

Look at other dictionaries:

  • Special relativity — (SR) (also known as the special theory of relativity or STR) is the physical theory of measurement in inertial frames of reference proposed in 1905 by Albert Einstein (after considerable contributions of Hendrik Lorentz and Henri Poincaré) in the …   Wikipedia

  • Relativity of simultaneity — thumb|Event B is simultaneous with A in the green reference frame, but it occurredbefore in the blue frame, and will occur later in the red frame.The relativity of simultaneity is the concept that simultaneity is not absolute, but dependent on… …   Wikipedia

  • General relativity — For a generally accessible and less technical introduction to the topic, see Introduction to general relativity. General relativity Introduction Mathematical formulation Resources …   Wikipedia

  • Criticism of relativity theory — Criticism of Albert Einstein s theory of relativity was mainly expressed in the early years after its publication on a scientific, pseudoscientific, philosophical, or ideological basis. Reasons for criticism were, for example, alternative… …   Wikipedia

  • Introduction to general relativity — General relativity (GR) is a theory of gravitation that was developed by Albert Einstein between 1907 and 1915. According to general relativity, the observed gravitational attraction between masses results from the warping of space and time by… …   Wikipedia

  • Tests of general relativity — General relativity Introduction Mathematical formulation Resources Fundamental concepts …   Wikipedia

  • Mathematics of general relativity — For a generally accessible and less technical introduction to the topic, see Introduction to mathematics of general relativity. General relativity Introduction Mathematical formulation Resources …   Wikipedia

  • History of general relativity — Creation of General Relativity Early investigations As Albert Einstein later said, the reason for the development of general relativity was that the preference of inertial motions within special relativity was unsatisfactory, while a theory which …   Wikipedia

  • Relativistic wave equations — Before the creation of quantum field theory, physicists attempted to formulate versions of the Schrödinger equation which were compatible with special relativity. Such equations are called relativistic wave equations. The first such equation was… …   Wikipedia

  • cosmos — /koz meuhs, mohs/, n., pl. cosmos, cosmoses for 2, 4. 1. the world or universe regarded as an orderly, harmonious system. 2. a complete, orderly, harmonious system. 3. order; harmony. 4. any composite plant of the genus Cosmos, of tropical… …   Universalium