• Mechanics
    • —
      • M1. Vectors vs. Vector Quantities; Scalars vs. Scalar Quantities
      • M2. Significance of Newton’s First Law
      • M3. Newton’s Third Law: Its Formulation, Its Significance
      • M4. Momentum Conservation; Its Central Role
      • M5. Space Homogeneity And Momentum Conservation
      • M6. Inertial Mass
      • M7. Gravitational Mass
    • —
      • M8. Angular Momentum Characteristics
      • M9. Vanishing Of Total Internal Torque
      • M10. The Isotropy Of Space And Angular-Momentum Conservation
      • M11. Energy, A Central Concept
      • M12. Work And Its Relation To Kinetic And Potential Energy
      • M13. From Kepler’s Laws To Universal Gravitation
      • M14. Error And Uncertainty Distinguished
  • Thermodynamics
    • —
      • T1. What Is Thermodynamics
      • T2. Heat Vs. Internal Energy
      • T3. Equipartition And Degrees Of Freedom
      • T4. Frozen Degrees Of Freedom
      • T5. Six Versions Of The Second Law Of Thermodynamics
    • —
      • T6. Available And Unavailable Energy
      • T7. Entropy On Two Levels
      • T8. Subtleties Of Entropy
      • T9. The Arrow Of Time
  • Electricity & Magnetism
    • —
      • E1. Charge
      • E2. Early Links Between Electricity And Magnetism
      • E3. Monopoles, Not!
      • E4. The Q-ℰ-ℬ Triangle
    • —
      • E5. Inductance
      • E6. The Nature Of Light
      • E7. Why Light Travels At Speed C
      • E8. Notes On The History Of Electromagnetism
  • Relativity
    • —
      • R1. Agreement And Disagreement: Relativistic And Classical
      • R2. Transformations: Galilean And Lorentz
      • R3. “Michelson Airspeed Indicator”
      • R4. c = Constant Means Time Must Be Relative
      • R5. More Relativity And More Invariance
      • R6. E = mc2 As Einstein Derived It
    • —
      • R7. Momentum In Relativity, And Another Approach To E = mc2
      • R8. The Fourth Dimension: Spacetime And Momenergy
      • R9. Versions Of The Twin Paradox
      • R10. The Principle Of Equivalence
      • R11. Geometrodynamics
  • Quantum Physics
    • —
      • Q1. Five Key Ideas Of Quantum Mechanics
      • Q2. Granularity
      • Q3. Probability
      • Q4. Annihilation And Creation
      • Q5. Waves And Particles (The de Broglie Equation)
      • Q6. The Uncertainty Principle
      • Q7. Why Is The Hydrogen Atom As Big As It Is?
      • Q8. Localization Of Waves; Relation To Uncertainty Principle
    • —
      • Q9. Planck’s Quantum Not Yet A Photon
      • Q10. Planck’s Constant As The Particle-Wave Link
      • Q11. The Bohr Atom: Obsolete But Important
      • Q12. Bohr’s Key Atomic Postulates
      • Q13. Bohr’s Triumph: Explaining The Rydberg Constant
      • Q14. H-Atom Wave Functions And Classical Correspondence
      • Q15. The Jovian Task: Building The Atoms
      • Q16. Feynman Diagrams
  • Nuclear Physics
    • —
      • N1. Why Are There No Electrons In The Nucleus?
      • N2. The Line Of Nuclear Stability Bends And Ends
      • N3. The “Miracle” Of Nuclear Stability
      • N4. Pauli Letter Proposing What Came To Be Called The Neutrino
    • —
      • N5. Early History Of Radioactivity And Transmutation
      • N6. Bohr-Wheeler Theory Of Fission
      • N7. Sun’s Proton-Proton Cycle
  • General, Historical, Philosophical
    • —
      • G1. Faith In Simplicity As A Driver Of Science
      • G2. Science: Creation Vs. Discovery
      • G3. Is There A Scientific Method?
      • G4. What Is A Theory?
      • G5. The “Great Theories” Of Physics
      • G6. Natural Units, Dimensionless Physics
      • G7. Three Kinds Of Probability
      • G8. The Forces Of Nature
      • G9. Laws That Permit, Laws That Prohibit
    • —
      • G10. Conservation Laws, Absolute And Partial
      • G11. Math As A Tool And A Toy
      • G12. The “System Of The World”: How The Heavens Drove Mechanics
      • G13. The Astromical World, Then And Now
      • G14. Superposition
      • G15. Physics At The End Of The Nineteenth Century: The Seeds Of Rel & QM
      • G16. The Submicroscopic Frontier: Reductionism
      • G17. Submicroscopic Chaos
      • G18. The Future Path Of Science
  • Supplemental
    • Rainbows: Figuring Their Angles
  • Index
Basic PhysicsBasic Physics
A Resource for Teachers by Ken Ford
  • Mechanics
    • —
      • M1. Vectors vs. Vector Quantities; Scalars vs. Scalar Quantities
      • M2. Significance of Newton’s First Law
      • M3. Newton’s Third Law: Its Formulation, Its Significance
      • M4. Momentum Conservation; Its Central Role
      • M5. Space Homogeneity And Momentum Conservation
      • M6. Inertial Mass
      • M7. Gravitational Mass
    • —
      • M8. Angular Momentum Characteristics
      • M9. Vanishing Of Total Internal Torque
      • M10. The Isotropy Of Space And Angular-Momentum Conservation
      • M11. Energy, A Central Concept
      • M12. Work And Its Relation To Kinetic And Potential Energy
      • M13. From Kepler’s Laws To Universal Gravitation
      • M14. Error And Uncertainty Distinguished
  • Thermodynamics
    • —
      • T1. What Is Thermodynamics
      • T2. Heat Vs. Internal Energy
      • T3. Equipartition And Degrees Of Freedom
      • T4. Frozen Degrees Of Freedom
      • T5. Six Versions Of The Second Law Of Thermodynamics
    • —
      • T6. Available And Unavailable Energy
      • T7. Entropy On Two Levels
      • T8. Subtleties Of Entropy
      • T9. The Arrow Of Time
  • Electricity & Magnetism
    • —
      • E1. Charge
      • E2. Early Links Between Electricity And Magnetism
      • E3. Monopoles, Not!
      • E4. The Q-ℰ-ℬ Triangle
    • —
      • E5. Inductance
      • E6. The Nature Of Light
      • E7. Why Light Travels At Speed C
      • E8. Notes On The History Of Electromagnetism
  • Relativity
    • —
      • R1. Agreement And Disagreement: Relativistic And Classical
      • R2. Transformations: Galilean And Lorentz
      • R3. “Michelson Airspeed Indicator”
      • R4. c = Constant Means Time Must Be Relative
      • R5. More Relativity And More Invariance
      • R6. E = mc2 As Einstein Derived It
    • —
      • R7. Momentum In Relativity, And Another Approach To E = mc2
      • R8. The Fourth Dimension: Spacetime And Momenergy
      • R9. Versions Of The Twin Paradox
      • R10. The Principle Of Equivalence
      • R11. Geometrodynamics
  • Quantum Physics
    • —
      • Q1. Five Key Ideas Of Quantum Mechanics
      • Q2. Granularity
      • Q3. Probability
      • Q4. Annihilation And Creation
      • Q5. Waves And Particles (The de Broglie Equation)
      • Q6. The Uncertainty Principle
      • Q7. Why Is The Hydrogen Atom As Big As It Is?
      • Q8. Localization Of Waves; Relation To Uncertainty Principle
    • —
      • Q9. Planck’s Quantum Not Yet A Photon
      • Q10. Planck’s Constant As The Particle-Wave Link
      • Q11. The Bohr Atom: Obsolete But Important
      • Q12. Bohr’s Key Atomic Postulates
      • Q13. Bohr’s Triumph: Explaining The Rydberg Constant
      • Q14. H-Atom Wave Functions And Classical Correspondence
      • Q15. The Jovian Task: Building The Atoms
      • Q16. Feynman Diagrams
  • Nuclear Physics
    • —
      • N1. Why Are There No Electrons In The Nucleus?
      • N2. The Line Of Nuclear Stability Bends And Ends
      • N3. The “Miracle” Of Nuclear Stability
      • N4. Pauli Letter Proposing What Came To Be Called The Neutrino
    • —
      • N5. Early History Of Radioactivity And Transmutation
      • N6. Bohr-Wheeler Theory Of Fission
      • N7. Sun’s Proton-Proton Cycle
  • General, Historical, Philosophical
    • —
      • G1. Faith In Simplicity As A Driver Of Science
      • G2. Science: Creation Vs. Discovery
      • G3. Is There A Scientific Method?
      • G4. What Is A Theory?
      • G5. The “Great Theories” Of Physics
      • G6. Natural Units, Dimensionless Physics
      • G7. Three Kinds Of Probability
      • G8. The Forces Of Nature
      • G9. Laws That Permit, Laws That Prohibit
    • —
      • G10. Conservation Laws, Absolute And Partial
      • G11. Math As A Tool And A Toy
      • G12. The “System Of The World”: How The Heavens Drove Mechanics
      • G13. The Astromical World, Then And Now
      • G14. Superposition
      • G15. Physics At The End Of The Nineteenth Century: The Seeds Of Rel & QM
      • G16. The Submicroscopic Frontier: Reductionism
      • G17. Submicroscopic Chaos
      • G18. The Future Path Of Science
  • Supplemental
    • Rainbows: Figuring Their Angles
  • Index

R8. The Fourth Dimension: Spacetime And Momenergy

Based on Basic Physics Feature 118

The mixing together of space and time in the Lorentz transformation, and the concept of a spacetime “interval” between two events lead one to the idea of a four-dimensional spacetime, filled with world lines and events. Each event is a point in spacetime located by three space coordinates and one time coordinate, and any pair of events is separated by a spacetime “distance,” the interval. With this picture of spacetime, one may quite naturally think of the four coordinates (three of space and one of time) locating an event as being the four components of a single vector. To avoid confusion with old-fashioned three-dimensional vectors, this is called a four-vector. This spacetime four-vector is a generalization of the idea of a position vector in ordinary space. Instead of locating a point in space, it locates an event in spacetime. Its components are x, y, z, and ct, and the square of its length is x2 + y2 + z2 – (ct)2. The minus sign preceding the contribution of the fourth component is important and distinguishes the fourth component from the first three. The length of the four-vector is a constant for all observers, for it is just the interval under a new name.1 If the squared length is positive, the interval is said to be “spacelike.” If it is negative, the interval is “timelike.”2

In Newtonian mechanics, several different vector quantities appear: position, velocity, acceleration, momentum, force. One extends the idea of the position vector to the four-dimensional world by appending ct to it as a fourth component. This extension has several technical advantages in the theory of relativity, the most important of which, for our present purpose, is that the length of the four-vector is an invariant quantity, whereas the ordinary three-dimensional length is not invariant, but depends on the state of motion of the observer. This process of generalizing vectors from three to four dimensions can be carried out not only for the position vector but for all of the vectors of mechanics, and some unexpected and interesting partnerships turn up. Next in interest to the joining together of space and time is the union of momentum and energy.

Momentum, because it is a three-dimensional vector, may be expressed in component form:

Since space has acquired a fourth dimension—time—momentum needs a fourth component, or time component. Remarkably, energy (or, more exactly, energy divided by the speed of light) proves to be the time component of momentum:

This merger of two of the key concepts of mechanics into a single four-dimensional entity was achieved by Hermann Minkowski in 1908, and later dubbed momenergy by John Wheeler. Soon other mergers were recognized, such as electric charge with electric current, and electric field with magnetic field, so that before long all of classical physics became imbedded in the new spacetime.

The four-dimensional momentum-energy (or momenergy) vector has a length, whose square is defined in much the same way as the square of the space-time interval. It is

px2 + py2 + pz2 – pt2 .

This combination, as a little algebra reveals, is exactly equal to the simple constant – m2c2, the same for all observers. Although both the energy and momentum of a particle depend on the state of motion of the observer, here is a certain invariant combination about which all observers agree.

Although spacetime vectors connecting pairs of events may be either “spacelike” or “timelike,” the momentum-energy vector of a material particle is always timelike, as indicated by the minus sign on the right of the equation

px2 + py2 + pz2 – pt2 = – m2c2 .

For a massless particle, always standing apart as a special case, the momentum-energy vector has zero length, although momentum and energy are of course not separately zero . Such a vector is called a null vector. A briefer and often useful way to write this equation, valid for particles with or without mass, is

E2 = p2c2 + m2c4 .

This expresses the total energy of a particle in terms of its momentum and its mass.

In general, what does the fourth component of any vector mean? It scarcely seems an adequate answer to say it is a component pointing in the time direction. We can appreciate the meaning of north, south, east, west, up, and down. But which direction is the time direction? Unfortunately humans don’t seem able to visualize four dimensions, yet that is just what the theory of relativity is asking us to do. The best one can do is try and extrapolate one’s pattern of thought from two dimensions to three and on to four, to form analogies, and to make use of what has already been learned about space and time. By way of analogy, we might think of a two-dimensional worm living out its life in a plane. The worm would know that space has two dimensions. If a more learned worm tried to explain to him the meaning of the third dimension, he might become irritated and exclaim, “But what can you mean by a third dimension It is nothing you can point to; it is not anything we can experience.” We three-dimensional creatures must likewise be content to accept the fourth dimension as something at best vaguely visualizable, yet vitally important in deepening our view of the world.

Relativity has revealed two important new aspects of energy. First, there exists a new kind of energy, the energy of mass. Second, energy is linked to momentum in the same way that time is linked to space. Just as space and time become mixed in relating the measurements of two different observers, so do momentum and energy become inextricably mixed, and the laws of conservation of momentum and of energy combine into a single more general conservation law. All this because the ether was rejected. How beautiful and how unexpected are the consequences of Einstein s two simple postulates.


1 The squared interval is sometimes written (ct)2 – x2 + y2 + z2, in which the time between a pair of events is emphasized rather than the distance between them.

2 How can the square of a real number be negative? It can’t. It is actually only the squared quantity, positive or negative, that enters into the equations of special relativity. It is called an interval-squared because it has the dimension of length-squared.


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