• 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

G14. Superposition

Based on Basic Physics Features 58, 91, and 103

Simply stated, the principle of superposition is this: The result of several actions taken together is equal to the sum of the results of the actions taken separately. Here are some examples where it is a (mostly) valid principle:

A. Force F1 applied to a certain object produces acceleration a1 and force F2 applied to the same object produces acceleration a2. When force F = F1 + F2 is applied to the object, the resulting acceleration is a = a1 + a2 (these are vector sums).

B. Two objects have weights W1 and W2. When they are placed on a scale together, the recorded weight is W1 + W2. (This implies the additivity of mass—valid up to a point!)

C. At a certain location, the electric field arising from a collection of charges is the vector sum of the fields that would be produced at that location by the charges acting separately. The same principle holds for magnetic fields.

Example A may seem “obviously” true. Example B may seem so, too (since it is consistent with ordinary experience), but in fact, the masses of two objects are not strictly additive when the objects exert forces on one another—forces that can change the energy and therefore the mass of the pair of objects. Masses are additive in classical Newtonian theory, but not in relativity theory. The truth of Example C at first seems more doubtful because fields occupy space. Can they coexist in space without “bothering” one another? In classical electromagnetic theory (the theory of James Clerk Maxwell), the answer is yes. Fields of arbitrary strength can share space without mutual “disturbance.” In quantum theory, not quite. So both relativity theory and quantum theory slightly “besmirch” the superposition principle.

Consider some examples where the superposition principle is not true.

D. You pour a pint of water into a quart jar. The jar is half full. You separately pour a pint of alcohol into another quart jar. That jar, too, is half full. Now you pour a pint of water and a pint of alcohol together into a quart jar. The jar doesn’t quite fill up. One pint + one pint in this case is not equal to one quart.

E. You and a friend both earn $50,000 per year and pay the same tax. Another friend earns $100,000 per year. Her tax is more than twice yours.

F. Put a neutron on an imaginary super-sensitive scale and measure its mass to be mn. On that same scale put a proton and measure its mass to be mp. Now combine the neutron and proton to form a deuteron, and measure its mass. The deuteron’s mass md is not mp + mn. It is less.

So, even in physics, the superposition principle is not universally valid. Yet it does have widespread validity and is appealing for its utter simplicity: Effect (A + B) = Effect A + Effect B. It supports our view that nature usually chooses the simplest rules (or is kind enough to let us mere humans figure out the rules).

Since electric and magnetic fields can be superposed, it follows that electromagnetic waves can be superposed. Think of light from two stars intersecting somewhere in the depths of space. Each beam continues inexorably on its way, undeflected and unchanged by having interpenetrated the other. Of vital practical importance on Earth is the superposition of radio waves, without which radio communication would be impossible. Think of the electromagnetic disturbances in the space around you. If they were visible you would see a gaudy and ever changing splash of every conceivable color. If they were audible you would hear a cacophony of sound. Yet every component of this turmoil, with its own frequency, polarization, and direction of propagation, retains its unique identity, undisturbed by sharing the same space with thousands of other signals.

In the seventeenth century, long before the full import of superposition was appreciated for electromagnetic waves, Christian Huygens made use of the idea of superposition in describing the propagation of a single wave. He asserted that each point on an advancing wave front could be regarded as the source of a new wavelet, and that the subsequent position of the wave front was determined by the superposition of all of the tiny wavelets. This application of the idea of superposition, summing individual contributions from an advancing wave to get the total wave, is known now as Huygens’ principle. In a modernized form that takes proper account of the phase of the wavelets, it provides a very useful approach for understanding many wave phenomena, including interference and diffraction.

For water waves and other waves in material media, the principle of superposition is usually valid to good approximation, but it is never precisely valid. Looking at the surface of a pond on a perfectly still day, for instance, you can see that waves emanating from two dropped pebbles proceed on their way, crossing one another and hardly losing their individuality. The condition required for superposition of material waves is that the wave disturbance be relatively weak—gentle waves on water, for example, but not breaking waves at the beach; or mild sound waves, but not shock waves. If two shock waves cross one another, the resulting wave at their point of intersection is not the sum of the two separate waves, and they do not continue on their way uninfluenced by the encounter.

The development of the quantum theory of radiation in the 1930s revealed that not even for electromagnetic waves is the principle of superposition precisely valid. If two photons meet in space there is a chance—an exceedingly small chance—that they will interact and be deflected by the encounter. This violates the principle of superposition, for the resulting radiation flow is not the same as for the two photons passing separately by. This process, known as the scattering of light by light, has been measured in the laboratory, but it is too improbable to have any perceptible effect on radio communications or on any of the other practical examples of superposed electromagnetic waves or photons.1 It is interesting, however, to know that if photons are crowded together densely enough, they can begin to act like bits of matter.


1 The scattering of light by light was first studied theoretically by Gregory Breit and John Wheeler in 1934, and finally observed in the laboratory in 1997, after laser beams of sufficient intensity were available.


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