• 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

R2. Transformations: Galilean And Lorentz

Based on Basic Physics Features 30 and 108

The principle that the laws of mechanics are the same in all inertial frames of reference is called the principle of Galilean relativity. It is really a principle of invariance, a statement that the laws governing motion are the same in different inertial frames of reference, even though the description of a particular example of motion might be different in the different reference frames (see Essay R1). The significance of Galilean relativity can perhaps best be emphasized by stating the principle in this way: If a particular example of motion is possible (that is, consistent with the laws of motion) in one inertial frame of reference, it is also possible in every other inertial frame of reference. This way of looking at Galilean relativity can be illustrated with the help of the figure below: The motion of the ball as observed by player B is straight-line vertical motion. Although this is not the motion observed by player A, it is a possible motion that player A could produce in his own frame of reference if he wished to—simply by throwing the ball straight up. Similarly, the parabolic motion observed by player A is a motion that could be observed in player B’s moving frame of reference if the ball were thrown differently. The class of all possible motions for observer A is precisely the same as the class of all possible motions for observer B. Therefore they agree about the laws of motion.

An important consequence of the principle of Galilean relativity is that it is impossible to discover the existence of a truly stationary frame of reference, a frame at rest with respect to a hypothetical ether filling all of space. Since all physical phenomena (at least mechanical phenomena) follow the same laws in a frame moving uniformly with respect to this supposed ether as in a frame at rest with respect to the ether, there is no mechanical experiment that can distinguish the two. Galileo himself used the principle to support the Copernican view of the solar system. He argued that the laws of motion would be no different on a moving earth than on a stationary earth, so that one might as well adopt the simpler Copernican view of a moving earth in place of the far more complicated Ptolemaic view of a solar system built around a stationary earth. Before Galileo, almost all scientists and philosophers from Ptolemy onward had argued that the straight vertical fall of a dropped stone demonstrated that the earth must be at rest. According to Galileo’s principle of relativity, it proved no such thing.

As illustrated in the figure above, two observers in relative motion disagree about the velocity of a ball whose motion they are watching. This disagreement does not prevent them from agreeing about the laws of motion because the law a = F/m does not contain velocity explicitly. It contains instead acceleration, about which the two observers agree. In the theory of electromagnetism, however, the fundamental equations do contain velocity. The magnetic field generated by a moving charge depends on the charge’s velocity. So does the magnetic force on a moving charge. And the basic equations of electromagnetism contain constants related to the speed of light. All of these velocities would be changed by a Galilean transformation. This is one reason why the laws of electromagnetism do not demonstrate Galilean invariance. They seem to call for a preferred frame of reference.

This difference between the theory of mechanics and the theory of electromagnetism can be viewed in several alternative ways.

1. The Principle of Relativity happens to be satisfied by mechanics but it is not a general principle of nature and is not very important.

2. The theory of electromagnetism is incorrect and must be changed to conform to the Principle of Relativity.

3. The Principle of Relativity is correct, but the Galilean transformation and therefore Newtonian mechanics must be discarded and a new transformation found that will permit the laws of electromagnetism to be invariant.

Einstein adopted the third bold view, which led to the theory of relativity, with its enormously successful consequences, including a new mechanics, a new view of the world, and incidentally even a deeper new insight into electromagnetism. Although the equations of electromagnetism weathered the revolution of relativity unchanged, the interpretation of these equations was somewhat altered.

Einstein’s transformation law relating the space and time measurements of different observers (all in inertial frames!) is called the Lorentz transformation. Hendrik Lorentz had shown in 1904 (a year before Einsteins “miraculous year”) that this transformation law would preserve the invariance of the theory of electromagnetism and account for the shyness of the ether. Over the course of the next five years, as scientists reluctantly but finally discarded the ether altogether, the more general validity of the Lorentz transformation and some of its startling consequences came to be realized.

The Lorentz transformation plays a vital role in the theory of relativity because it is the essential quantitative link between the measurements of different observers. Without it, science would be reduced to a chaos of subjectivity: One observer measures one thing, another measures something different, and no two observers could get together and agree about what is really happening. The Lorentz transformation is a world court of arbitration, reconciling to everyones satisfaction the divergent parochial viewpoints of scientists who insist on referring their measurements to frames of reference that are in states of relative motion. Because it accounts quantitatively for the relativity of observation, it makes possible the invariant objective agreement among different observers. Actually, human observers do not move fast enough to reveal the special features of the Lorentz transformation. However, the scientist can cast herself mathematically into a high-speed frame of reference and can describe physical processes in that frame without climbing aboard it herself.


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