A Gaussian random variable is a random variable whose probability distribution is a normal distribution. For , write with a standard normal random variable ; conversely, standardization of a normal random variable recovers . For example, has mean , standard deviation , and variance . The outcome corresponds to standard score , one standard deviation above the mean.
Some definitions also allow a Gaussian random variable with . This means almost surely, with variance zero and probability distribution equal to the Dirac measure . It has no probability density function with respect to Lebesgue measure: . The positive-scale density formula and division by apply only when . MIT's constructive definition explicitly includes the constant case. [ref]
https://ocw.mit.edu/courses/6-436j-fundamentals-of-probability-fall-2018/ceb423b6a703abd60429367b733f45bf_MIT6_436JF18_lec14.pdf. MIT 6.436, Lecture 14, §2: degenerate normal distributions
.For independent standard Gaussian and , the partial sums are Cauchy in L2 space, since a tail's squared norm is the corresponding sum of coefficient squares. Completeness gives an limit. The finite-sum characteristic functions converge to , identifying the limit as Gaussian, including the zero-variance case. The identification needs convergence of distributions, not just agreement of the first two moments.
For independent standard Gaussian random variables, the partial sums have characteristic functions , where . A finite almost-sure limit implies convergence of these characteristic functions to one continuous at zero; would instead give zero at every nonzero . Conversely, bounded makes the partial sums an martingale bounded in L2 space, which converges almost surely and in L2 space.
Let , and stop on first reaching a fixed positive threshold. If the coefficient squares are summable, uniform integrability gives the stopped mean zero, with the terminal limit used on . If the coefficient squares diverge, for each fixed . Thus . This event is unaffected by changing finitely many of the independent variables, so the Kolmogorov zero-one law makes its probability one. Hence and is at least the positive threshold; its expectation, finite or infinite, cannot be zero.
A standard normal random variable has the standard normal distribution, mean zero and variance one. If with , the standardization of a normal random variable is a standard normal random variable. Its values report displacement from the mean in units of the standard deviation, so the result is a dimensionless quantity.
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