Intuition The one core idea
A nucleus is a tight clump of protons and neutrons, and pulling that clump apart costs energy — which means the clump weighs slightly less than its loose pieces. Everything in this topic is just measuring that tiny missing mass, turning it into energy with E = m c 2 , and comparing "glue strength per particle" across nuclei.
Before you can read the parent note, you need the vocabulary it quietly assumes. This page builds every single symbol from nothing — plain words, then a picture, then why the topic needs it . Read top to bottom; each block leans on the one above.
Definition Proton and neutron — the nucleons
At the centre of every atom sits a tiny dense ball called the nucleus . It is built from two kinds of particle:
a proton — carries a positive electric charge,
a neutron — carries no charge (neutral).
Together, protons and neutrons are called nucleons ("things in the nucleus").
Look at the figure: the red balls are protons, the grey balls are neutrons, all crammed together. The parent note talks about "separated free nucleons" versus "the nucleus" — that is exactly the difference between the scattered balls on the right and the clumped balls on the left of the picture.
Intuition Why the clump doesn't fly apart
Same-charge things repel. All those positive protons should shove each other away. Something stronger must be holding them — the Strong nuclear force . That force is the "glue" the whole topic is really about.
Definition The three counting numbers
Z = the atomic number = how many protons the nucleus has. It also names the element (Z=2 is always helium).
N = the neutron number = how many neutrons .
A = the mass number = the total count of nucleons.
Definition Reading the symbol
Z A X
A nucleus is written Z A X : bottom-left is Z (protons), top-left is A (total nucleons), X is the element symbol.
1 2 H → Z = 1 , A = 2 , N = 2 − 1 = 1 ( 1 proton, 1 neutron )
2 4 He → Z = 2 , A = 4 , N = 2 ( 2 protons, 2 neutrons )
Recall Quick self-check
For 92 235 U , how many neutrons? ::: N = A − Z = 235 − 92 = 143 .
Definition The mass symbols
m p = mass of one proton (in practice the parent uses m 1 H , the mass of a hydrogen atom — a proton plus one electron).
m n = mass of one neutron .
M nucleus (or M atom ) = the actual measured mass of the whole nucleus (or atom).
Intuition The picture: a balance scale
Put all the loose nucleons on the left pan and the assembled nucleus on the right pan. The topic's central surprise is that the pans do not balance — the assembled nucleus is lighter. The next figure shows this.
The gap between the two pans is the star of the whole chapter. We give it a name in §5.
Definition Why a special mass unit
Nucleons are absurdly tiny (a proton is about 1.67 × 1 0 − 27 kg). Writing that repeatedly is painful, so physicists use a friendlier ruler: the atomic mass unit , symbol u .
1 u = 12 1 of the mass of one 12 C atom ≈ 1.6605 × 1 0 − 27 kg
On this scale a proton weighs almost exactly 1 u , a neutron just over 1 u — clean numbers like 1.007825 u .
u is just a convenient tick-mark
Think of u like measuring people in "average-adult-heights" instead of metres — the numbers become small and comparable. See Atomic mass unit (u) . Why the topic needs it: every table value and every worked example is quoted in u .
Δ (delta) = "the change / difference in"
The Greek capital delta Δ is a universal shorthand for "how much something differs." So Δ m literally reads "the difference in mass."
Common mistake "Defect" does not mean broken
Wrong feels right: "defect = flaw = something went wrong." Fix: here "defect" just means deficit / shortfall of mass. Nothing is broken — the mass turned into energy (next section).
E = m c 2 at all — and why THIS tool?
We have a leftover mass Δ m but the topic wants an energy (the "glue"). We need a bridge that converts mass into energy. That exact bridge is Einstein's Mass–energy equivalence ($E=mc^2$) : it is the only law that says mass and energy are two currencies for the same thing, with a fixed exchange rate c 2 . No other tool converts kilograms into joules.
Definition The symbols in
E = m c 2
E = energy,
m = mass,
c = the speed of light, c ≈ 3 × 1 0 8 m/s ; c 2 is the fixed "exchange rate" turning a little mass into a lot of energy.
Definition Binding energy
Binding energy E B = the energy you must pour in to rip a nucleus back into free nucleons (equally, the energy released when they first snapped together). By §5 and §6:
E B = Δ m c 2
Intuition The energy-well picture
In the figure, free nucleons sit at the top (high energy). As they fall together into the nucleus they drop into a well — the depth of that well is E B . To climb back out (break the nucleus) you must supply that same E B . Lower energy = lower mass, which is why the clump is lighter.
Definition Binding energy per nucleon
The bar over a symbol means "average." So
E B = A E B
reads "the average binding energy per nucleon " — total glue shared out over all A nucleons.
Why the topic needs it: total E B always grows with more nucleons, so it is unfair for comparing. Dividing by A asks the fair question "how hard is it to remove one average nucleon?" — the real stability score.
BE per nucleon E_B over A
Stability and the BE curve
Fusion and Fission release energy
Read it top to bottom: counts and masses give the mass defect , the mass–energy bridge turns it into binding energy , dividing by A gives the per-nucleon score, and that score explains the stability curve — and therefore Nuclear fusion and Nuclear fission .
Test yourself — you are ready for the parent note only if each reveal comes instantly.
What are nucleons, and which one is charged? Protons and neutrons; the proton is positively charged, the neutron is neutral.
What do Z , N and A count, and how are they related? Z = protons, N = neutrons, A = total nucleons; A = Z + N , so N = A − Z .
How do you read Z A X ? Bottom-left Z = protons, top-left A = total nucleons, X = element; neutrons = A − Z .
What is 1 u and why use it? One-twelfth of a 12 C atom's mass (≈ 1.66 × 1 0 − 27 kg); it makes nuclear masses clean small numbers.
What does Δ mean, and what is Δ m ? Δ = "difference in"; Δ m = mass of loose nucleons minus mass of the assembled nucleus.
Why is the assembled nucleus lighter than its parts? Assembling it releases binding energy that leaves the system, so by E = m c 2 the mass drops.
State the mass→energy conversion the topic uses. 1 u c 2 = 931.5 MeV, so E B = Δ m ( in u ) × 931.5 MeV.
What is E B in words? The energy needed to break a nucleus into free nucleons (or released when they combine).
What does the bar in E B mean and why divide by A ? "Average"; dividing total E B by A gives a fair per-nucleon stability score.