Mass–Energy · System boundaries & empirical checks
System boundaries and the energy ledger.
When energy leaves a body as radiation, which system loses mass, and which does not? Drag a thermodynamic boundary around the components and inspect what energy crosses it.
System boundary energy ledger
System-boundary energy ledger with cited energy-source cards
Static worked example
CurrentThese numbers match the current settings.
Model note
- Primary outputs energyChange, massChange, radiationEnergyChange, radiationMassChange, systemEnergyChange, systemMassChange: Host calculation (massEnergy.boundaryLedger). Owner massEnergy.boundaryLedger.
- Primary output invariantMass: Host calculation (massEnergy.fourMomentum). Owner massEnergy.fourMomentum.
- Accepted input revision 1.
- Snapshot version 1.
- Not modeled: gravitational weighing; wall stresses, or external work beyond declared inputs; nuclear and chemical mechanisms beyond cited energies; heat losses not declared; neutrino and solar-wind mass loss; the practical measurability of tiny mass changes; the 1905 argument's premises (inherited, not re-derived); non-inertial or accelerated frames.
Predict before the numbers
A sealed box holds a battery-powered lamp and a mirror. When the lamp lights up inside, does the box's total mass change?
The result appears when you choose, say you have one in mind, or skip.
Experiment settings seven cited energy sources, notation
Worked example: Radium-226 alpha decay, with the boundary around the body alone: the radiation escapes, and the energy figure is 4.871 MeV.
Where the boundary is drawn
Inside the boundary: the body alone. The radiation escapes.
Energy and mass inside the boundary
- Inside the boundary
- The body alone
- Energy change ΔE
- −1 J
- Mass change Δm
- −1.1127 × 10−17 kg
- Case study
- Radium-226 alpha decay
- Mass change
- 0.0052292 u/decay (5.229 mg/mol)
Case study facts: Radium-226 alpha decay
Citation: NuDat 3.0 / Evaluated Nuclear Structure Data File (ENSDF), Brookhaven National Laboratory (226Ra Q-alpha = 4.871 MeV).
- 1. System before:
- Radium-226 nucleus at rest
- 2. System after:
- Radon-222 nucleus and alpha particle after heat emission
- 3. Matter crosses boundary:
- No (Closed system: The radon-222 nucleus and the alpha particle both stay inside the boundary.)
- 4. Radiation disposition:
- escapes (The decay energy leaves as heat.)
- 5. Reference frame:
- Rest frame of parent nucleus
- 6. Energy figure:
- 4.871 MeV (energy released per decay)
Show the reference code & kernel bindings
Reference evaluator: src/physics/reference/massEnergy.ts
// evaluateBoundaryLedger
const bodyDeltaM = -emittedEnergy / (c * c);
const sysDeltaM = disposition === "retained" ? inputEnergy / (c * c) : 0;
// evaluateFourMomentum
const mSquared = (totalEnergy / c)^2 - p^2;
const invariantMass = Math.sqrt(Math.max(0, mSquared));Energy that leaves a body takes mass with it. Draw the boundary around the body alone and it gets lighter; draw it around the body and the light it gave off, and nothing is lost.
The mass–energy paper concludes that a body giving off energy L loses mass L/V², that it does not matter that the energy leaves as radiation, and that, if the theory is right, radiation carries inertia from the body that emits it to the body that absorbs it. The instrument keeps the accounting honest by making you choose where the boundary goes. With 1 J emitted and the boundary around the body alone, the body's energy falls by 1 J and its mass by 1.11 × 10−17 kg. Around the radiation alone, 1 J arrives, and the lab gives it no rest mass in the 1905 account, saying so rather than inventing one. Around the body and its light together, an isolated system, nothing changes. In the four-momentum lens, a modern addition, two opposite pulses of total energy 1 J have an invariant mass of 1.11 × 10−17 kg, which is where the body's lost mass went. The energy-source cards apply ΔE/c² to cited modern transfers: a radium-226 alpha decay of 4.871 MeV changes mass by 8.68 × 10−30 kg; the Sun's 3.828 × 1026 W takes away 4.26 × 109 kg each second; a kilogram of coal burned at 30 MJ, 3.34 × 10−10 kg; a candle for an hour, 3.20 × 10−12 kg; a 100 W bulb for a year, 3.51 × 10−8 kg. In the 1906 photon-in-a-box mode (credit: Poincaré 1900), a pulse crossing a floating box shows that the centre of mass stays put only if the light is given the mass E/c².
The rule is Δm = ΔE/c², with c² = (2.998 × 108)² = 8.988 × 1016 m²/s², so 1 J corresponds to 1/(8.988 × 1016) = 1.11 × 10−17 kg. The sign follows the boundary. A body that emits 1 J has 1 J less inside its boundary, so its mass falls by 1.11 × 10−17 kg. Move the boundary around the body and its light, and the energy inside does not change, so neither does the mass: the joule left the body but not the system. Now the cards. The radium decay releases 4.871 × 106 × 1.602 × 10−19 = 7.80 × 10−13 J, which divided by c² is 8.68 × 10−30 kg, about 2 parts in 100 000 of the radium atom's mass. The Sun radiates 3.828 × 1026 J each second, and dividing by c² gives 4.26 × 109 kg, some four million tonnes a second. The bulb uses 100 W × 31 557 600 s = 3.156 × 109 J in a year, which is 3.51 × 10−8 kg, about 35 micrograms. Now the 1906 box argument. A box of mass 1 kg and length 1 m floats free. A pulse of 1 J leaves one end carrying momentum E/c = 1/(2.998 × 108) = 3.34 × 10−9 kg·m/s, so the box recoils the other way at 3.34 × 10−9 m/s. The pulse takes l/c = 3.34 × 10−9 s to cross, and in that time the box moves back 3.34 × 10−9 × 3.34 × 10−9 = 1.11 × 10−17 m, which is El/(Mc²). When the pulse is absorbed at the far end, the box stops. Nothing outside acted on the box, so the centre of mass of the whole system cannot have moved. The box's backward step is balanced only if the pulse carried a mass m across the length l with ml = M × 1.11 × 10−17 m, so m = 1.11 × 10−17 kg = E/c². Switch that assignment off and the lab shows the centre of mass moving by 1.11 × 10−17 m, which an isolated system cannot do.
The 1905 conclusions are conditional. The paper says it is not excluded that bodies whose energy content varies greatly, radium salts for instance, could test the theory, and that if the theory corresponds to the facts, radiation carries inertia between the emitting and absorbing bodies. It gives no rest mass to free radiation; the invariant mass of a system of light belongs to the later four-momentum language. The box is Einstein's 1906 argument (credit: Poincaré 1900): his paper credits Poincaré's remark of 1900 that electromagnetic energy behaves like a fluid with inertia. The energy-source values are modern and cited on each card; none was measured in 1905, and the mass changes of chemical and everyday transfers are far too small to weigh.
The physics of the boundary
Three thermodynamic boundaries
Einstein concludes that if a body gives off the energy L in the form of radiation, its mass diminishes by L/V² (or in modern notation L/c²):
The total energy of an isolated system is strictly conserved. If the boundary is drawn around the emitting body and the radiation together inside a sealed container, no energy escapes, and the total mass of the enclosure remains completely unchanged:
Closed systems versus isolated systems
A system is closed if no matter crosses its boundary. It is isolated only if neither matter nor energy crosses its boundary. A radioactive radium salt sealed in an ampoule exchanges heat with its surroundings without losing matter; its mass decreases only as that heat leaves the container.
Modern four-momentum invariant mass
In modern relativistic mechanics, the invariant mass m of any system of particles or photons is the Lorentz norm of its total four-momentum P^μ = (E/c, p):
While a single light pulse has |p| = E/c and is therefore massless (m = 0), two equal and opposite light pulses have total momentum p = 0 and carry a nonzero system invariant mass:
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