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Encyclopedia > Lorentz scalar

In physics a Lorentz scalar is a scalar which is invariant under a Lorentz transformation. A Lorentz scalar is generated from vectors and tensors. While the vectors and tensors are altered by Lorentz transformations, scalars are unchanged. A Superconductor demonstrating the Meissner Effect. ... The term scalar is used in mathematics, physics, and computing basically for quantities that are characterized by a single numeric value and/or do not involve the concept of direction. ... A Lorentz transformation (LT) is a linear transformation that preserves the spacetime interval between any two events in Minkowski space, while leaving the origin fixed (=rotation of Minkowski space). ...

Contents


Simple scalars in special relativity

The length of a position vector

World lines for two particles at different speeds.
World lines for two particles at different speeds.

In Special relativity the location of a particle in 4-dimensional spacetime is given by its world line Image File history File links Fermi_walker_1. ... Special relativity (SR) or the special theory of relativity is the physical theory published in 1905 by Albert Einstein in his article On the Electrodynamics of Moving Bodies. It replaced Newtonian notions of space and time and incorporated electromagnetism as represented by Maxwells equations. ... World line of the orbit of the Earth depicted in two spatial dimensions X and Y (the plane of the Earth orbit) and a time dimension, usually put as the vertical axis. ... World line of the orbit of the Earth depicted in two spatial dimensions X and Y (the plane of the Earth orbit) and a time dimension, usually put as the vertical axis. ...

x^{mu} = (ct, mathbf{x} )

where mathbf{x} = mathbf{v} t is the position in 3-dimensional space of the particle, mathbf{v} is the velocity in 3-dimensional space and c is the speed of light. Cherenkov effect in a swimming pool nuclear reactor. ...


The "length" of the vector is a Lorentz scalar and is given by

x_{mu} x^{mu} = eta_{mu nu} x^{mu} x^{nu} = (ct)^2 - mathbf{x} cdot mathbf{x} equiv tau^2

where τ is c times the proper time as measured by a clock in the rest frame of the particle and the metric is given by

eta^{munu} =eta_{munu} = begin{pmatrix} 1 & 0 & 0 & 0 0 & -1 & 0 & 0 0 & 0 & -1 & 0 0 & 0 & 0 & -1 end{pmatrix}.

This is a time-like metric. Often the Minkowski metric is used in which the signs of the ones are reversed. In physics and mathematics, Minkowski space (or Minkowski spacetime) is the mathematical setting in which Einsteins theory of special relativity is most conveniently formulated. ...

eta^{munu} =eta_{munu} = begin{pmatrix} -1 & 0 & 0 & 0 0 & 1 & 0 & 0 0 & 0 & 1 & 0 0 & 0 & 0 & 1 end{pmatrix}.

This is a space-like metric. In the Minkowski metric the space-like interval s is defined as

x_{mu} x^{mu} = eta_{mu nu} x^{mu} x^{nu} = mathbf{x} cdot mathbf{x} - (ct)^2 equiv s^2.

We use the Minkowski metric in the rest of this article.


The length of a velocity vector

The velocity vectors in spacetime for a particle at two different speeds. In relativity an acceleration is equivalent to a rotation in spacetime
The velocity vectors in spacetime for a particle at two different speeds. In relativity an acceleration is equivalent to a rotation in spacetime

The velocity in spacetime is defined as Image File history File links Fermi_walker_2. ...

v^{mu} equiv {dx^{mu} over dtau} = left (c {dt over dtau}, { dt over dtau}{dmathbf{x} over dt} right ) = left ( gamma , gamma { mathbf{v} over c } right )

where

gamma equiv { 1 over {sqrt {1 - {{mathbf{v} cdot mathbf{v} } over c^2} } } }.

The magnitude of the 4-velocity is a Lorentz scalar and is minus one,

vμvμ = − 1.

The 4-velocity is therefore, not only a representation of the velocity in spacetime, is is also a unit vector in the direction of the position of the particle in spacetime.


The inner product of acceleration and velocity

Diagram 1. Changing views of spacetime along the world line of a rapidly accelerating observer.

In this animation, the dashed line is the spacetime trajectory ("world line") of a particle. The balls are placed at regular intervals of proper time along the world line. The solid diagonal lines are the light cones for the observer's current event, and intersect at that event. The small dots are other arbitrary events in the spacetime. For the observer's current instantaneous inertial frame of reference, the vertical direction indicates the time and the horizontal direction indicates distance.

The slope of the world line (deviation from being vertical) is the velocity of the particle on that section of the world line. So at a bend in the world line the particle is being accelerated. Note how the view of spacetime changes when the observer accelerates, changing the instantaneous inertial frame of reference. These changes are governed by the Lorentz transformations. Also note that:
• the balls on the world line before/after future/past accelerations are more spaced out due to time dilation.
• events which were simultaneous before an acceleration are at different times afterwards (due to the relativity of simultaneity),
• events pass through the light cone lines due to the progression of proper time, but not due to the change of views caused by the accelerations,and
• the world line always remains within the future and past light cones of the current event.

The 4-acceleration is given by Image File history File links Source of program used to generate image: //GPL #include <stdio. ... World line of the orbit of the Earth depicted in two spatial dimensions X and Y (the plane of the Earth orbit) and a time dimension, usually put as the vertical axis. ... World line of the orbit of the Earth depicted in two spatial dimensions X and Y (the plane of the Earth orbit) and a time dimension, usually put as the vertical axis. ... Proper time is time as measured by the clock for an observer who is traveling through spacetime. ... In special relativity, a light cone is the pattern describing the temporal evolution of a flash of light in Minkowski spacetime. ... Relativity of simultaneity means that events that are considered to be simultaneous in one reference frame are not simultaneous in another reference frame moving with respect to the first. ...

a^{mu} equiv {dv^{mu} over dtau}.

The 4-acceleration is always perpendicular to the 4-velocity

0 = {1 over 2} {d over dtau} left ( v_{mu}v^{mu} right ) = {d v_{mu} over dtau} v^{mu} = a_{mu} v^{mu}.

Therefore, we can regard acceleration in spacetime as simply a rotation of the 4-velocity. The inner product of the acceleration and the velocity is a Lorentz scalar and is zero. This rotation is simply an expression of energy conservation:

{d E over dtau} = mathbf{F} cdot { mathbf{v} over c}

where E is the energy of a particle and mathbf{F} is the 3-force on the particle.


Energy, rest mass, 3-momentum, and 3-speed from 4-momentum

See [Ref. 2, P. 65]. A space-like metric is used.


The 4-momentum of a particle is

p^{mu} = m v^{mu} = left ( gamma m , gamma { m mathbf{v} over c } right ) = left ( gamma m , { mathbf{p} over c } right ) = left ( {E over c^2 } , { mathbf{p} over c } right )

where m is the particle rest mass, mathbf{p} is the momentum in 3-space, and

E = γmc2

is the energy of the particle.


Measurement of the energy of a particle

Consider a second particle with 4-velocity u and a 3-velocity mathbf{u}_2. In the rest frame of the second particle the inner product of u with p is proportional to the energy of the first particle

p_{mu} u^{mu} = - { E_1 over c^2}

where the subscript 1 indicates the first particle.


Since the relationship is true in the rest frame of the second particle, it is true in any reference frame. E1, the energy of the first particle in the frame of the second particle, is a Lorentz scalar. Therefore

{ E_1 over c^2} = gamma_1 gamma_2 m_1 - gamma_2 mathbf{p}_1 cdot mathbf{u}_2

in any intertial reference frame, where E1 is still the energy of the first particle in the frame of the second particle .


Measurement of the rest mass of the particle

In the rest frame of the particle the inner product of the momentum is


pμpμ = − m2.


Therefore m2 is a Lorentz scalar. The relationship remains true independent of the frame in which the inner product is calculated.


Measurement of the 3-momentum of the particle

Note that

left ( p_{mu} u^{mu} right )^2 + p_{mu} p^{mu} = { E_1^2 over c^4} -m^2 = left ( gamma_1^2 -1 right ) m^2 = gamma_1^2 { {mathbf{v}_1 cdot mathbf{v}_1 } over c^2 }m^2 = mathbf{p}_1 cdot mathbf{p}_1.

The square of the magnitude of the 3-momentum of the particle as measured in the frame of the second particle is a Lorentz scalar.


Measurement of the 3-speed of the particle


The 3-speed, in the frame of the second particle, can be constructed from two Lorentz scalars


v_1^2 = mathbf{v}_1 cdot mathbf{v}_1 = { { mathbf{p}_1 cdot mathbf{p}_1 c^6 } over { E_1^2 } }.


More complicated scalars

Scalars may also be constructed from the tensors and vectors, from the contraction of tensors, or combinations of contractions of tensors and vectors.


See also

Albert Einstein
Fermi-Walker transport

For other topics related to Einstein see Einstein (disambiguation). ... Fermi Walker transport is a process in General relativity to define a coordinate system or reference frame such that all curvature in the frame is due to the presence of mass/energy density and not to arbitrary spin or rotation of the frame. ...

References

[1] Einstein, A. (1961). Relativity: The Special and General Theory, New York: Crown. ISBN 0-517-029618.
[2] Misner, Charles; Thorne, Kip S. & Wheeler, John Archibald (1973). Gravitation, San Francisco: W. H. Freeman. ISBN 0-7167-0344-0.
[3] Landau, L. D. and Lifshitz, E. M. (1975). Classical Theory of Fields (Fourth Revised English Edition), Oxford: Pergamon. ISBN 0-08-018176-7.



edit General subfields within physics

Atomic, molecular, and optical physics | Classical mechanics | Condensed matter physics | Continuum mechanics | Electromagnetism | Special relativity | General relativity | Particle physics | Quantum field theory | Quantum mechanics | Statistical mechanics | Thermodynamics A Superconductor demonstrating the Meissner Effect. ... Atomic, molecular, and optical physics is the study of matter-matter and light-matter interactions on the scale of single atoms or structures containing a few atoms. ... Classical mechanics is a branch of physics which studies the deterministic motion of objects. ... Condensed matter physics is the field of physics that deals with the macroscopic physical properties of matter. ... Continuum mechanics is a branch of physics (specifically mechanics) that deals with continuous matter, including both solids and fluids (i. ... Electromagnetism is the physics of the electromagnetic field: a field, encompassing all of space, which exerts a force on those particles that possess the property of electric charge, and is in turn affected by the presence and motion of such particles. ... Special relativity (SR) or the special theory of relativity is the physical theory published in 1905 by Albert Einstein in his article On the Electrodynamics of Moving Bodies. It replaced Newtonian notions of space and time and incorporated electromagnetism as represented by Maxwells equations. ... It has been suggested that Einsteins theory of gravitation be merged into this article or section. ... Particles erupt from the collision point of two relativistic (100 GeV per nucleon) gold ions in the STAR detector of the Relativistic Heavy Ion Collider. ... Quantum field theory (QFT) is the application of quantum mechanics to fields. ... A simple introduction to this subject is provided in Basics of quantum mechanics. ... Statistical mechanics is the application of statistics, which includes mathematical tools for dealing with large populations, to the field of mechanics, which is concerned with the motion of particles or objects when subjected to a force. ... Thermodynamics (from the Greek thermos meaning heat and dynamis meaning power) is a branch of physics that studies the effects of changes in temperature, pressure, and volume on physical systems at the macroscopic scale by analyzing the collective motion of their particles using statistics. ...


  Results from FactBites:
 
Lorentz transformation - Wikipedia, the free encyclopedia (1350 words)
A quantity invariant under Lorentz transformations is known as a Lorentz scalar.
The composition of two Lorentz transformations is a Lorentz transformation and the set of all Lorentz transformations with the operation of composition forms a group called the Lorentz group.
The Lorentz transformations were published in 1897 and 1900 by Joseph Larmor and by Hendrik Lorentz in 1899 and 1904.
Magnetic field - Wikipedia, the free encyclopedia (2330 words)
When an electric charge is moving from the perspective of an observer, the electric field of this charge due to space contraction is no longer seen by the observer as spherically symmetric (and due to time dilation not radial) and must be computed using the Lorentz transformations.
Lorentz transformation of spherically symmetric proper electric field E of moving electric charge (for example, electric field of an electron moving in a conducting wire) from charge's reference frame to non-moving observer's reference frame results in the following term:
Because Lorentz force is charge sign dependent (see above), it results in a charges separation, when a conductor with current is placed in transverse magnetic field—with a buildup of opposite charges on two opposite sides of conductor (in the direction normal to the magnetic field direction)—and the potential difference between these sides can be measured.
  More results at FactBites »


 

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