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Chapter 04 · Unit 4 · 7 syllabus hours

Statistical Methods in Analytical Chemistry

Counting is a statistical act: probability and the binomial distribution, radioactivity as a statistical phenomenon, the standard deviation of counting data, the Poisson distribution, and how to optimise a counting experiment.

Semester VII CHEM7012 Nuclear Analytical 7 syllabus hours ≈ 20 min read 6 PYQs · solved counting statistics
Unit 4 · Statistical Methods in Analytical Chemistry Live

1 Chapter overview

Every number you will ever measure in nuclear chemistry comes from counting — counts of disintegrations, counts of particles reaching a detector, counts in a minute. And counting is a statistical act. Count the same source twice for five minutes each and you will get two different numbers. That scatter is not sloppy technique; it is the physics of radioactive decay itself.

Each nucleus in your sample decays independently, with only a tiny probability of decaying in any given second. With millions of nuclei, the total number that happen to decay while you watch fluctuates randomly about a mean. This chapter gives you the mathematics of that fluctuation — the binomial and Poisson distributions — and shows how to extract the two things every chemist needs from a counting experiment: the best value and its uncertainty.

  • §2 Concepts — why decay is random, the probability rules you need, and what each distribution describes.
  • §3 Derivations — the binomial law from coin-toss logic, rˉ=np\bar{r} = np, σ2=npq\sigma^{2} = npq, the binomial → Poisson limit, σ=N\sigma = \sqrt{N} for counting data, background-subtraction error propagation, and the optimal split of counting time.
  • §4 Examples — full numericals: rate ± error, counts needed for 1% precision, a χ² check of counter behaviour, background subtraction, optimal time division.
  • §6 PYQ bank — all 6 real questions (2022 and 2024), each solved.
📋 Exam record

This unit has appeared only in the 2022 and 2024 MSCH-102 papers, and only on three themes: the binomial distribution (derivation, asked twice), variance in terms of p (asked twice) and Poisson from binomial with its applicability conditions. Standard deviation of counting data and optimisation of counting experiments are in the syllabus but have never been asked — they are covered here in full from the reference books, marked with a "Syllabus, never asked" callout.

2 Core concepts

2.1 · Radioactivity is a statistical phenomenon

You cannot predict when a single nucleus will decay. There is no internal clock; the decay constant λ\lambda is a probability per unit time — in a short interval Δt\Delta t, each undecayed nucleus has probability λ Δt\lambda\,\Delta t of decaying, independent of its history and of every other nucleus. This is why radioactivity is called a statistical phenomenon: the law N=N0e−λtN = N_{0}e^{-\lambda t} predicts only the fraction of a large number of nuclei surviving, never the fate of one.

In a counting experiment you watch a vast number nn of nuclei, each with a tiny probability pp of producing a recorded count in your counting interval. The count you get is one random draw from a distribution — repeat the count and you get a different draw. The whole of this chapter is the statistics of those draws.

2.2 · The probability rules you need

An event is one possible outcome of a trial (a nucleus decays / does not decay in Δt\Delta t). Its probability PP is a number between 0 and 1 measuring how likely it is. Two rules do all the work in this chapter:

  • Addition rule (mutually exclusive events — they cannot both happen): P(A∪B)=P(A)+P(B)P(A \cup B) = P(A) + P(B). Example: the probability of getting either exactly 3 or exactly 4 counts is P(3)+P(4)P(3) + P(4).
  • Multiplication rule (independent events — one does not affect the other): P(A∩B)=P(A) P(B)P(A \cap B) = P(A)\,P(B). Example: if each nucleus decays with probability pp in Δt\Delta t, the probability that three specified nuclei all decay is p3p^{3}.

A sequence of nn independent trials, each with the same success probability pp, is called a set of Bernoulli trials — the coin-toss model. Radioactive counting is a Bernoulli process with enormous nn and tiny pp.

2.3 · The three distributions of this chapter

DistributionDescribesParametersMeanVariance
Binomialnumber of successes rr in a fixed number nn of trialsn,pn, pnpnpnpqnpq
Poissonnumber of rare, random events rr in a fixed interval of time/spaceμ\mu (mean count)μ\muμ\mu
Normal (Gaussian)large-sample limit of both; the familiar bell curveμ,σ\mu, \sigmaμ\muσ2\sigma^{2}
  • Binomial is the exact, fundamental law: it answers "in nn trials with success probability pp each, what is the chance of exactly rr successes?"
  • Poisson is the binomial law in the limit n→∞n \to \infty, p→0p \to 0 with np=μnp = \mu held fixed — exactly the situation of a counting experiment (huge number of nuclei, tiny per-nucleus probability). Its signature: variance equals mean, σ2=μ\sigma^{2} = \mu.
  • Normal is what both become when the mean is large (roughly μ≳20–30\mu \gtrsim 20\text{–}30): the distribution turns symmetric and bell-shaped with σ=μ\sigma = \sqrt{\mu}. In practice, counting data with more than a few dozen counts is treated as normal — which is why "±N\pm\sqrt{N} error bars" work.
🔑 The one line to remember

For counting data the total count NN estimates the Poisson mean, so the standard deviation of the count is the square root of the count: σN=N\sigma_{N} = \sqrt{N}, and the relative standard deviation is 1/N1/\sqrt{N}. Want 1% precision? You need N=10,000N = 10{,}000 counts. Want 0.1%? N=106N = 10^{6}.

2.4 · Where the syllabus topics sit

  • Counting statistics — this whole chapter: treating a count as a random variable with a distribution, not as an exact number.
  • Probability and binomial distribution — §2.2 and the binomial derivation in §3.
  • Radioactivity as a statistical phenomenon — §2.1: decay is random per nucleus, predictable only in the large-number average.
  • Standard deviation of counting data — σ=N\sigma = \sqrt{N}, relative error 1/N1/\sqrt{N}, background subtraction.
  • Poisson distribution — derived as the binomial limit; the working distribution of counting experiments.
  • Optimisation of counting experiments — how to split a fixed total time between sample and background, and preset-count versus preset-time.

3 Key derivations

3.1 · The binomial distribution law

🔥 Exam favourite — asked 2022(a) and 2024(a)

Learn this derivation cold, with every symbol defined. It is the single most repeated question of this unit.

Set up the trials. Consider nn independent, identical trials. In each trial the probability of "success" is pp and of "failure" is q=1−pq = 1 - p. (In counting: a trial is one nucleus in the counting interval; "success" is its decay being recorded.)

One particular sequence. Fix attention on one specific order of outcomes — say the first rr trials succeed and the remaining n−rn-r fail. The trials are independent, so by the multiplication rule the probability of this exact sequence is pr q n−rp^{r}\,q^{\,n-r}. Every specific sequence with rr successes and n−rn-r failures has this same probability.

Count the sequences. How many distinct sequences contain exactly rr successes among nn trials? Choose which rr of the nn positions hold the successes: (nr)=n!r!(n−r)!\binom{n}{r} = \frac{n!}{r!(n-r)!} ways. These sequences are mutually exclusive.

Add them up. By the addition rule, the probability of exactly rr successes in any order is the number of sequences times the probability of each:

(1)P(r)=(nr) pr q n−r,q=1−pP(r) = \binom{n}{r}\,p^{r}\,q^{\,n-r}, \qquad q = 1-p

Meaning of every symbol: P(r)P(r) — probability of obtaining exactly rr successes; nn — total number of independent trials (fixed); rr — number of successes observed, r=0,1,…,nr = 0, 1, \ldots, n; pp — probability of success in a single trial (same for all trials); q=1−pq = 1-p — probability of failure in a single trial; (nr)\binom{n}{r} — binomial coefficient, the number of ways to choose the rr successful trials out of nn.

3.2 · Mean of the binomial distribution: rˉ=np\bar{r} = np

🔥 Exam favourite — asked 2024(b)

A short, clean proof. Examiners expect the combinatorial identity r(nr)=n(n−1r−1)r\binom{n}{r} = n\binom{n-1}{r-1} used explicitly.

Write the mean as a sum. By definition, rˉ=∑r=0nr P(r)=∑r=0nr(nr)prqn−r\bar{r} = \sum_{r=0}^{n} r\,P(r) = \sum_{r=0}^{n} r\binom{n}{r}p^{r}q^{n-r}. The r=0r = 0 term is zero.

Use the identity r(nr)=n(n−1r−1)r\binom{n}{r} = n\binom{n-1}{r-1} (check: r⋅n!/[r!(n−r)!]=n⋅(n−1)!/[(r−1)!(n−r)!]r\cdot n!/[r!(n-r)!] = n\cdot (n-1)!/[(r-1)!(n-r)!]. Pull the constant nn out and split one power of pp:

rˉ=np∑r=1n(n−1r−1) p r−1 q (n−1)−(r−1)\bar{r} = np\sum_{r=1}^{n}\binom{n-1}{r-1}\,p^{\,r-1}\,q^{\,(n-1)-(r-1)}

Recognise the binomial expansion. Put s=r−1s = r-1; the sum is ∑s=0n−1(n−1s)psq(n−1)−s=(p+q)n−1\sum_{s=0}^{n-1}\binom{n-1}{s}p^{s}q^{(n-1)-s} = (p+q)^{n-1}. Since p+q=1p + q = 1, the sum equals 1.

(2)rˉ=np\bar{r} = np

3.3 · Variance of the binomial distribution: σ2=npq\sigma^{2} = npq

🔥 Exam favourite — asked 2022(b) and 2024(c)

The question asks for variance "in terms of p" — the expected final line is σ2=np(1−p)\sigma^{2} = np(1-p). Derive it via E[r(r−1)]E[r(r-1)]; it is far shorter than expanding (r−rˉ)2(r-\bar{r})^{2} directly.

Variance in terms of moments. σ2=(r−rˉ)2‾=r2‾−rˉ2\sigma^{2} = \overline{(r-\bar{r})^{2}} = \overline{r^{2}} - \bar{r}^{2}, where r2‾=∑r2P(r)\overline{r^{2}} = \sum r^{2}P(r). Write r2=r(r−1)+rr^{2} = r(r-1) + r, so r2‾=r(r−1)‾+rˉ\overline{r^{2}} = \overline{r(r-1)} + \bar{r}.

Evaluate r(r−1)‾\overline{r(r-1)}. Using r(r−1)(nr)=n(n−1)(n−2r−2)r(r-1)\binom{n}{r} = n(n-1)\binom{n-2}{r-2}:

r(r−1)‾=∑r=2nr(r−1)(nr)prqn−r=n(n−1)p2∑s=0n−2(n−2s)psq(n−2)−s\overline{r(r-1)} = \sum_{r=2}^{n}r(r-1)\binom{n}{r}p^{r}q^{n-r} = n(n-1)p^{2}\sum_{s=0}^{n-2}\binom{n-2}{s}p^{s}q^{(n-2)-s}

The sum is (p+q)n−2=1(p+q)^{n-2} = 1, so r(r−1)‾=n(n−1)p2\overline{r(r-1)} = n(n-1)p^{2}.

Assemble. r2‾=n(n−1)p2+np\overline{r^{2}} = n(n-1)p^{2} + np, and rˉ2=n2p2\bar{r}^{2} = n^{2}p^{2}. Hence σ2=n(n−1)p2+np−n2p2=np−np2=np(1−p).\sigma^{2} = n(n-1)p^{2} + np - n^{2}p^{2} = np - np^{2} = np(1-p).

(3)σ2=npq=np(1−p),σ=npq\sigma^{2} = npq = np(1-p), \qquad \sigma = \sqrt{npq}

3.4 · The Poisson distribution as the limit of the binomial

🔥 Exam favourite — asked 2022(c)

Do this limit carefully, one factor at a time. The examiner wants to see why each piece tends to its limit.

Take the binomial law and fix the mean. Start from P(r)=n!r!(n−r)! pr(1−p) n−rP(r) = \frac{n!}{r!(n-r)!}\,p^{r}(1-p)^{\,n-r}. Now let the number of trials grow without bound, n→∞n \to \infty, while the per-trial probability shrinks, p→0p \to 0, in such a way that the mean stays fixed: np=μnp = \mu (constant). Substitute p=μ/np = \mu/n:

P(r)=n(n−1)⋯(n−r+1)r!(μn)r(1−μn)n−rP(r) = \frac{n(n-1)\cdots(n-r+1)}{r!}\left(\frac{\mu}{n}\right)^{r}\left(1-\frac{\mu}{n}\right)^{n-r}

Regroup into three factors:

P(r)=μrr!×n(n−1)⋯(n−r+1)nr⏟(A)×(1−μn)n⏟(B)×(1−μn)−r⏟(C) ,P(r) = \frac{\mu^{r}}{r!}\times \underbrace{\frac{n(n-1)\cdots(n-r+1)}{n^{r}}}_{\text{(A)}}\times \underbrace{\left(1-\frac{\mu}{n}\right)^{n}}_{\text{(B)}}\times \underbrace{\left(1-\frac{\mu}{n}\right)^{-r}}_{\text{(C)}}\,,

where (1−μn)n−r=(1−μn)n(1−μn)−r\left(1-\frac{\mu}{n}\right)^{n-r} = \left(1-\frac{\mu}{n}\right)^{n}\left(1-\frac{\mu}{n}\right)^{-r} was used.

Take the limit term by term. (A) has rr factors, each of the form (n−k)/n=1−k/n→1(n-k)/n = 1 - k/n \to 1, so (A) → 1. (C) has a fixed exponent −r-r, and (1−μ/n)→1(1-\mu/n) \to 1, so (C) → 1. (B) is the classic exponential limit: lim⁡n→∞(1−μ/n)n=e−μ\lim_{n\to\infty}(1-\mu/n)^{n} = e^{-\mu}.

(4)P(r)=μr e−μr!r=0,1,2,…P(r) = \frac{\mu^{r}\,e^{-\mu}}{r!}\qquad r = 0, 1, 2, \ldots

Conditions for Poisson to apply to a counting experiment (the second half of the 2022 question): the limit above demands (i) a very large number of nuclei, n→∞n \to \infty; (ii) a very small probability of any one nucleus being counted in the interval, p→0p \to 0; (iii) a finite, constant mean count μ=np\mu = np. In laboratory language: disintegrations must be random, independent events occurring at a constant average rate — the source must not decay appreciably during the count, geometry and detector efficiency must stay fixed, and dead-time losses must be negligible. Then μ\mu is estimated by the observed mean count, and — the Poisson signature — variance equals mean.

3.5 · Mean and variance of the Poisson distribution

Mean. rˉ=∑r=0∞r μre−μr!=μe−μ∑r=1∞μr−1(r−1)!=μe−μ⋅eμ=μ.\bar{r} = \sum_{r=0}^{\infty} r\,\frac{\mu^{r}e^{-\mu}}{r!} = \mu e^{-\mu}\sum_{r=1}^{\infty}\frac{\mu^{r-1}}{(r-1)!} = \mu e^{-\mu}\cdot e^{\mu} = \mu. (The series is eμe^{\mu}.)

Variance. r(r−1)‾=μ2e−μ∑r=2∞μr−2/(r−2)!=μ2\overline{r(r-1)} = \mu^{2}e^{-\mu}\sum_{r=2}^{\infty}\mu^{r-2}/(r-2)! = \mu^{2}, so r2‾=μ2+μ\overline{r^{2}} = \mu^{2} + \mu and σ2=r2‾−rˉ2=μ.\sigma^{2} = \overline{r^{2}} - \bar{r}^{2} = \mu.

(5)Poisson:rˉ=μ,σ2=μ,σ=μ\text{Poisson:}\quad \bar{r} = \mu,\qquad \sigma^{2} = \mu,\qquad \sigma = \sqrt{\mu}

3.6 · Standard deviation of counting data: σ=N\sigma = \sqrt{N}

Syllabus, never asked

Never appeared in 2020–2024, but it is explicitly in the syllabus and it is the most-used result of the chapter in real analytical work. Examiners can lift it straight from Friedlander or Arnikar at any time.

Identify the Poisson mean with the observed count. A counting experiment satisfies the Poisson conditions (§3.4), so the counts follow P(r)=μre−μ/r!P(r) = \mu^{r}e^{-\mu}/r! with σ2=μ\sigma^{2} = \mu. The best (maximum-likelihood) estimate of the unknown true mean μ\mu from a single measurement is the observed total count NN itself.

Read off the standard deviation. Replacing μ\mu by its estimate NN:

(6)σN=N,σNN=1N\sigma_{N} = \sqrt{N}, \qquad \frac{\sigma_{N}}{N} = \frac{1}{\sqrt{N}}

So a count of N=10,000N = 10{,}000 carries σ=100\sigma = 100, i.e. ±1% relative. For a count rate R=N/tR = N/t measured over time tt, dividing by the exact time gives σR=N/t=R/t\sigma_{R} = \sqrt{N}/t = \sqrt{R/t}. Two consequences examiners love: (a) the absolute error grows as N\sqrt{N} while the relative error shrinks as 1/N1/\sqrt{N}; (b) to halve the relative error you must quadruple the counts (or the counting time).

3.7 · Background subtraction and error propagation

Syllabus, never asked

Straight from the reference books. Any numerical on "net count rate" needs this.

A real measurement gives gross counts NsN_{s} in time tst_{s}; a separate background count gives NbN_{b} in time tbt_{b}. The net (sample-only) rate is Rn=Rs−RbR_{n} = R_{s} - R_{b} with Rs=Ns/tsR_{s} = N_{s}/t_{s}, Rb=Nb/tbR_{b} = N_{b}/t_{b}. The two counts are independent Poisson variables, and for a sum or difference of independent quantities variances add (never standard deviations):

Net counts. Nn=Ns−NbN_{n} = N_{s} - N_{b}, so σn2=σs2+σb2=Ns+Nb\sigma_{n}^{2} = \sigma_{s}^{2} + \sigma_{b}^{2} = N_{s} + N_{b}. Note the background increases the error even though it is subtracted from the value.

Net rate. Rn=Ns/ts−Nb/tbR_{n} = N_{s}/t_{s} - N_{b}/t_{b}; the times are exact, so σRn2=σs2/ts2+σb2/tb2=Ns/ts2+Nb/tb2.\sigma_{R_{n}}^{2} = \sigma_{s}^{2}/t_{s}^{2} + \sigma_{b}^{2}/t_{b}^{2} = N_{s}/t_{s}^{2} + N_{b}/t_{b}^{2}.

(7)σRn2=Rsts+Rbtb(Rn=Rs−Rb)\sigma_{R_{n}}^{2} = \frac{R_{s}}{t_{s}} + \frac{R_{b}}{t_{b}} \qquad \bigl(R_{n} = R_{s} - R_{b}\bigr)

using Ns/ts2=Rs/tsN_{s}/t_{s}^{2} = R_{s}/t_{s}. If background is negligible, this collapses to σR=R/t\sigma_{R} = \sqrt{R/t}.

3.8 · Optimisation: how to split the counting time

Syllabus, never asked

The syllabus says "optimisation of counting experiments". This is the standard textbook result (Evans; Friedlander, Kennedy and Macias): with total time TT fixed, do not split it equally — give more time to whichever count is noisier.

Minimise the net-rate variance. From (7), with ts+tb=Tt_{s} + t_{b} = T fixed, minimise f(ts)=Rs/ts+Rb/(T−ts)f(t_{s}) = R_{s}/t_{s} + R_{b}/(T - t_{s}). Differentiate and set to zero:

dfdts=−Rsts2+Rb(T−ts)2=0    ⟹    Rsts2=Rbtb2.\frac{df}{dt_{s}} = -\frac{R_{s}}{t_{s}^{2}} + \frac{R_{b}}{(T-t_{s})^{2}} = 0 \;\;\Longrightarrow\;\; \frac{R_{s}}{t_{s}^{2}} = \frac{R_{b}}{t_{b}^{2}}.

Take square roots. Rs/ts=Rb/tb\sqrt{R_{s}}/t_{s} = \sqrt{R_{b}}/t_{b}, i.e.

(8)tstb=RsRb\frac{t_{s}}{t_{b}} = \sqrt{\frac{R_{s}}{R_{b}}}

(The second derivative is positive, so this is a minimum.) In words: split the time in proportion to the square roots of the rates — spend longer on the noisier (higher-rate) count. If sample and background rates are equal, split equally; if the sample is much hotter than background, most of the time goes to the sample. A useful companion choice is preset-count versus preset-time: in preset-time you fix tt and let the counts vary (Poisson); in preset-count you fix NN and measure the time needed. The relative precision of the rate is σR/R=1/N\sigma_{R}/R = 1/\sqrt{N} either way — preset-count simply guarantees the precision you asked for, while preset-time is operationally simpler.

4 Worked examples

Example 1 — Rate and its error from one count

Given. A sample gives N=2500N = 2500 counts in t=5t = 5 min.

Solution. The count rate is R=N/t=2500/5=500R = N/t = 2500/5 = 500 cpm. The standard deviation of the count is σN=N=2500=50\sigma_{N} = \sqrt{N} = \sqrt{2500} = 50. The time is exact, so the error in the rate is σR=σN/t=50/5=10\sigma_{R} = \sigma_{N}/t = 50/5 = 10 cpm. Result: R=500±10R = 500 \pm 10 cpm, a relative error of 10/500=2%10/500 = 2\%. (≈68% of repeat counts would fall in 490–510 cpm; ≈95% in ±2σ\pm 2\sigma, i.e. 480–520 cpm.)

Example 2 — How many counts for 1% precision?

Given. You need the count rate to ±1% relative.

Solution. Relative error =1/N= 1/\sqrt{N}. Set 1/N=0.01  ⇒  N=100  ⇒  N=10,0001/\sqrt{N} = 0.01 \;\Rightarrow\; \sqrt{N} = 100 \;\Rightarrow\; N = 10{,}000 counts. At 500 cpm that needs 10,000/500=2010{,}000/500 = 20 min of counting. For ±0.5% you need 1/N=0.005⇒N=40,0001/\sqrt{N} = 0.005 \Rightarrow N = 40{,}000 counts — four times the counts (80 min): halving the error always quadruples the counting time. Preset-count shortcut: set the scaler to stop at N=10,000N = 10{,}000; if it stops after 25.0 min, R=10,000/25.0=400R = 10{,}000/25.0 = 400 cpm with σR/R=1/10,000=1%\sigma_{R}/R = 1/\sqrt{10{,}000} = 1\%, i.e. 400±4400 \pm 4 cpm — the precision is guaranteed by the preset.

Example 3 — χ² check: is the counter behaving statistically?

Given. Ten successive 1-min background counts: 52, 41, 49, 58, 44, 50, 39, 55, 47, 51. Is the scatter consistent with pure statistical fluctuation?

Solution. Mean xˉ=486/10=48.6\bar{x} = 486/10 = 48.6. For Poisson data the test statistic χ2=∑i(xi−xˉ)2/xˉ\chi^{2} = \sum_{i}(x_{i}-\bar{x})^{2}/\bar{x} should be ≈ the degrees of freedom, n−1=9n-1 = 9. Deviations squared: 3.42+7.62+0.42+9.42+4.62+1.42+9.62+6.42+1.62+2.42=322.43.4^{2} + 7.6^{2} + 0.4^{2} + 9.4^{2} + 4.6^{2} + 1.4^{2} + 9.6^{2} + 6.4^{2} + 1.6^{2} + 2.4^{2} = 322.4, so χ2=322.4/48.6=6.63\chi^{2} = 322.4/48.6 = 6.63. The 95% acceptance band for χ92\chi^{2}_{9} is about 2.7–19.0, and 6.63 lies comfortably inside — the counter is behaving; the scatter is statistical. (A value far above ~19 would signal extra, non-statistical noise — drifting high voltage, for instance.)

Example 4 — Background subtraction with error propagation

Given. Gross count: Ns=3600N_{s} = 3600 in ts=10t_{s} = 10 min. Background: Nb=900N_{b} = 900 in tb=10t_{b} = 10 min.

Solution. Rates: Rs=360R_{s} = 360 cpm, Rb=90R_{b} = 90 cpm, net Rn=360−90=270R_{n} = 360 - 90 = 270 cpm. Variances add for a difference: σRn2=Rs/ts+Rb/tb=360/10+90/10=36+9=45\sigma_{R_{n}}^{2} = R_{s}/t_{s} + R_{b}/t_{b} = 360/10 + 90/10 = 36 + 9 = 45, so σRn=45=6.71\sigma_{R_{n}} = \sqrt{45} = 6.71 cpm. Result: Rn=270±6.7R_{n} = 270 \pm 6.7 cpm. Check via net counts: Nn=2700N_{n} = 2700, σn=3600+900=67.1\sigma_{n} = \sqrt{3600+900} = 67.1, and 67.1/10=6.7167.1/10 = 6.71 cpm ✓. Note the background contributes 9 of the 45 units of variance — subtracting background raises the error.

Example 5 — Optimal split of counting time

Given. Sample rate Rs=400R_{s} = 400 cpm, background Rb=100R_{b} = 100 cpm, total time T=30T = 30 min. Compare the optimal split with an equal split.

Solution. Optimal: ts/tb=Rs/Rb=4=2t_{s}/t_{b} = \sqrt{R_{s}/R_{b}} = \sqrt{4} = 2, so ts=20t_{s} = 20 min, tb=10t_{b} = 10 min. Then σ2=400/20+100/10=20+10=30\sigma^{2} = 400/20 + 100/10 = 20 + 10 = 30, σ=5.48\sigma = 5.48 cpm. Equal split (15/15): σ2=400/15+100/15=33.33\sigma^{2} = 400/15 + 100/15 = 33.33, σ=5.77\sigma = 5.77 cpm. Net rate Rn=300R_{n} = 300 cpm, so 300±5.5300 \pm 5.5 cpm optimal vs 300±5.8300 \pm 5.8 cpm equal-split. The gain is modest here but grows when the rates differ more — and it costs nothing.

5 Figures

Binomial distributions converging to the Poisson shape Three bar charts of the binomial distribution with mean np = 5 fixed: n = 10 with p = 0.5 is broad and symmetric, n = 25 with p = 0.2 is skewed, and n = 100 with p = 0.05 is close to the dashed Poisson limit curve. Binomial with fixed mean np = 5, approaching the Poisson limit n = 10, p = 0.50 0.0 0.1 0.2 r=0 r=5 r=10 n = 25, p = 0.20 0.0 0.1 0.2 r=0 r=5 r=10 n = 100, p = 0.05 0.0 0.1 0.2 r=0 r=5 r=10 bars = binomial P(r); dashed curve = Poisson limit (mean 5)
Fig. 1. The binomial distribution with fixed mean np=5np = 5 as nn grows and pp shrinks: at n=100,p=0.05n = 100, p = 0.05 the bars already hug the dashed Poisson curve — the §3.4 limit made visible.
Relative standard deviation 1 over root N versus total counts A log-log plot of relative standard deviation equal to 1 over the square root of N against total counts N. At 100 counts the relative error is 10 percent, at ten thousand counts it is 1 percent, and at one million counts it is 0.1 percent. Relative error falls as 1/√N (log–log) 10² 10³ 10⁴ 10⁵ 10⁶ 10⁷ 0.1% 1% 10% N = 100 → 10% N = 10,000 → 1% N = 1,000,000 → 0.1% total counts N (log scale) relative σ = 1/√N (log scale) to halve the error you must quadruple the counts
Fig. 2. Relative standard deviation 1/N1/\sqrt{N} against total counts on log–log axes — a straight line of slope −½. Memorise the three landmarks: 100 counts → 10%, 10⁴ counts → 1%, 10⁶ counts → 0.1%.
Optimal split of counting time between sample and background Variance of the net counting rate against the fraction of a fixed 30-minute total spent on the sample, for a 400 counts-per-minute sample and 100 counts-per-minute background. The curve is lowest at two thirds of the time on the sample, matching t_s over t_b equals the square root of R_s over R_b. Splitting 30 min between sample (400 cpm) and background (100 cpm) 0 0.25 0.5 0.75 1 30 45 60 75 90 minimum: t_s/t_b = √(R_s/R_b) = 2 equal split is worse fraction of time on sample, t_s/T variance of net rate σ² (cpm²) spend more time where the counts are noisier
Fig. 3. Variance of the net rate versus the fraction of a fixed total time spent on the sample. The minimum sits at ts/tb=Rs/Rbt_{s}/t_{b} = \sqrt{R_{s}/R_{b}} (dashed line, §3.8) — an equal split is measurably worse.

6 PYQ bank

Every question below was asked in a Burdwan M.Sc. MSCH-102 final paper — nothing is invented. This unit appears only in 2022 and 2024.

2022 · MSCH-102asked 2×

Q(a). Derive the binomial distribution law mentioning the meaning of all symbols used in the context of statistical data analysis.

Solution. See §3.1. Consider nn independent identical trials; in each, success has probability pp and failure q=1−pq = 1-p. One particular sequence with rr successes then n−rn-r failures has probability prq n−rp^{r}q^{\,n-r} by the multiplication rule. There are (nr)\binom{n}{r} such mutually exclusive sequences, so by the addition rule

P(r)=(nr) pr q n−r,q=1−p.P(r) = \binom{n}{r}\,p^{r}\,q^{\,n-r},\qquad q = 1-p.

Symbols: P(r)P(r) probability of exactly rr successes; nn number of trials (fixed); r=0,…,nr = 0,\dots,n successes observed; pp per-trial success probability; qq per-trial failure probability; (nr)=n!/[r!(n−r)!]\binom{n}{r} = n!/[r!(n-r)!] the number of ways to place the rr successes. (Repeated as 2024(a).)

2022 · MSCH-102asked 2×

Q(b). Write down the equation of "Variance" in terms of "probability of success (p)".

Solution. For the binomial distribution the variance is (derived in §3.3)

σ2=np(1−p)=npq,\sigma^{2} = np(1-p) = npq,

where nn is the number of trials and q=1−pq = 1-p the failure probability. Derivation sketch: σ2=r2‾−rˉ2\sigma^{2} = \overline{r^{2}}-\bar{r}^{2}; with r(r−1)‾=n(n−1)p2\overline{r(r-1)} = n(n-1)p^{2} and rˉ=np\bar{r} = np, one gets σ2=n(n−1)p2+np−n2p2=np(1−p)\sigma^{2} = n(n-1)p^{2}+np-n^{2}p^{2} = np(1-p). (Repeated as 2024(c).)

2022 · MSCH-102asked 1×

Q(c). Starting from binomial distribution, derive the expression for "Poisson distribution". Mention the condition that a radioactive counting experiment must satisfy so that Poisson distribution may be applied.

Solution. From P(r)=(nr)pr(1−p)n−rP(r) = \binom{n}{r}p^{r}(1-p)^{n-r}, let n→∞n \to \infty, p→0p \to 0 with np=μnp = \mu fixed, and put p=μ/np = \mu/n. Regrouping (full steps in §3.4),

P(r)=μrr!⋅n(n−1)⋯(n−r+1)nr⋅(1−μn)n⋅(1−μn)−r→n→∞μre−μr!.P(r) = \frac{\mu^{r}}{r!}\cdot\frac{n(n-1)\cdots(n-r+1)}{n^{r}}\cdot\left(1-\frac{\mu}{n}\right)^{n}\cdot\left(1-\frac{\mu}{n}\right)^{-r}\xrightarrow[n\to\infty]{}\frac{\mu^{r}e^{-\mu}}{r!}.

The first and third factors tend to 1, the middle one to e−μe^{-\mu}. Applicability conditions: the number of nuclei must be very large, the probability of any one nucleus being counted in the interval very small, with finite constant mean μ=np\mu = np — i.e. disintegrations must be random, independent events at a constant average rate (no appreciable decay during counting, fixed geometry and efficiency, negligible dead-time).

2024 · MSCH-102asked 2×

Q(a). Derive binomial distribution law mentioning the meaning of all symbols used in the context of statistical data analysis.

Solution. Identical to 2022(a) above: P(r)=(nr)prq n−rP(r) = \binom{n}{r}p^{r}q^{\,n-r} with q=1−pq = 1-p, from "one sequence has probability prqn−rp^{r}q^{n-r} (multiplication rule)" × "(nr)\binom{n}{r} mutually exclusive sequences (addition rule)". Symbol meanings: P(r)P(r) probability of exactly rr successes; nn trials; rr successes, 0≤r≤n0 \le r \le n; pp success probability per trial; qq failure probability per trial; (nr)\binom{n}{r} ways to choose the successful trials. Full derivation in §3.1.

2024 · MSCH-102asked 1×

Q(b). Prove that rˉ=np\bar{r} = np where the symbols carry usual meaning in the context of statistical data analysis.

Solution. rˉ=∑r=0nr(nr)prqn−r=np∑r=1n(n−1r−1)pr−1q(n−1)−(r−1),\bar{r} = \sum_{r=0}^{n} r\binom{n}{r}p^{r}q^{n-r} = np\sum_{r=1}^{n}\binom{n-1}{r-1}p^{r-1}q^{(n-1)-(r-1)},

using r(nr)=n(n−1r−1)r\binom{n}{r} = n\binom{n-1}{r-1}. With s=r−1s = r-1 the sum is ∑s=0n−1(n−1s)psq(n−1)−s=(p+q)n−1=1\sum_{s=0}^{n-1}\binom{n-1}{s}p^{s}q^{(n-1)-s} = (p+q)^{n-1} = 1, since p+q=1p+q = 1. Hence rˉ=np\bar{r} = np: the mean number of successes is the number of trials times the per-trial success probability. Full steps in §3.2.

2024 · MSCH-102asked 2×

Q(c). Hence, derive the equation of 'Variance' in terms of 'probability of success (p)'.

Solution. "Hence" points back to the binomial setup of Q(a)–(b). Using σ2=r2‾−rˉ2\sigma^{2} = \overline{r^{2}}-\bar{r}^{2} with r2‾=r(r−1)‾+rˉ\overline{r^{2}} = \overline{r(r-1)}+\bar{r}, and r(r−1)‾=n(n−1)p2\overline{r(r-1)} = n(n-1)p^{2} (via r(r−1)(nr)=n(n−1)(n−2r−2)r(r-1)\binom{n}{r} = n(n-1)\binom{n-2}{r-2}, together with rˉ=np\bar{r} = np from Q(b):

σ2=[n(n−1)p2+np]−n2p2=np−np2=np(1−p).\sigma^{2} = \bigl[n(n-1)p^{2} + np\bigr] - n^{2}p^{2} = np - np^{2} = np(1-p).

Full derivation in §3.3. (Same demand as 2022(b).)

7 Exam Q&A

Q1. Why is radioactivity called a statistical phenomenon?

A. The moment of decay of any single nucleus is unpredictable — the decay constant λ\lambda is only a probability per unit time (λΔt\lambda\Delta t in Δt\Delta t). Only for a huge number of nuclei does the fraction decaying become predictable, via N=N0e−λtN = N_{0}e^{-\lambda t}.

Q2. State the addition and multiplication rules of probability, with the condition for each.

A. Addition: P(A∪B)=P(A)+P(B)P(A \cup B) = P(A)+P(B) for mutually exclusive events. Multiplication: P(A∩B)=P(A) P(B)P(A \cap B) = P(A)\,P(B) for independent events. The binomial law uses multiplication for one fixed sequence of outcomes and addition over the (nr)\binom{n}{r} mutually exclusive sequences.

Q3. In P(r)=(nr)prqn−rP(r) = \binom{n}{r}p^{r}q^{n-r}, what is qq, and why must p+q=1p+q = 1?

A. q=1−pq = 1-p is the probability of failure in one trial. Success and failure are the only two, mutually exclusive and exhaustive outcomes of a trial, so their probabilities sum to 1 — which is also what makes the binomial probabilities sum to 1 via (p+q)n=1(p+q)^{n} = 1.

Q4. What is special about the variance of a Poisson distribution?

A. It equals the mean: σ2=rˉ=μ\sigma^{2} = \bar{r} = \mu, so σ=μ\sigma = \sqrt{\mu}. This is the entire basis of counting statistics — one measurement NN gives both the value and its error, σ=N\sigma = \sqrt{N}.

Q5. A scaler records 900 counts. Quote the result with its standard deviation and relative error.

A. σ=900=30\sigma = \sqrt{900} = 30, so 900±30900 \pm 30 counts; relative error 30/900=3.3%30/900 = 3.3\% (equivalently 1/9001/\sqrt{900}).

Q6. When subtracting background, why do variances add rather than standard deviations?

A. For independent random variables, the variance of a sum or difference is the sum of the variances — cross terms average to zero because the fluctuations are uncorrelated. So σn2=Ns+Nb\sigma_{n}^{2} = N_{s}+N_{b}: the background measurement adds error even though its value is subtracted.

Q7. State the optimal time-split rule. When is an equal split optimal?

A. ts/tb=Rs/Rbt_{s}/t_{b} = \sqrt{R_{s}/R_{b}}: split the total time in proportion to the square roots of the rates — more time for the noisier count. Equal split is optimal only when Rs=RbR_{s} = R_{b}.

Q8. Preset-count versus preset-time: which guarantees the precision you want, and what is the relative error in each?

A. Preset-count (fix NN, measure tt) guarantees the precision, because σR/R=1/N\sigma_{R}/R = 1/\sqrt{N} is set by your chosen NN. Preset-time (fix tt, count NN) gives the same formula, σR/R=1/N\sigma_{R}/R = 1/\sqrt{N}, but you only learn NN — and hence the precision — after the count.

8 Quick revision

(1) Binomial law

P(r)=(nr)prqn−r,  q=1−pP(r)=\binom{n}{r}p^{r}q^{n-r},\;q=1-p

(2) Binomial mean

rˉ=np\bar{r}=np

(3) Binomial variance

σ2=npq=np(1−p)\sigma^{2}=npq=np(1-p)

(4) Poisson law

P(r)=μre−μ/r!P(r)=\mu^{r}e^{-\mu}/r!

(5) Poisson mean = variance

rˉ=μ,  σ2=μ\bar{r}=\mu,\;\sigma^{2}=\mu

(6) Counting error

σN=N,  σrel=1/N\sigma_{N}=\sqrt{N},\;\sigma_{\rm rel}=1/\sqrt{N}

(7) Net-rate variance

σRn2=Rs/ts+Rb/tb\sigma_{R_{n}}^{2}=R_{s}/t_{s}+R_{b}/t_{b}

(8) Optimal time split

ts/tb=Rs/Rbt_{s}/t_{b}=\sqrt{R_{s}/R_{b}}

SymbolMeaningSymbolMeaning
P(r)P(r)probability of exactly rr successes/countsμ\muPoisson mean (= npnp in the limit)
nnnumber of independent trialsNNtotal counts observed
rrnumber of successes observedRRcount rate N/tN/t
ppsuccess probability per trialttcounting time
q=1−pq=1-pfailure probability per trialRs,RbR_{s}, R_{b}sample (gross) and background rates
rˉ\bar{r}mean of the distributionχ2\chi^{2}∑(xi−xˉ)2/xˉ\sum(x_{i}-\bar{x})^{2}/\bar{x}, ≈ n−1n-1 if statistical
σ2,σ\sigma^{2}, \sigmavariance, standard deviationλ\lambdadecay constant = decay probability per unit time