Annus Mirabilis · Interactive critical edition in preparation

The system-boundary energy ledger

Choose where the boundary goes, and see which system loses mass when a body emits light.

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?

Three relations the model could have

The result appears when you choose, say you have one in mind, or skip.

Compare
Inside the boundary
The radiation
Try
Experiment settings seven cited energy sources, notation
A cited energy source
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.

isolated systembodyΔm = −L/V²radiation, L

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)
7. Closed but not isolated: Nothing material crosses this boundary, but the system is not isolated: energy still enters or leaves it.
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));

Not modeled in this ideal reference calculation:

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

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 explanation

Full explanation

Around the emitting body alone, the energy falls and the mass falls by the energy divided by c². Around the body and its light together, an isolated system, nothing changes. The energy-source cards apply the same rule to cited modern energy transfers, and the four-momentum view is labelled as a later addition.

Show every step of the investigation

Put the boundary around the body, then around the radiation, then around both, and read what crosses it each time. Open an energy-source card and compare its mass change with the body's. The 1906 photon-in-a-box mode is a later argument, shown with its credit to Poincaré (1900).

An explanatory model, not an observation of nature. This embed starts from the laboratory’s worked defaults, not a saved run. Presentation options change the surrounding guide, never the numerical inputs.