• 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

G1. Faith In Simplicity As A Driver Of Science

Based on Basic Physics Features 1 and 63

The commonly known and accepted miracle of science is the enormous power it has given to humankind to change the world we inhabit. There is another miracle of science, less often appreciated. It is the miracle of the simplicity, generality, and beauty of fundamental physical theories. The straitjacket of experimental confirmation, far from enclosing the imagination of the scientist in a stuffy, cheerless room, has spurred on the scientist’s imagination. The successful theories of physical science that have been created possess a simplicity and inner harmony as satisfying to the human mind as any creation of the free and unfettered imagination. Expressed differently, we should be grateful to nature for revealing its secrets to us in such a rewarding way.

Scientists like to say that nature is simple. What they mean is that it has been found possible to describe parts of nature—the parts we understand—in a simple way. Without the underlying faith in simplicity and the rewards of success, scientists would lack the stamina to overcome the obstacles to understanding that line the route to the discovery of simplicity. As every student of science is well aware, the simplicity of nature is not synonymous with ease of comprehension. The theory of general relativity, viewed as a formal structure, is exceedingly simple. But to understand it and to use it requires a heroic effort of the mind, for the concepts employed, and the ways of thinking required, are largely foreign to our everyday experience. Simplicity to the scientist means economy and compactness—of assumptions, of fundamental concepts, of mathematical equations. The fewer the basic elements of a theory and the greater the range of phenomena described by the theory, the simpler do we declare nature to be.

Throughout human history, the faith in simplicity has been a primary motivating force in science. In essence it is the faith in the possibility of science at all, that nature, or parts of nature, follow an orderly and predictable pattern governed by fixed laws. It is more than just a faith that nature follows laws that can be expressed mathematically; it adds a conviction that these laws are sufficiently simple that scientists dare hope to find and comprehend them. So powerful was the faith in simplicity among some Greek philosophers that simplicity itself came to be regarded as a sufficient test of the truth of a theory. Aristotle accepted circular motion as the rule in the heavens not because careful measurements showed the stars and planets to move in circles, but because the circle is the simplest (or most “harmonious,” or most “perfect”) of plane figures. In describing motion on Earth, he advanced a theory of utmost economy. It required but four elements—earth, water, air, and fire (which today we can interpret as solid, liquid, gas, and energy)—and but two kinds of natural motion, vertically up and vertically down. Surely the simplicity of Aristotelian physics must have contributed to its durability.

The birth of modern science in the sixteenth and seventeenth centuries brought with it no change in the ancient faith in the simplicity of nature. Rather a new element was added: the reliance on accurate observations (usually in carefully controlled experiments) to test the acceptability of a theory. The pyramiding successes of science in the past few centuries have richly rewarded the scientist’s faith in simplicity coupled with insistence on experimental confirmation.

Because the simplicity of basic science is so little appreciated, it is proper to emphasize it, even to extol it. At the same time, we must keep in mind that, at least in part, science is fundamentally simple because we humans have made it so. From science we get simple answers because we ask easy questions. But what exactly is an easy question? Compare these two, the first scientific, the second nonscientific:

1. What is the transition probability for radiation from the n=2 level in the hydrogen atom that gives rise to the Lyman Alpha line?

2. What are the advantages of foreign travel?

The average reader without scientific training will regard the first question as incomprehensible and therefore obviously difficult. But anyone should be willing to venture an answer to the second, which appears easy enough. Upon a little reflection, of course, you should convince yourself that it is after all the first question that is easy, the second that is difficult. Assuming the first question is meaningful (it is) and that science has progressed to the point that an answer exists (it does), then the answer is just a simple number upon which the thousands who can give an answer amicably agree, and which the millions of others as amicably accept. The second question, on the other hand, deals with what is good for humankind, and there are no harder questions that we have posed to ourselves than questions of good and evil.

Too often we think that science began in the seventeenth century after millennia in which superstition and blind faith reigned. The evolution of human thinking about the system of the world clearly shows otherwise. The faith in simplicity, the assumption that mathematics describes nature—these essential attributes of modern science were equally parts of ancient science.

For the development and growth of science, criteria for rejection of an idea may be even more important than criteria for acceptance. Ptolemy rejected and revised Aristotle’s picture of the world in order to get rid of the excessive number of intermediate spheres. The accumulated complexity of the later Ptolemaic picture led Copernicus to reject it in favor of a simpler Sun-centered model. Kepler found the Copernican universe still excessively complex (as well as insufficiently accurate) and rejected it even before he had discovered the true laws of planetary motion. The necessary precondition for his great step forward was dissatisfaction with existing explanations. The groundwork for modern science was laid by scientists who sought simplicity and believed in the mathematical basis of natural phenomena.


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