The Standard Normal Distribution

Introduces the standard normal distribution N(0,1)N(0,1) and its cumulative distribution function Φ\Phi. Covers reading P(Za)P(Z \leq a) directly from a standard normal table, the complement rule P(Z>a)=1Φ(a)P(Z > a) = 1 - \Phi(a), the symmetry identity Φ(a)=1Φ(a)\Phi(-a) = 1 - \Phi(a), and combining these to compute P(aZb)P(a \leq Z \leq b).

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Introduction

The standard normal distribution is a continuous probability distribution with mean μ=0\mu = 0 and standard deviation σ=1\sigma = 1. A random variable ZZ following this distribution is written ZN(0,1)Z \sim N(0, 1).

Its probability density function is

φ(z)=12πez2/2,\varphi(z) = \dfrac{1}{\sqrt{2\pi}}\, e^{-z^2/2},

whose graph is the familiar bell-shaped curve: symmetric about z=0z = 0, with total area under the curve equal to 11.

Probabilities involving ZZ correspond to areas under this curve. The cumulative distribution function of ZZ is

Φ(a)=P(Za).\Phi(a) = P(Z \leq a).

Values of Φ(a)\Phi(a) for a0a \geq 0 are listed in a standard normal table; for example, Φ(1.00)=0.8413\Phi(1.00) = 0.8413.

Two facts follow immediately from the shape of the curve:

  • By symmetry about z=0z = 0, exactly half the area lies to the left of 00, so Φ(0)=0.5\Phi(0) = 0.5.
  • Because ZZ is continuous, P(Z=a)=0P(Z = a) = 0 for every aa. Therefore P(Z<a)=P(Za)=Φ(a)P(Z < a) = P(Z \leq a) = \Phi(a).
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