• 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

M6. Inertial Mass

Based on Basic Physics Feature 26

It is easy to study the properties of uniformly accelerated motion in the laboratory using the familiar “air track,” on which a car rides with very little friction. A student places weights of various size on a car. With the track arranged to be horizontal, she pulls or pushes the car with a known constant force, and measures the acceleration. The first result of such an experiment is that a constant force produces constant acceleration. The second result is that for the car loaded in a particular way, its acceleration is proportional to the force applied. These results are summarized by the proportionality

F ~ a.

This proportionality can be converted to an equality by introducing a constant of proportionality. For the car loaded in a particular way, the force may be written as a constant times the acceleration (now in vector form):

F = ma.

This is Newton’s second law.1 Here I want to discuss just its role in defining mass.

The constant of proportionality in this equation, m, is called the inertial mass, or often simply the mass, of the object under study, in this case the car plus its load. Before discussing the physical meaning of mass, let me note some facts about it revealed by its appearance in this equation. Its dimension must be the dimension of force divided by the dimension of acceleration, or force × (time)2/length. In standard units, the unit of mass, the kilogram, is equal to one newton (second)2/meter. With standard abbreviations, this equality may be written,

1 kg = 1 N s2/m.

Which of the two concepts, force and mass, is taken to be fundamental and which derived is arbitrary. So the connection above may also be written

1 N = 1 kg m/s2.

Notice also from the equation F = ma that mass appears to be a numerical quantity (or scalar quantity), not a vector quantity. The only thing that can multiply a vector (a) to give another vector in the same direction (F) is a number. However, the numerical or scalar character of mass requires experimental verification.

Experiments performed with cars loaded differently reveal different masses. Not surprisingly, the rule is: The greater the load, the greater the mass. From the definition of mass, it follows that a particular force gives more acceleration to a small mass than to a large mass. The greater is the load carried by a car, the more sluggishly it responds to a given force, and the less velocity it acquires in a given time. In short, it has more “inertia.” And inertia inhibits any change in velocity—to greater speed, less speed, or a change of direction. Mass, to put it generally, is a measure of an object’s resistance to a change in its state of motion.

Among charged particles, the least massive electron is the easiest to accelerate to high speed and the easiest to deflect into a curved path. It responds most readily to the pushes and pulls of electric and magnetic forces. Some particles—the photon and the graviton—are actually massless. If Newton’s second law remained valid in the particle world, these particles could achieve infinite acceleration and infinite velocity. They would have absolutely no resistance to a change in their state of motion. In fact, because of the existence of a speed limit in nature, they reach only the speed of light rather than infinite speed. However, they can be said to experience infinite acceleration. A photon spends no time reaching the speed of light, but starts immediately with that speed at the moment of its birth.

Returning to the loaded car on the track whose mass is defined as the ratio of the horizontal component of force acting on it to its horizontal component of acceleration, one must inquire about the self-consistency of the definition. If mass is truly a scalar quantity, the mass of two objects (or “loads”) is the sum of the masses of the individual loads. Numerous laboratory experiments confirm that this is true, leading to the conclusion that mass is indeed a scalar quantity. But as always in science, one must be cautious. It turns out that in the submicroscopic realm where relativity and quantum mechanics hold sway—in domains far removed from ordinary lab experience—masses do not necessarily add as scalar quantities. For example, the mass of a deuteron, composed of a proton and a neutron, is less than the sum of the masses of a proton and a neutron. The so-called “binding energy” holding the neutron and proton together plays a role. In keeping with E = mc2, the negative binding energy subtracts some mass from the total.

One more subtlety. Although, in modern physics, mass is not strictly a scalar quantity (in that the mass of a combination of two objects need not be the sum of the masses of the individual objects), it is still a numerical quantity. It is measured by a single number, has no direction, and, in the equations of physics, behaves as a number.

A solid law of chemistry—and indeed of physics, too, before the twentieth century, is the law of mass conservation. Mixing and matching atoms and molecules does not change their total mass—a law concordant with the scalar nature of mass. Where mass does not behave as a scalar (in modern particle physics), mass is not conserved. Mass conservation was a vital tool supporting advances in chemistry in the nineteenth century, and fortunately remains valid to a high degree in chemistry laboratories in the twenty-first century—and no doubt beyond. Not so in the physicist’s world of fundamental particles, where mass conservation is not even close to being valid.


1 Newton’s own version of his second law, although equivalent in content to this equation, was phrased differently.


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