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SCIENCE · INVESTIGATE AND EXPLAIN

Separate deposited energy from neutrino escape

Close the energy ledger and distinguish required rates from achieved fusion.

Learning outcome: Calculate a conditional completion rate from deposited energy and photon demand.

Starting recap

Total energy includes escaping neutrinos; deposited energy is total minus that channel.

All lessons are open directly. Your saved experiments remain when you leave and return.

Try

26.731 minus 0.530 gives approximately 26.201 MeV deposited.

Open the experiment

Predict

What changes when photon demand doubles while inventory stays fixed?

Experiment

Capture one and two nominal solar luminosities, then test zero available fuel with the same positive demand.

Trace fusion energy into a conditional fuel budget

Worked teaching model · synthetic values · Synthetic total mass 2.0×10³⁰ kg; the chosen accessible region has fixed hydrogen-1 mass fraction 0.70. Neutral-atom mass differences include electron bookkeeping. A restricted pp-I mean assigns 0.530 MeV per completion to escaping neutrinos. Remaining energy is assumed to support the specified average photon demand. Rates are required, not achieved; zero fuel supports zero duration. No actual stellar lifetime, reaction-rate, structure, mixing or evolution prediction is made.

Reset keeps your prediction, captures and practice history.

Build helium from hydrogen, then ask how much energy a specified fuel inventory could supply. The two controls change the hypothetical inventory and average photon demand; they do not change nuclear masses or calculate an actual stellar reaction rate.

pp-I worked mechanism · p = proton; n = neutron; e⁺ = positron; νe = neutrinoTwice: p + p → ²H (1p + 1n) + e⁺ + νeTwo weak conversions produce two neutrons and two escaping neutrinos.Twice: ²H + p → ³He (2p + 1n) + γγ denotes a gamma photon. Both intermediate helium-3 nuclei are used next.Once: ³He + ³He → ⁴He (2p + 2n) + p + pSix protons entered the preceding stages; two return. Net consumption: four.Also twice: e⁺ + e⁻ → photons. Surrounding electrons supply the e⁻.Cancel intermediates on paper. This chain is not one four-proton collision.Reaction count does not determine a rate; temperature and density are not modeled.

For the energy ledger, use four neutral hydrogen-1 atoms and one neutral helium-4 atom. This is consistent rest-mass bookkeeping for the net process, not neutral atoms inside the hot core. Four initial electrons account for two in the final atom and two annihilating with positrons. Do not add annihilation rest energy again. Plasma ionization and tiny neutrino rest-mass corrections are omitted.

Rest masses · common scale 0–4.1 u4 neutral H-11 neutral He-40 u4.1 uDifference 0.02869687 u ≈ 0.712% of initial fuel rest mass.Released energy · separate scale 0–27 MeV0 MeV27 MeVDeposited: 26.201 MeV; neutrinos: 0.530 MeV mean.Total: 26.731 MeV. Mass-energy is conserved.

The gold energy segment is the stipulated mean carried away by two pp neutrinos, not a fixed energy for each event or a universal average over all fusion branches. Deposited energy can thermalize before escaping as photons. Nearly all initial fuel rest mass remains in helium.

Hypothetical available inventory and required demand rates
QuantitySelected demandSame inventory, 1 nominal solar luminosity
Accessible region kg2.00000e+292.00000e+29
Hydrogen inventory kg1.40000e+291.40000e+29
Possible net completions2.09138e+552.09138e+55
Helium product rest mass kg1.39003e+291.39003e+29
Total released budget J8.95692e+438.95692e+43
Neutrino budget J1.77591e+421.77591e+42
Deposited budget J8.77933e+438.77933e+43
Prescribed photon demand W3.82800e+263.82800e+26
Required completions per second9.11894e+379.11894e+37
Required hydrogen processing kg/s6.10434e+116.10434e+11
Required rest-mass conversion kg/s4.34538e+94.34538e+9
Implied neutrino power at required rate W7.74338e+247.74338e+24
Conditional support duration Gyr7.267517.26751
Compare independent reservoirs · NOT a stellar time historyConditional support duration (Gyr) · solid/circle selected; dashed/square reference030609012015005101520Available core region (% of synthetic total mass)Hydrogen fraction fixed at 0.70. Long budget ≠ a physically predicted stellar lifetime.

Selected support budget: 7.26751 Gyr; same inventory at the reference demand: 7.26751 Gyr. The two curves coincide because their demands are equal. Each curve compares separate inventories; it does not show a core expanding over time.

Connect fuel, mass difference and power

Let q be the selected region percentage divided by 100. Available hydrogen mass is Mfuel = 0.70 × q × 2.0 × 10³⁰ kg. Count possible net completions as N = Mfuel / (4mH u), with mH = 1.00782503223 and u = 1.66053906892 × 10⁻²⁷ kg. The selected isotope mass differs from a natural-isotope average.

Mass defect per completion is Δm = (4mH − mHe)u, with mHe = 4.00260325413. Released energy is Qtotal = Δm c²; c = 299792458 m/s. Subtract the stipulated mean neutrino energy once: Qdeposit = Qtotal − Qν. One MeV = 1.602176634 × 10⁻¹³ J. Total deposited budget is N Qdeposit.

Divide that energy budget by prescribed average photon luminosity Lγ to obtain a duration in seconds. Divide by 31557600 and one billion to express Gyr. A required completion rate Lγ/Qdeposit is distinct from the amount of fuel. At 10% region and one nominal solar luminosity, 1.40 × 10²⁹ kg of hydrogen supplies about 8.77933 × 10⁴³ J deposited energy, a conditional 7.26751 Gyr budget.

This assumes all deposited energy supports the average photon demand, with no net storage change, mechanical loss or alternate source. Actual stellar temperature, density, mixing, luminosity history and other branches are absent. No present age, remaining lifetime or feasible reaction rate follows from this ratio.

Sources: isotope-specific masses from NIST hydrogen and helium; CODATA conversion constants; Berkeley pp-chain explanation; Fukugita and Peebles on neutrino energy; IAU nominal luminosity. Values use central reference constants without uncertainty propagation; displayed precision is not a new measurement.

Available hydrogen 1.4000e+29 kg; deposited budget 8.7793e+43 J; conditional support duration 7.2675 Gyr.

The prescribed photon demand would require 9.1189e+37 pp-I completions/s and 6.1043e+11 kg/s of hydrogen processing. These are demand-derived required rates, not actual output. The energy/power ratio is not a stellar lifetime prediction.

Captures preserve hypothetical fuel-region and photon-demand choices. Replaying calculates conditional energy budgets and required rates, not measured fusion output or actual stellar lifetimes.

Understand

Follow energy after the reaction

A completed pp-I construction releases approximately 26.73 MeV, but the lab does not assign all of it to the star’s photon output. Neutrinos carry some energy away. Other released energy, initially carried by energetic particles and photons, is deposited and thermalized. This is not an immediate flash of identical visible photons from one reaction.

Draw a box for total released energy with two exit arrows. Label one escaping neutrinos and the other deposited energy. Before reading the numbers, predict whether subtracting the neutrino channel should alter the atomic mass defect or only the energy available to support the prescribed photon luminosity.

Close the per-completion ledger

The model assumes two pp neutrinos with mean energy 0.265 MeV each. Thus the mean escaping energy Qν is 0.530 MeV per completed construction. The NASA/IPAC-hosted discussion of stellar neutrino losses supplies this approximate pp-neutrino mean and distinguishes other contributions.

Define Qtotal as total released energy and Qdeposit as deposited energy. Then Qtotal = Qdeposit + Qν. Subtraction gives Qdeposit approximately 26.201 MeV. Divide deposited by total energy to find about 98.017 percent deposited. The remaining approximately 1.983 percent escapes in the stipulated neutrino channel.

This percentage has a different denominator from the roughly 0.712 percent of initial fuel rest mass converted into released energy. Write both fractions as words before comparing them. A small fraction of fuel rest mass is converted, and most of that released energy is deposited. Those statements are compatible.

The fixed neutrino value is an ensemble mean, not the energy of every individual neutrino. Nor is it a universal solar-fusion mean: pep reactions, pp-II and pp-III branches and the CNO cycle are absent. We do not measure a neutrino spectrum or determine branch proportions in this lab.

Convert an energy per event into a required rate

Photon luminosity is power, measured in joules per second. If deposited energy ultimately supplies the stated average photon output, divide desired photon power Lγ by deposited energy per completion: required rate = Lγ/Qdeposit. Units provide a useful check: J/s divided by J/completion gives completions/s.

At one nominal solar luminosity, 3.828 × 10²⁶ W, the required rate is about 9.119 × 10³⁷ completions each second. The IAU nominal-constant resolution defines that luminosity unit; using it does not turn this synthetic budget into a measured solar model.

Compare one and two nominal solar luminosities at the same 10 percent reservoir. Predict that required completion rate and required neutrino power both double. Possible total completions do not double, because the fuel inventory is unchanged. Capture both settings and explain why the support duration halves.

Keep demand separate from achieved output

At the one-unit demand, the hypothetical required neutrino power is about 7.743 × 10²⁴ W. Multiplying the required completion rate by Qtotal gives photon demand plus this neutrino power. This is a conditional energy ledger. It does not prove a core can achieve the required reaction rate.

Set available core region to zero without changing luminosity. The positive selected power remains a proposed demand; the fuel inventory, available energy and support duration become zero. A displayed required rate is still the rate needed to meet the demand, not a reaction actually occurring. Record this boundary case in your notebook with a sentence explaining the distinction.

Required hydrogen processing is about 6.104 × 10¹¹ kg/s at the one-unit demand, while required rest-mass conversion is about 4.345 × 10⁹ kg/s. Almost all processed mass remains in helium. Neither number is a measured mass-loss wind or a rate computed from temperature and density.

Transfer: an incomplete mass-energy estimate

An analyst calculates photon luminosity divided by c² and labels it the full rest-mass conversion rate. The analyst knows neutrinos escape but says they were already subtracted from deposited energy, so they should be ignored. Repair the argument without subtracting neutrinos twice.

Check the fusion-channels transfer

Photon demand determines the required rate using Qdeposit. At that rate, total released power is photon power plus required escaping-neutrino power. Divide that sum by c² for total rest-mass conversion. Neutrino energy is already part of Qtotal; subtracting it determines deposition, but does not erase it from total energy conservation.

Apply

At zero available fuel and positive selected photon demand, the displayed required rate is:

Public practice checks a specific claim. It does not establish independent mastery.

Explain why required rate is not proof of an achieved rate.

Continue

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