The probability that the true mean lies inside the computed interval [501.02,502.98] is 0.95.
False. Once computed, both endpoints and μ are fixed numbers, so μ is either in or out — probability 0 or 1. The 95% describes the long-run success rate of the method, not this one band.
A 99% confidence interval is more likely to be "correct" for a single given sample than a 95% one.
True in the long-run sense: a higher confidence level means a larger fraction of intervals capture μ. The cost is that the 99% interval is wider (uses a bigger critical value), so it is less precise.
Widening the confidence level from 95% to 99% makes the interval narrower because we are "more sure."
False. More confidence demands a bigger critical value (z0.005=2.576>1.96), which widens the band. Certainty and precision trade off against each other.
For the same data, the t-interval is always at least as wide as the z-interval.
True. For any finite n−1 degrees of freedom, tα/2,n−1>zα/2 because the t-distribution has fatter tails, so its critical value is larger. They converge only as n→∞ — see Student's t-distribution.
Doubling the sample size n halves the margin of error.
False. The margin scales like 1/n, so quadrupling n halves it; doubling n shrinks it only by a factor 1/2≈0.71. This is why big precision gains get expensive — see Sample Size Determination.
If a 95% CI for μ excludes the value 0, then a two-sided hypothesis test of μ=0 at level α=0.05 rejects.
True. This is the CI–test duality: the CI is exactly the set of null values that would not be rejected, so a value outside it is rejected — see Hypothesis Testing.
The confidence interval tells us the range in which 95% of individual data values fall.
False. It bounds the meanμ, whose spread is the standard error σ/n, not the raw data spread σ. A range for individual values (a prediction/tolerance interval) is much wider.
For a proportion, the standard error p^(1−p^)/n is largest when p^=0.5.
True. The function p(1−p) peaks at p=0.5 (value 0.25) and drops toward the extremes, so a 50/50 split is the hardest to pin down — this drives worst-case sample-size planning.
The Central Limit Theorem guarantees Xˉ is exactly normal for any sample size.
False. It gives an approximate normal shape for largen; for small n from a skewed population the approximation can be poor. See Central Limit Theorem.
"We're 95% confident, so we look up the 95th percentile z=1.645."
Error: two-sided intervals split α=0.05 into two tails of 0.025 each, so we need z0.025=1.96. The value 1.645 is a one-sided 95% bound.
"Since we don't know σ, we just use s in place of it and keep the z critical value, even for n=12."
Error: replacing σ by the random s adds uncertainty, so for small n we must use the wider tn−1 critical value, not z. Only for large n do they roughly agree.
"Margin of error =zα/2σ."
Error: the missing n makes the interval absurdly wide. The correct margin is zα/2σ/n because we bound the mean, whose spread is the standard error — see Standard Error.
"With 3 successes in 20 trials, p^=0.15, we apply the Wald interval directly."
Error: the validity check np^=20(0.15)=3<5 fails, so the normal approximation is unreliable. With so few successes the Wald interval can even spill below 0; use an exact or adjusted method instead.
"The t-distribution has n degrees of freedom."
Error: it has n−1. Computing s imposes the constraint ∑(Xi−Xˉ)=0, using up one degree of freedom and leaving n−1 free deviations.
"Because our 95% interval is [65.7,74.3], if we sampled again we'd get a mean in that range 95% of the time."
Error: the interval is about the fixed parameterμ, not about future sample means. A future Xˉ could easily fall outside; the 95% refers to how often intervals capture μ.
"A wider interval means our estimate is better."
Error: a wider interval means less precision — we've pinned μ down over a larger range. Narrow intervals (from larger n or smaller σ) are the precise ones; width and quality are inverted here.
Why do we split α into two equal tails instead of putting it all in one?
Because a symmetric two-sided interval brackets μ from both above and below, so we reserve α/2 probability in each tail; the central band then holds 1−α. A one-tailed split gives a one-sided bound, a different question.
Why does the variance of Xˉ shrink as σ2/n rather than staying σ2?
Averaging n independent values lets their random ups and downs partly cancel; the variance of the sum is nσ2, and dividing by n scales variance by 1/n2, leaving σ2/n.
Why must a proportion be treated as a special case of a mean?
A 0/1 (Bernoulli) trial has mean p and variance p(1−p), so p^ is literally the sample mean of these indicators; the whole mean machinery transfers with σ2 replaced by p(1−p) — see Bernoulli & Binomial Distributions.
Why do we plug p^ into the standard error when the true SE uses the unknown p?
We can't compute p(1−p)/n without knowing p, so we substitute our best estimate p^. This is the "Wald" approximation and is why the interval is only reliable when successes and failures are both plentiful.
Why does the t-interval get closer to the z-interval as n grows?
With more data, s estimates σ more accurately, so the extra uncertainty that fattened the t-tails vanishes and tn−1→N(0,1).
Why does "95% confidence" refer to the procedure and not to one interval?
Randomness lives in the sampling, not in μ. Before sampling, the yet-to-be-built band has a 95% chance of catching the fixed μ; after we observe data, the band is fixed too, so no probability remains to speak of.
The standard error σ/n→0, so the margin shrinks to zero and the interval collapses onto the true μ — infinite data pins the mean exactly.
What if p^=0 (zero successes observed)?
The Wald SE p^(1−p^)/n=0, giving the degenerate interval [0,0], which is clearly wrong — p isn't certainly zero. This is exactly where the approximation breaks and an adjusted (e.g. Wilson) interval is required.
What if the population is already exactly normal but n=2?
The z-approximation via CLT isn't needed for shape (it's normal already), but σ is unknown, so we still use tn−1=t1, whose tails are extremely fat — the interval is very wide, honestly reflecting how little two points tell us.
What happens to the margin when the confidence level is 100%?
The critical value zα/2 diverges to infinity (no finite band can be certain under a normal model), so a 100% interval is (−∞,∞) — technically always correct, practically useless.
What if σ=0 (no variability in the population)?
The standard error is 0, so every sample gives Xˉ=μ exactly and the interval collapses to the single point {μ} — with no randomness there is nothing to be uncertain about.
If two researchers each build a 95% CI from independent samples and the intervals don't overlap, is one of them definitely wrong?
Not necessarily — non-overlap is strong evidence the means differ but each interval individually still had a 5% miss chance, and non-overlap is a conservative (not exact) test for a difference.
Is μ random or fixed? ::: Fixed and unknown; the interval is the random object (before data are seen).
Does higher confidence give a narrower or wider interval? ::: Wider — a larger critical value is needed to catch μ more often.
When is the proportion standard error largest? ::: At p^=0.5, since p(1−p) peaks there.
Why n−1 and not n degrees of freedom? ::: Estimating s imposes one constraint ∑(Xi−Xˉ)=0, removing one free deviation.
Non-overlapping 95% CIs — proof of difference? ::: Strong but not definitive evidence; it's a conservative check, and each interval still had its own 5% miss rate.