Intuition The one core idea
Radiation safety is really counting things that happen by pure chance : an atom might decay this second or not, a photon might be absorbed in this slab or not — and when countless tiny chances add up, you always get the same shape , an exponential curve. Master "constant probability per step ⇒ exponential" and every formula on the parent page (decay, activity, shielding) becomes the same picture wearing different labels.
This page assumes you have seen none of the notation. We build each symbol from plain words, tie it to a picture, and only then let it appear in a formula. When you are done, everything on the parent topic will read like sentences you already know.
Definition Nucleus (the thing that decays)
Every atom has a tiny dense centre called the nucleus — a clump of protons and neutrons. Some clumps are unstable : their internal forces don't quite balance, so sooner or later the clump rearranges and shoots out a particle. That event is a decay .
Picture a jar of popcorn kernels sitting on a hot plate. Each kernel might pop at any instant. It has no memory — a kernel that hasn't popped for a while is no more "ready" than a fresh one. The energy locked inside the nucleus is why it wants to change; the randomness is why we can only speak of probabilities.
We won't need the internal physics here — only this fact: each nucleus has a fixed chance of decaying in the next second, and it never ages.
N
N (capital N) just means "how many radioactive nuclei are present right now." It is a plain count — a whole number like 8,900,000,000,000,000,000. No units, just a tally.
Look at the jar in the figure. Each dot is one nucleus. N is simply how many dots are still un-popped. As time passes dots disappear, so N shrinks . That shrinking is the whole story of radioactivity — everything else measures how fast it shrinks.
Intuition WHY we need a "rate", and WHY calculus
We don't just want to know how many nuclei there are; we want how fast the count is dropping . "How fast something changes" is exactly the question calculus was invented to answer. The tool for it is the derivative .
Definition The derivative
d t d N
Read it aloud: "dee-N dee-tee " = the change in N for a tiny change in time t . Picture the count-vs-time curve in the next figure: the derivative is the steepness (slope) of that curve at each instant.
If the curve slopes downward , the slope is negative .
The steeper the drop, the larger (more negative) the number.
Because nuclei only ever leave the count (they don't come back), N always goes down , so d t d N is always negative . That is why the parent writes a minus sign :
− d t d N = ( how many decayed per second, as a positive number ) .
The minus flips the negative slope into a positive count of decays. Why bother? Because "number of decays per second" should feel positive — nobody says "minus 500 pops happened."
Common mistake "Why the minus? Isn't the rate positive?"
Feels right: decays are events, events are positive. Fix: d t d N measures the change in N , and N falls , so that quantity is negative. We attach − to report the decay count as the positive number we mean.
λ (Greek letter "lambda")
λ is the probability that any one nucleus decays in one second. Plain words: "the pop-rate per kernel." Its units are per second (s − 1 ) — a chance-per-unit-time.
Picture: give every dot in the jar the same tiny chance λ of vanishing this second. Then the total number vanishing this second is:
( chance each ) × ( how many ) = λ × N .
That product is the decay rate. Setting it equal to our positive decay count from §2:
− d t d N = λ N .
This is not a new law — it is the sentence "chance-per-nucleus times number-of-nuclei" written in symbols.
λ
A big λ = each nucleus is very likely to pop = the jar empties fast. A small λ = a sluggish, long-lasting source. Hold this: λ is the single dial that sets the speed of everything.
Intuition WHY exponential, and WHY the letter
e
When the rate of loss is proportional to how much is left , the amount follows a special curve: it drops by the same fraction in each equal time step (halve, then halve again, then again...). The number e ≈ 2.718 is the natural base that makes this "same-fraction-per-step" math clean. We use e (not 2 or 10) because it is the base for which the slope of the curve equals the curve's own height — exactly matching "− d N / d t = λ N ."
N = N 0 e − λ t
N 0 = the count at the start, when t = 0 (the "0 " subscript means "initial").
t = time elapsed.
e − λ t = the shrinking factor: at t = 0 it equals 1 (nothing lost yet); as t grows it slides toward 0 .
In the figure, notice the curve never touches zero — it just keeps halving. That "never quite gone" behaviour is why the parent says gamma rays are "never fully stopped, only attenuated." Same curve, different label.
t 1/2
The time for the count to fall to half . Read the subscript as "one-half." It is a friendlier way to state λ : instead of "chance per second," you say "time to lose half."
Definition The natural logarithm
ln
ln is the question-asker that undoes e . If e something = y , then ln y = that something . We need it because the unknown (λ t 1/2 ) is stuck up in the exponent, and ln is the tool that pulls an exponent back down to ground level. In particular ln 2 ≈ 0.693 .
To find t 1/2 : set the shrinking factor to one-half, e − λ t 1/2 = 2 1 , take ln of both sides (that's why we use ln — to free the exponent), and get
t 1/2 = λ l n 2 .
See Half-life and Radioactive decay law for the full walkthrough — here we only needed to earn the symbols.
A and the becquerel (Bq)
A = decays per second you'd actually detect from the sample. Since "decays per second" is exactly λ N :
A = λ N , 1 Bq = 1 decay per second .
The unit is named becquerel (Bq) . It's a rate , not a count — that's the whole distinction between A (per second) and N (plain tally).
Because N shrinks as e − λ t and A is just λ times N , activity rides the same exponential: A = A 0 e − λ t .
Now the three deposit-and-harm symbols. Each is one honest division or multiplication.
E and mass m
E = energy the radiation dumps into matter, measured in joules (J) . Picture a bullet stopping in sand: its motion-energy becomes broken bonds and heat.
m = mass of the stuff soaking it up, in kilograms (kg) .
D — the gray (Gy)
D = m E , 1 Gy = 1 kg J .
Divide energy by mass so we count "energy per kilogram of you ," which is what actually breaks chemical bonds — see Biological effects of radiation .
Definition Weighting factor
w R and equivalent dose H — the sievert (Sv)
w R = a plain multiplier ("radiation weighting factor") that says how nasty a given radiation type is per joule. Gamma/beta: w R = 1 ; alpha: w R = 20 . Then
H = w R ⋅ D , 1 Sv = 1 kg J ( weighted ) .
Same J/kg dimension as Gy, but multiplied by the harm-factor. That is why Gy and Sv look alike but mean different questions. Which particle you have (alpha vs gamma) comes from Types of radiation (alpha beta gamma) .
Definition The inverse-square idea
1/ r 2
Even with no shield, radiation gets weaker just by spreading out . The same energy paints a sphere whose area grows as r 2 (the surface of a sphere of radius r ), so the intensity per patch falls as 1/ r 2 . Doubling your distance quarters the dose — see Inverse-square law . That's the "Distance" pillar of protection.
Fixed chance per second lambda
Exponential N equals N0 e to minus lambda t
Half-life from ln 2 over lambda
Activity A equals lambda N in Bq
Weight by wR gives H in Sv
Same shape shielding I equals I0 e to minus mu x
Half-value layer ln 2 over mu
Inverse square one over r squared
Test yourself — cover the right side. If any line stumps you, re-read its section above before tackling the parent note.
What does the plain symbol N count? The number of radioactive nuclei present right now (a tally, no units).
What does d t d N measure, and why is it negative? The slope of the count-vs-time curve; negative because N only ever falls.
In plain words, what is λ and its units? The chance any one nucleus decays per second; units s − 1 .
Why does "− d N / d t = λ N " describe decay? Decays per second = (chance per nucleus λ ) × (number of nuclei N ).
Why is the base e (not 2 or 10) natural here? For e − λ t the slope equals the height, matching "− d N / d t = λ N ".
What does ln do and why do we need it for half-life? It undoes e , pulling the unknown down from the exponent to solve e − λ t 1/2 = 2 1 .
State t 1/2 in terms of λ . t 1/2 = ln 2/ λ ≈ 0.693/ λ .
How does activity A differ from the count N ? A = λ N is decays per second (a rate, Bq); N is a plain count.
Give absorbed dose D in words and units. Energy per unit mass, D = E / m , unit gray = 1 J/kg.
What is w R and why turn Gy into Sv with it? A harm-multiplier per radiation type; H = w R D converts physical energy to biological harm (Sv).
What makes the shielding law I = I 0 e − μx the twin of decay? Both come from constant chance per step — μ per metre plays the role of λ per second.
Why does intensity fall as 1/ r 2 with no shield at all? The energy spreads over a sphere whose area grows as r 2 , so intensity per patch drops as 1/ r 2 .