2.3.24 · D1Modern Physics

Foundations — Fusion — solar fusion, tokamak (concept)

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This page assumes you have seen none of the notation on the parent note. We build each symbol from the picture up, in an order where every symbol only uses symbols already earned.


1. The nucleus, the proton, the neutron

Figure — Fusion — solar fusion, tokamak (concept)

The picture: look at figure s01. A nucleus is a little cluster of red balls (protons) and grey balls (neutrons) packed together. The electrons live far outside — we ignore them here because fusion is about the nucleus.

Why the topic needs this: fusion means combining nuclei. You cannot talk about combining things you haven't named.


2. Nuclide notation

The parent note writes things like and . Let us fully unpack that stack of numbers.

Why the topic needs this: the whole reaction is bookkeeping with these labels. Notice the totals balance: protons before , after ; balls before , after . Nothing is lost in count — but as we'll see, a sliver of mass is.


3. Why nuclei push apart — the Coulomb barrier

Figure — Fusion — solar fusion, tokamak (concept)

The picture: figure s02 shows the energy "hill" two protons must climb as they approach (the red curve). Far apart, the push is gentle. Very close, a different, much stronger attraction (the strong force) suddenly takes over and yanks them together — that's the deep valley on the right.

Why the topic needs this: every "insane temperature" and "compress it" statement on the parent page exists purely to defeat this hill.


4. Temperature = how fast the particles jiggle

The picture: imagine the red balls of figure s01 vibrating. Cold → gentle jiggle, they never reach the hilltop of s02. Hot → violent jiggle, some pairs ram right over the barrier.

Why the topic needs this: "heat to K" literally means "make them jiggle hard enough to climb the Coulomb hill." appears again inside the Lawson criterion.


5. Mass, the mass defect , and

Now the heart of the energy release. First, mass.

Here (capital sigma) just means "add up all of these."

Why the topic needs this: the entire "Derivation of energy released" and every worked -value on the parent page is just plugging masses into .


6. Binding energy per nucleon — the "map" that says which way is downhill

Figure — Fusion — solar fusion, tokamak (concept)

The picture: figure s03 is the famous Binding Energy per Nucleon Curve. It rises steeply from hydrogen, peaks near iron (, about per nucleon), then gently falls. Higher up the curve = more tightly bound = more stable.

Why the topic needs this: this curve is the reason fusion releases energy at all, and why only light nuclei qualify.


7. Plasma — the stuff inside the reactor

Why the topic needs this: you can't magnetically grab a neutral gas. Fusion fuel must first become plasma so magnets can hold it.


8. Magnetic field , velocity , and the Lorentz force

Figure — Fusion — solar fusion, tokamak (concept)

The picture: figure s04. A charged particle moves along ; the field points into the region; the resulting force points sideways, at a right angle to . A force forever sideways to motion doesn't speed the particle up or slow it down — it curves the path into a circle. So charged particles spiral around field lines instead of crossing them.

Why the topic needs this: this is why a magnetic doughnut can confine plasma — particles are leashed to the looped field lines. It also debunks the "magnet heats the plasma" mistake on the parent page.


9. Putting the confinement symbols together: , , and the triple product

Why the topic needs this: this single line is the scoreboard for "did the reactor produce more energy than it cost."


The prerequisite map

Proton neutron nucleus

Nuclide notation A Z X

Coulomb repulsion and strong force

Temperature T heats fuel

Rest mass and mass defect

E equals m c squared gives Q

Binding energy per nucleon curve

Why fusion releases energy

Plasma charged soup

Magnetic field and Lorentz force

Magnetic confinement torus

Lawson triple product n T tau

FUSION topic


Equipment checklist

Test yourself — cover the right side and answer:

What do the top and bottom numbers in mean?
Top = protons + neutrons (mass number); bottom = number of protons (charge).
Why do two nuclei resist fusing?
Both are positively charged, so the Coulomb force pushes them apart; you must climb that barrier.
What force finally sticks them, and over what range?
The strong nuclear force — extremely strong but only over a nucleus-sized distance.
What does stand for?
Change in mass = (total mass before) − (total mass after); the sliver that becomes energy.
State in words and give the u→MeV conversion.
Energy equals mass times the speed of light squared; .
What is and where does its curve peak?
Binding energy per nucleon; it peaks near iron-56 at about .
Why does fusion release energy only for light nuclei?
Joining light nuclei moves you up toward the iron peak (more tightly bound); heavy nuclei are already past the peak.
What is plasma and why does it matter for a tokamak?
A hot soup of free ions and electrons; being charged, it can be held by magnetic fields.
Why does the magnetic force do no work?
is always perpendicular to , so it steers but never speeds up or heats.
What three things multiply in the Lawson criterion?
Density , temperature , and energy confinement time .