p-values
Step 1: Recall what Ξ± actually is
Ξ± is a threshold you pick in advance, before seeing data. It’s the maximum false-positive rate you’re willing to tolerate. You commit to a rule: “I’ll reject Hβ if my data lands in some rejection region R, and I’ve built R so that P(reject Hβ | Hβ true) β€ Ξ±.”
Common choices: Ξ± = 0.05, Ξ± = 0.01. You pick one Ξ±, run your test, and get a binary answer: reject or don’t reject.
The limitation: if you tested at Ξ± = 0.05 and rejected, you don’t know how strongly you rejected. Would you have also rejected at Ξ± = 0.01 (very strong evidence)? Or would you have failed to reject at Ξ± = 0.04 (borderline)? Testing at one fixed Ξ± throws this information away.
Step 2: The p-value fixes this β it summarizes ALL possible Ξ± at once
The p-value is the smallest Ξ± at which we would reject Hβ.
Think of it like a dial. As you slide Ξ± from 0 up to 1, at some point your test flips from “don’t reject” to “reject” β and it stays “reject” for all larger Ξ± from then on (this is what “we reject at all Ξ± β₯ p” is describing β it’s a one-way switch, not something that flickers back and forth).
The p-value is exactly the location of that switch.
Intuitive picture:
Ξ±: 0 -------- p -------- 1
Decision: [ don't reject ][ reject ]
So instead of running your test separately at Ξ± = 0.05, then Ξ± = 0.01, then Ξ± = 0.10, etc., the p-value tells you the entire history of what would’ve happened at every Ξ±, compressed into one number.
This is why “p < Ξ±” is the rejection rule. If p = 0.03:
- At Ξ± = 0.05: since 0.05 β₯ 0.03, you reject. β
- At Ξ± = 0.01: since 0.01 < 0.03, you don’t reject. β
The smaller the p-value, the stronger the evidence β it means you’d reject even at very strict (small) Ξ± thresholds.
Step 3: Theorem 11 β how to actually compute a p-value
$$p = \sup_{\theta \in \Theta_0} P_\theta\big(T_n(X_1,\ldots,X_n) \geq T_n(x_1,\ldots,x_n)\big)$$Don’t let the sup scare you β break it into pieces:
- $T_n(x_1, \ldots, x_n)$ is just a number: the test statistic you actually observed in your real data. Call this the “observed value.”
- $T_n(X_1, \ldots, X_n)$ is the test statistic as a random variable β what you’d get from a hypothetical fresh dataset.
- $P_\theta(T_n(X) \geq T_n(x))$ asks: “If ΞΈ were the true parameter, what’s the probability that a fresh random dataset gives a test statistic at least as extreme as what I actually observed?”
- The $\sup_{\theta \in \Theta_0}$ (supremum over the null region) says: check this probability for every ΞΈ allowed under Hβ, and take the worst case (largest probability) β this ensures your p-value is valid no matter which specific ΞΈ within Ξβ happens to be true.
Intuition: the p-value answers “assuming Hβ, how surprising/extreme is the data I actually got?” A small p-value means “this data would be really unusual if Hβ were true” β that’s evidence against Hβ.
Step 4: Example 12 β seeing this in action
Setup: $X_1, \ldots, X_n \sim N(\theta, 1)$, testing $H_0: \theta = \theta_0$ vs $H_1: \theta \neq \theta_0$ (two-sided test).
Here $\Theta_0$ is just a single point, ${\theta_0}$ β so no need for sup, just plug in $\theta_0$ directly.
- $T_n = \sqrt{n}(\bar{X}_n - \theta_0)$ β this measures how far your sample mean is from the hypothesized value, scaled by sample size.
- $t_n$ = the actual observed value of $T_n$ from your real data.
- We reject when $|T_n|$ is large (far from 0 in either direction β makes sense for a two-sided test).
Under $H_0$, $T_n \sim N(0,1)$ exactly (that’s why they call it $Z$). So:
$$p = P_{\theta_0}(|T_n| \geq |t_n|) = P(|Z| \geq |t_n|) = 2\Phi(-|t_n|)$$In words: “If Hβ is true, what’s the probability a fresh sample would give a $|T_n|$ value at least as extreme as what I got?” The $2\Phi(-|t_n|)$ formula is just the standard normal tail probability, doubled because it’s two-sided (extreme in either direction counts).
If your observed $t_n$ was huge (far from 0), that tail probability is tiny β small p-value β strong evidence against Hβ. Exactly matches intuition: “my data is really unlikely under Hβ” = “evidence against Hβ.”
Step 5: Theorem 13 β p ~ Uniform(0,1) under Hβ
This is a slightly deeper fact, but here’s the intuition: if Hβ is really true, then your p-value is just as likely to be 0.5 as 0.05 as 0.83 β it’s uniformly random over [0,1]. There’s no reason for it to systematically be small unless Hβ is actually false.
This is why p < Ξ± gives you a valid test with false-positive rate Ξ±: if Hβ is true, $P(p < \alpha) = \alpha$ exactly (since p is uniform). So testing “reject if p < Ξ±” automatically controls your Type I error rate at Ξ±, by construction.
Step 6: The crucial warning β p β P(Hβ | data)
This is probably the single most common misinterpretation of p-values, so it’s worth being very explicit:
- p-value = P(data this extreme or more | Hβ is true) β this is a frequentist quantity. It says nothing directly about whether Hβ is true; it’s about how surprising your data would be if Hβ were true.
- P(Hβ | data) = “given what I observed, what’s the probability Hβ is true?” β this is a Bayesian quantity, and requires a prior probability on Hβ to even define. Classical (frequentist) hypothesis testing doesn’t compute this at all.
Common wrong interpretation: “p = 0.03 means there’s a 3% chance Hβ is true.” This is false. The p-value is a statement about the data’s extremity assuming Hβ, not a probability statement about Hβ itself.
Summary intuition to hold onto: the p-value is a dial-sweep over all possible Ξ± thresholds, condensed into one number that tells you exactly how strong your evidence against Hβ is β small p = would’ve rejected even under very strict standards = strong evidence.