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The Central Limit Theorem

The law of large numbers says Mn→μM_n\to\mu, but says nothing about the shape of the (shrinking) fluctuations around μ\mu along the way. The Central Limit Theorem (CLT) answers exactly that question, and the answer is the single most important reason the normal distribution is ubiquitous in probabilistic modelling: at the natural 1/n1/\sqrt n scale, the fluctuations of any sum of i.i.d. random variables — discrete, continuous, or mixed, whatever their own shape — converge to a normal distribution. This note states the theorem, develops the standard normal-approximation procedure, and works three examples that show the CLT in action: a package-weight sum, a counting problem disguised as a sum, and — most tellingly — a return to the polling problem of the previous two lessons, where the CLT's sample-size requirement turns out to be more than five times sharper than Chebyshev's.
Learning objectives. By the end of this note you should be able to:
  • state the Central Limit Theorem precisely, including what is and is not assumed about the XiX_i's distribution;
  • apply the normal-approximation procedure to compute an approximate probability for a sum of i.i.d. random variables;
  • apply the De Moivre-Laplace continuity correction when approximating a binomial with a normal;
  • explain why the CLT gives a materially sharper sample-size bound than Chebyshev's inequality.

In this lesson

  1. The theorem
  2. The normal approximation procedure
  3. Sharper than Chebyshev: the polling problem revisited
  4. The De Moivre-Laplace approximation and the continuity correction

Before you start

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