Scalar Random Variables (GPS)

This section presents various fundamental concepts related to probability and random variables that will be required to support subsequent discussions. The discussion will focus on continuous random variables.

Basic Properties

Let w represent a real, scalar random variable. In the following, the notationtmp3AC511_thumbdenotes the probability that the random variable w is less than the real number W.

The distribution function of the random variable w is defined as the function

tmp3AC512_thumb

The functiontmp3AC513_thumbis monotonically increasing in W, is continuous from the right withtmp3AC514_thumbThe derivative of the distribution function is the (density function of the random variable w and will be denoted by


tmp3AC517_thumb

The density function has the interpretation thattmp3AC518_thumbrepresents the probability that the random variable w assumes a value in the differential range tmp3AC519_thumbBecause the density is the derivative of a monotone function, tmp3AC520_thumbfor any W. Based on the above definitions, for a scalar random variable,

tmp3AC524_thumb

Lettmp3AC525_thumbbe a function of the random variable w. The expected value of tmp3AC526_thumbis defined by

tmp3AC529_thumb

In particular, the expected value or mean of w is

tmp3AC530_thumb

As a simplified notation, this topic will typically use the notationtmp3AC531_thumbto indicate the expected value of the random variabletmp3AC532_thumbIn cases where the meaning is clear or where double subscripting would otherwise occur, the subscript indicating the random variable may be dropped.

The variance of a scalar valued random variabletmp3AC533_thumbis defined by

tmp3AC537_thumb

The variance of a random variable quantifies the variation of the random variable relative to its expected value. If we definetmp3AC538_thumb is called the standard deviation oftmp3AC539_thumb

The fc-th moment oftmp3AC540_thumbis defined by

tmp3AC544_thumb

The first moment is the mean value. The variance and second moment are related by eqn. (4.13):

tmp3AC545_thumb

Example 4.3 Compute the mean, second moment, variance, and standard deviation of the random variable x with the exponential density

tmp3AC546_thumb

where

tmp3AC547_thumb

The mean is

tmp3AC548_thumb

The second moment is

tmp3AC549_thumb

The variance istmp3AC550_thumbbut can also be easily calculate from the information above using the eqn. (4-13) as

tmp3AC552_thumb

Therefore, the standard deviation istmp3AC553_thumb

Gaussian Distributions

The notationtmp3AC554_thumbis used to indicate that the scalar (or univariate) random variable x has the Gaussian or Normal density function described by

tmp3AC556_thumb

therefore, the density of a Normal random variable is completely described by two parameterstmp3AC557_thumbIt can be shown that

tmp3AC559_thumb

therefore, the parameterstmp3AC560_thumbare the expected value and variance of the random variable x.

Transformations of Scalar Random Variables

This section presents the method to find the density for the random variable v under the conditions thattmp3AC562_thumbthe function g is invertible, and the density for the random variable w is known.

Due to the assumption that g is monotone, it has an inverse function tmp3AC563_thumbThe derivation begins with the basic idea that the probability of the events causingtmp3AC564_thumband

tmp3AC565_thumbmust be the same whether measured with respect totmp3AC566_thumbMathematically this is expressed astmp3AC567_thumbtmp3AC568_thumbtmp3AC572_thumb

where this formulation assumes that dW is positive. Therefore,tmp3AC573_thumb which will be used below. For positive, dW, the quantity dV can still be either positive or negative, depending on the sign oftmp3AC574_thumbThe computation of the probabilities in eqn. (4.15) must account for either possible sign:

tmp3AC577_thumb

For the second integral, due to dV being negative, the original integral would have been overtmp3AC578_thumbwhich is equivalent to the integral in the expression above after interchanging the limits of integration and multiplying the integral by —1. The above integral relationships are equivalent to

tmp3AC580_thumb

which can be rewritten as

tmp3AC581_thumb

Issues related to the transformation of random variables are clarified by the following examples.

Example 4.4 Find the density for y wheretmp3AC582_thumb tmp3AC583_thumb

In this case,

tmp3AC586_thumb

Therefore,

tmp3AC587_thumb

 

 

 

 

Graph ofwith variables defined for Example 4.5.

Figure 4.3: Graph oftmp3AC589_thumbwith variables defined for Example 4.5.

Note thattmp3AC591_thumbhas the form of a Gaussian distribution with mean b and variancetmp3AC592_thumbtherefore, y is a Gaussian random variable. In general, all linear operations on Gaussian random variables result in Gaussian random variables.

Example 4.5 Find the density for y wheretmp3AC593_thumb

Because the function g is not invertible, the result of eqn. (4.16) cannot be used. Instead, we have to revert to the main idea of eqn. (4.15) which is that the change of variable must preserve the probability of events. Consider the variables defined in Figure 4.3. For this problem, we have

tmp3AC598_thumb

where dY represents a positive differential change fromtmp3AC599_thumband

tmp3AC602_thumb

The above expression translates into the following integral

tmp3AC603_thumb

Using the changes of variables this integral simplifies as followstmp3AC604_thumb

tmp3AC606_thumb

This integral relationship must hold for all nonnegativetmp3AC607_thumband arbitrarily small dY. In addition, fortmp3AC608_thumbwe havetmp3AC609_thumbtherefore,

tmp3AC613_thumb

This density does not have the form of eqn. (4.14); therefore, y is not a Gaussian random variable. In general, nonlinear transformations of Gaussian random variables do not result in Gaussian random variables.

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