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Reading 10 Common Probability Distributions

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1. INTRODUCTION TO COMMON PROBABILITY DISTRIBUTIONS

Probability distribution: A probability distribution describes the values of a random variable and the probability associated with these values.

Types of distribution:

1. Uniform 2. Binomial 3. Normal 4. Lognormal

2. DISCRETE RANDOM VARIABLES

Random variable: A variable that has uncertain future outcomes is called random variable. The two basic types of random variables are:

1)Discrete random variables: Discrete random variables have a countable number of outcomes i.e. all possible outcomes can be listed without missing any of them. For example, counts, dice, number of students, quoted price of a stock etc. A discrete random variable can take

• On a limited (finite) number of outcomes i.e. x1, x2,

…,xn.

• On an unlimited (infinite) number of outcomes i.e. y1,

y2, …

2)Continuous random variables: Continuous random variables have an infinite and uncountable range of possible outcomes; thus, we cannot list all possible outcomes. For example, time, weight, distance, rate of return etc. The range of possible outcomes of a continuous random variable is the real line i.e. between -∞ and +∞ or some subset of the real line.

Probability function: The probability function describes the probability of a specific value that the random variable can take.

For a discrete random variable, it is denoted as:

P(X = x)

read as the “probability that a random variable X takes on the value x.

where,

X represents the name of the random variable. x represents the value of the random variable.

Example:

Suppose, X = number of heads in 15 flips of a coin.

P(X = 5) = P (5) probability of 5 heads (x) in 15 flips of a coin.

• For a continuous random variable, the probability function is called the probability density function (pdf) and is denoted as f(x).

Properties of a probability function:

1) 0 ≤ P(x) ≤ 1, for all x.

2) The sum of the probabilities p(x) over all values of X = 1 i.e. ∑ = 1.

Cumulative distribution function or distribution function:

The cumulative distribution function describes the probability that a random variable X ≤ particular value x i.e. P(X ≤ x). For both discrete and continuous random variables, it is denoted as F(x) = P(X ≤ x).

F(x) = Sum of all the values of the probability function for all outcomes ≤ x.

Properties of Cumulative distribution function (cdf):

1) The cdf lies between 0 and 1 for any x i.e. 0 ≤ F(x) ≤ 1. 2)With an increase in x the cdf either increases or

remains constant.

For detailed understanding, please refer to Example given after Table 1, Reading 10, Volume 1.

2.1 The Discrete Uniform Distribution

It the simplest form of probability distribution.

• The discrete uniform distribution has a finite number of specified outcomes.

• The probability of each outcome in a discrete uniform distribution is equally likely.

2.2 The Binomial Distribution

A distribution that involves binary outcomes is referred to as binomial distribution. It has following properties:

1. A binomial distribution has fixed number of trials i.e. Practice: Example 1,

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n.

2. Each trial in a binomial distribution has two possible outcomes i.e. a “success” and a “failure”.

3. Probability of success is denoted as P (success) = p and Probability of failure is denoted as P (failure) =1– p → for all trials.

4. The trials are independent, which means that the outcome of one trial does not affect the outcomes of any other trials.

Assumptions of the binomial distribution:

a) The probability of success (i.e. p) is constant for all trials.

b) The trials are independent.

Bernoulli trial: A trial that generates one of two outcomes is called a Bernoulli trial.

• In a Bernoulli trial with n number of trials, we can have 0 to n successes.

• If the outcome of an individual trial is random, then the total number of successes in n trials is also random.

Binomial random variable X: It represents the number of successes in n Bernoulli trials i.e.

X = sum of Bernoulli random variables X = Y1 + Y2 + …+ Yn

where,

Yi = Outcome on the ith trial

• A binomial random variable is completely described by two parameters i.e. n and p. It is stated as X~ B (n, p) read as “X has a binomial distribution with parameters n and p”.

• Thus, a Bernoulli random variable is a binomial random variable with n = 1 i.e. Y~B (1, p).

Probability function of the Bernoulli random variable Y:

• When the outcome is success Y = 1. • When the outcome is failure Y = 0.

p (l) = P(Y= 1) = p = probability of success p (0) = P( Y = 0) = 1 – p = probability of failure

For example, a stock price is a Bernoulli random variable with probability of success (an up move) = p and probability of failure (a down move) = 1 – p.

Suppose, Stock price today = S.

• When the stock price increases, ending price = uS = (1 + rate of return if the stock moves up) × S

• When the stock price decreases, ending price = dS

1 1

One-Period Stock Price as a Bernoulli Random Variable

Source: Example 2, Volume 1, Reading 10.

Number of sequences in n trials that result in x up moves (or successes) and n – x down moves (or failures) is calculated as follows:

Probability function for a binomial random variable:

1

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Example:

If a coin is tossed 20 times, what is the probability of getting exactly 10 heads?

p = 0.50

Stock price movement on three consecutive days:

• Each day is an independent trial.

• When the stock moves up u = 1 + rate of return for an up move.

• When the stock moves down d = 1 + rate of return for a down move.

A binomial tree is shown below. Each boxed value that represents successive moves (branch in the tree) is called a node.

• In the fig below, a node reflects the potential value for the stock price at a specified time.

• At each node, the transition probability for an up move is p and for a down move is (1 – P).

• Each of the sequences uud, udu, and duu, has probability = p2 (l – p).

• Stock price after three moves = P (S3 = uudS) = 3p2 (l -

p).

e.g. Number of ways to get 2 up moves in three periods = 3! / (3 – 2)! 2! = 3

3.1 Continuous Uniform Distribution

The continuous uniform distribution is the simplest continuous probability distribution. The uniform distribution has two main uses.

• It plays an important role in Monte Carlo simulation. • It is an appropriate probability model to represent an

uncertainty in beliefs with equally likely outcomes.

Probability density function (pdf): It is used to assign the probabilities to a continuous random variable and is denoted as f (x). According to pdf,

• The probability that value of x lies between a and b is the area under the graph of f(x) that lies between a and b or the integral of f(x) over the range a to b.

• Elsewhere, density of the distribution of a random variable x = 0.

Finding probability: The probabilities can be estimated as follows:

! " # # "

• F (x) = area under the curve graphing the pdf.

• Under a Continuous uniform distribution, probabilities for values of a continuous random variable x are assigned across an interval of values of x; thus, the probability that x takes on a specific value = 0. • Since the probabilities at the endpoints a and b = 0

for any continuous random variable X, P (a ≤ X ≤ b) = P (a < X ≤ b) = P (a ≤ X< b) = P (a< X < b).

For a continuous uniform random variable:

Mean = µ = (a + b) / 2

Variance = σ2 = (b – a) 2 / 12

S.D. = √

• Note that S.D. is not a useful risk measure for a uniform distribution; rather, the S.D. is a good risk measure for Normal Distribution.

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Example:

Suppose,

At the lower bound = a =100,000 km total cost = $40,000.

At the upper bound = b =150,000 km total cost = $60,000.

Outside the lower and upper bound total cost = $0. x = total anticipated annual travel costs in thousands of

dollars

• Over the range of values from $40,000 to $60,000, the distribution has density f(x) = 1/ (60 - 40) = 1/20. • Elsewhere, the distribution has density f(x) = 0.

The probability that travel costs are between 40 and 60 = Total area under the density function f(x) between 40 and 60 = height × length (or base) = (1/20) × (60–40) = 1

The probability that travel costs are between 40 and 50 = Area under the curve between 40 & 50 = (1/20) × (50–40) = 0.50

3.2 The Normal Distribution

• A normal distribution is a distribution that is symmetric about the centre (mean) and is bell-shaped. Thus,

o Mean = median = mode.

o Skewness = 0.

o Kurtosis = 3 and Excess kurtosis = 0.

• The range of possible outcomes of the normal distribution is the entire real line i.e. all real numbers lying between -∞ and +∞.

• The tails of the normal distribution never touches the horizontal axis and extend without limit to the left and to the right; however, as we move away from the center, the tails get closer and closer to the horizontal axis. This characteristic is referred to as the distribution is asymptotic to the horizontal axis. • The normal distribution is described by two

parameters i.e. its mean (µ) and its variance (σ2) or

standard deviation (σ). It is stated as:

X ~ N (µ, σ2) read “X follows a normal distribution

with mean µ and variance σ2”.

o When the mean increases (decreases), the curve shifts to the right (left).

• When the standard deviation increases (decreases),

• The smaller the S.D., the more the observations are concentrated around the mean.

• Since the normal distribution is symmetrical, it tends to underestimate the probability of extreme returns. Thus, it is not appropriate to use for Options. • The normal distribution can be used to model

returns; however, is not appropriate to use to model asset prices.

• According to the central limit theorem, sum and mean of a large number of independent random variables is approximately normally distributed. • It is important to note that a linear combination of

two or more normal random variables is also normally distributed.

A univariate normal distribution describes the probability of a single random variable.

A multivariate normal distribution describes the

probabilities for a group of related random variables. It is completely defined by three parameters:

1. The list of the mean returns on the individual securities i.e. total means = n.

2. The list of the securities’ variances of return i.e. total variances = n.

3. The list of all the distinct pair-wise return correlations i.e. total distinct correlations = n (n - 1) / 2.

For example, a bivariate normal distribution (i.e. a distribution with 2 stocks) has:

• Means = 2 • Variances = 2

• Correlation = 2 (2 –1) / 2 = 1

For a normal random variable standard deviation of:

• Sample skewness = 6/ n • Sample kurtosis = 24/ n

Normal density function: It is expressed as follows:

= 1

%√2& '

−(−()

2% )for − ∞ << +∞

• The probability that a normally distributed variable x takes on values in the range from a to b = Area Practice: Example 7,

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• The total area under the curve = 1.

• The area under the curve to the left of centre = 0.5 and the area right of centre = 0.5.

o Approximately 50% of all observations fall in the

interval µ ± (2/ 3) σ.

o Approximately 68% of all observations fall in the

interval µ ± σ.

o Approximately 95% of all observations fall in the interval µ ± 2σ.

o Approximately 99% of all observations fall in the

interval µ ± 3σ.

• More-precise intervals are µ ± 1.96σ for 95% of the

observations and µ ± 2.58σ for 99% of the

observations.

Standard normal distribution or unit normal distribution: It is a normal distribution with:

• The mean (µ ) = 0

• Standard deviation (σ) =1

When X is normally distributed, it can be standardized using the following formula:

Z =

• Z –score indicates how many standard deviations away from the mean the point x lies.

Example:

Suppose, a normal random variable, X = 9.5 with µ = 5

and σ = 1.5.

Z = (9.5 - 5) / 1.5 = 3

Example:

Finding the Probability i.e. P (Z < 2.67). It is found by first finding 2.6 in the left hand column, and then moving across the row to the column under 0.07. (Refer to table on the next page). Thus,

The area to the left of z = 2.67 = 0.9962.

• In order to find the area to the right of z, we use the Standard Normal Table given below to find the area that corresponds to z-value and then subtract the area from 1.

• Probability to the right of x = 1.0 - N(x).

• Since the normal distribution is symmetric around its mean, the area and the probability to the right of x = area and the probability to the left of -x, N (-x). • The probability to the right of –x i.e. P (Z ≥ -x) = N(x).

Example:

• Finding P (Z > 1.23):

• Finding P (-0.75 < Z < 1.23):

• Finding P (Z< -2.33):

Example:

The average (µ) on a corporate finance test was 78 with

a standard deviation of 8 (σ). If the test scores are

normally distributed, find the probability that a student receives a test score greater than 85.

Z =

= 0.875 ≈ 0.88

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NOTE:

• P (Z ≤ 1.282) = 0.90 = 90% → It implies that 90th

percentile point = 1.282 and % of values in the right tail = 10%.

• P (Z ≤ 1.65) = 0.95 = 95% → It implies that the 95th

percentile point = 1.65 and % of values in the right tail = 5%.

• P (Z ≤ 2.327) = 0.99 = 99% → It implies that the 99th

percentile point = 2.327 and % of values in the right tail = 1%.

3.3 Applications of the Normal Distribution

• The mean-variance analysis is based on the assumption that returns are normally distributed. • Safety-first rule: Safety-first rule focuses on shortfall

risk i.e. the risk that portfolio value will fall below some minimum acceptable level over some specified time horizon. For example, the risk that the assets in a defined benefit plan will fall below plan liabilities.

According to Roy's safety-first criterion, the optimal portfolio is the one that minimizes the probability that portfolio return (Rp) falls below the threshold level (RL).

When returns are normally distributed, the safety-first optimal portfolio is the portfolio that maximizes the safety-first ratio (SFRatio):

!*=+,*−*-/%

• Investors prefer the portfolio with the highest SFRatio. • Probability that the portfolio return < threshold level =

P (Rp< RL) = N (-SFRatio).

• The optimal portfolio has the lowest P (Rp< RL).

Example:

• Portfolio 1 expected return = 12% and S.D. = 15% • Portfolio 2 expected return = 14% and S.D. = 16% • Threshold level = 2%

• Assumes that returns are normally distributed.

SFRatio of portfolio 1 = (12 – 2) / 15 = 0.667 SFRatio of portfolio 2 = (14 – 2) / 16 = 0.75

• Since SFRatio of portfolio 2 > SFRatio 1, the superior Portfolio is Portfolio 2.

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Probability that return < 2% = N (–0.75) = 1 – N (0.75) = 1 – 0.7734* ≈ 23%. *Refer to table on previous page.

Sharpe Ratio:

Sharpe ratio = [E (Rp) – Rf] / σp

• The portfolio with the highest Sharpe ratio is the one that minimizes the probability that portfolio return will be less than the risk-free rate (assuming returns are normally distributed).

Managing Financial risk: Two important measures used to manage financial risk include:

•Value at risk (VAR): It provides the minimum value of losses (in money terms) expected over a specified time period (e.g. a day, quarter, year etc.) at a specified level of probability (e.g. 5%, 1%). VAR estimated using variance-covariance or analytical method assumes that returns are normally

distributed. Example:

A one week VAR of $10 million for a portfolio with 5% probability implies that portfolio is expected to loss $10 million or more in a single week.

•Stress testing/scenario analysis: It involves a use of set of techniques to estimate losses in extremely worst combinations of events or scenarios.

3.4 The Lognormal Distribution

A random variable (i.e. Y) whose natural logarithm (i.e. ln Y) has a normal distribution, is said to have a Lognormal distribution.

•Unlike Normal distribution, Lognormal random

variables cannot be negative.

Reason:

Since, negative values do not have logarithms, Y is always > 0 and thus the distribution is positively skewed (unlike normal distribution that is bell-shaped).

• Like normal distribution, it is completely described by two parameters i.e. the mean and variance of In Y,

given that Y is lognormal.

Mean (µL) of a lognormal random variable =

exp (µ + 0.50σ2)

Variance (σL2) of a lognormal random variable

= exp (2µ+ σ2) × [exp (σ2) – 1].

Strengths of lognormal distribution:

• The lognormal distribution is more appropriate

(relative to normal distribution) to use to model asset prices because asset prices cannot be negative.

• It is used in Black-Scholes-Merton model, which assumes that the asset’s price underlying the option is lognormally distributed.

It is important to note that when a stock's continuously compounded return is normally distributed, then future stock price is necessarily lognormally distributed.

ST = S0exp (r0,T)

Where, exp = e

r0,t = Continuously compounded return from 0 to T

• Since ST is proportional to the log of a normal

random variable → ST is lognormal.

Price relative = Ending price / Beginning price = St+1/ St=1 + Rt, t+1

where,

Rt, t+1 = holding period return on the stock from t to t + 1.

Continuously compounded return associated with a holding period from t to t + 1:

rt, t+1= ln(1 + holding period return)

Or

rt, t+1 = ln(price relative) = ln (St+1 / St) = ln (1 + Rt,t+1)

NOTE:

The continuously compounded return < associated holding period return.

Continuously compounded return associated with a holding period from 0 to T:

R0,T= ln (ST / S0)

Or

,=,+,+ ⋯ +,

Where,

rT-I, T = One-period continuously compounded returns

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Example:

Suppose, one-week holding period return = 0.04.

Equivalent continuously compounded return =

one-week continuously compounded return = ln (1.04) = 0.039221

• The intervals within which a certain percentage of the observations of a normally distributed random variable are expected to lie are symmetric around the mean.

• The intervals within which a certain percentage of the observations of a lognormally distributed random variable are expected to lie are not symmetric around the mean.

In many investment applications, it is assumed that returns are independently and identically distributed (IID).

• Returns are independently distributed implies that investors cannot forecast future returns using past returns (i.e., weak-form market efficiency). • Returns are identically distributed implies that the

mean and variance of return do not change from period to period (i.e. stationarity).

When one-period continuously compounded returns (i.e. r0,1) are IID random variables with mean µ and variance

• It implies that when the one-period continuously compounded returns are normally distributed, then the T holding period continuously compounded return (i.e. r0,T) is also normally distributed with mean

µT and variance σ2T.

• According to Central limit theorem, the sum of one-period continuously compounded returns is

approximately normal even if they are not normally distributed.

Volatility:

Volatility reflects the deviation of the continuously compounded returns on the underlying asset around its mean. It is estimated using a historical series of

continuously compounded daily returns.

Annualized volatility = sample S.D. of one period

continuously compounded returns × √0

where,

T = Number of trading days in a year = 250.

Example:

Michelin Daily Closing Prices

Date (2003) Closing Price (€)

Annualized volatility = 0.010354 × √250 = 0.163711

Expected continuously compounded annual return = Sample mean × T

= 0.009156 (250) = 2.289

Source: Example 10, Volume 1, Reading 10.

4. MONTE CARLO SIMULATION

Monte Carlo simulation involves the use of a computer

to generate a large number of random samples from a

probability distribution. It can be used in conjunction

with (i.e. as a complement) analytical methods.

Uses:

•It is used in planning and managing financial risk. •It can be used in valuing complex securities e.g.

• It can be used to estimate VAR e.g. using Monte Carlo simulation, portfolio's profit and loss performance for a specified time horizon are simulated to generate a frequency distribution for changes in portfolio value; the point that reflects the end point of the least favorable 5% of simulated changes is 95% VAR.

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Advantages:Monte Carlo simulation can be used to value complex securities i.e. European-style options.

Drawbacks: Unlike analytical methods (e.g. Black-Scholes-Merton option pricing model), Monte Carlo simulation provides only statistical estimates, not exact results. In addition, unlike black-scholes model, Monte Carlo simulation model cannot be used to quickly measure the sensitivity of call option value to changes in current stock price and other variables.

Steps of Monte Carlo simulation technique to examine a model's sensitivity to changes in assumptions:

1) Specify the underlying variable or variables e.g. stock price for an equity call option.

2) Specify the beginning values of the underlying

variables e.g. stock price.

• C iT = Value of the option at maturity T. The subscript I

reflects a value resulting from the ith simulation trial.

3) Specify a time period.

Time increment = ∆t

= Calendar time / Number of sub-periods (K)

4) Specify the regression model for changes in stock

price.

∆ ( ∆ %

3

where,

Zk= Risk factor in the simulation. It is a standard normal random variable.

5) K random variables are drawn for each risk factor

using a computer program or spreadsheet function.

6) Now the underlying variables are estimated by

substituting values of random observations in the model specified in Step 4.

7) The value of a call option at maturity i.e. CiT is

calculated and then this value is discounted back at time period 0 to get Ci0.

8) This process is repeated until a specified number of trials, i, is completed (e.g. tens of thousands of trials).

NOTE:

For obtaining each extra digit of accuracy in results, the appropriate increase in the number of trials depends on the problem. For example, in option value, tens of thousands of trials may be appropriate. Generally, the number of trials should be increased by a factor of 100.

9) Finally, mean value and S.D. for the simulation are calculated.

Mean value = Average value of the option over all trials in the simulation

• The mean value will be the Monte Carlo estimate of the value of the call option.

Random number generator: An algorithm that generates

uniformly distributed random numbers between 0 and 1 is referred to as random number generator. It is

important to note that random observations from any distribution can be generated using a uniform random variable.

Steps to generate random observations on variable X:

1)Generate a uniform random number (i.e. T) between

0 and 1 using the random number generator.

2)Evaluate the inverse of cumulative distribution

function F(x) i.e. F-1 (x) to obtain a random

observation on variable X.

Historical simulation or Back simulation: Under a

historical simulation, samples are generated using a historical record of underlying variables to simulate a process. It is based on the assumption that historical data can be used to predict future.

Drawback of Historical simulation: Unlike Monte Carlo simulation, historical simulation cannot be used to perform “what if” analyses.

Referensi

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