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Financial Risk Manager (FRM) Quantitative Analysis Syllabus
The Quantitative Analysis syllabus for Financial Risk Manager (FRM) in full: 6 chapters, 21 topics and 24 sub-topics, every one listed below, plus 51 Quantitative Analysis flashcards with answers.
Quantitative Analysis syllabus: all 6 chapters
Expand any chapter to see its topics and sub-topics.
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Probability and Random Variables
3 topics- Probability fundamentals
- Conditional and unconditional probability and Bayes' rule
- Independent versus mutually exclusive events
- Random variables and probability functions
- PMF, PDF, and cumulative distribution functions
- Quantiles and the inverse CDF
- Expectations and moments
- Mean, variance, skewness, and kurtosis
- Covariance, correlation, and coskewness
- Probability fundamentals
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Common Probability Distributions
4 topics- Discrete distributions: Bernoulli, binomial, and Poisson
- Continuous distributions: uniform, normal, and lognormal
- Fat-tailed and sampling distributions
- Student's t, chi-squared, and F distributions
- Mixture distributions and tail behavior
- The Central Limit Theorem and the law of large numbers
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Statistical Inference and Hypothesis Testing
3 topics- Sampling, estimators, and their properties
- Bias, efficiency, and consistency
- Standard error and confidence intervals
- Hypothesis testing framework
- Null and alternative hypotheses, Type I and Type II errors
- Test statistics, p-values, and significance levels
- One-tailed versus two-tailed tests
- Maximum likelihood estimation and method of moments
- Sampling, estimators, and their properties
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Regression Analysis
4 topics- Linear regression with one regressor
- OLS estimation and interpretation of coefficients
- R-squared, standard error of regression, and goodness of fit
- Multiple regression and the OLS assumptions
- Regression diagnostics
- Heteroskedasticity and serial correlation
- Multicollinearity and omitted-variable bias
- Hypothesis tests on coefficients and the F-test
- Linear regression with one regressor
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Time Series Analysis and Volatility Modeling
4 topics- Stationarity, autocorrelation, and white noise
- AR, MA, and ARMA models
- Model identification and forecasting
- Unit roots and random walks
- Volatility estimation
- Exponentially weighted moving average (EWMA)
- GARCH(1,1) and volatility clustering
- Correlation, copulas, and dependence modeling
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Simulation and Numerical Methods
3 topics- Monte Carlo simulation
- Generating random draws and inverse transform sampling
- Estimating standard errors of simulated quantities
- Variance reduction techniques
- Antithetic variates and control variates
- Bootstrapping and resampling methods
- Monte Carlo simulation
Financial Risk Manager (FRM) Quantitative Analysis flashcards — 51 questions with answers
State the three axioms of probability for events in a sample space.
For any event $A$: $P(A) \geq 0$. The probability of the entire sample space is $P(\Omega) = 1$. For mutually exclusive events $A_1, A_2, \ldots$, $P\left(\bigcup_i A_i\right) = \sum_i P(A_i)$.
Write the definition of conditional probability and Bayes' theorem.
Conditional probability: $P(A \mid B) = \dfrac{P(A \cap B)}{P(B)}$ for $P(B) > 0$. Bayes' theorem: $P(A \mid B) = \dfrac{P(B \mid A)\,P(A)}{P(B)}$.
What does it mean for two events $A$ and $B$ to be independent, and how does it simplify the joint probability?
Independence means the occurrence of one does not affect the other: $P(A \mid B) = P(A)$. Then the joint probability factors as $P(A \cap B) = P(A)\,P(B)$.
State the total probability rule for an event $A$ given a partition $\{B_i\}$.
$$P(A) = \sum_{i} P(A \mid B_i)\,P(B_i),$$ where the events $B_i$ are mutually exclusive and exhaustive.
Distinguish a discrete random variable from a continuous random variable.
A discrete random variable takes a countable set of values, described by a probability mass function (PMF) where $P(X = x) > 0$. A continuous random variable takes values on an interval, described by a probability density function (PDF) where $P(X = x) = 0$ and probabilities come from integrating the PDF.
Define the cumulative distribution function (CDF) and list its key properties.
$F(x) = P(X \leq x)$. It is non-decreasing, right-continuous, with $\lim_{x \to -\infty} F(x) = 0$ and $\lim_{x \to +\infty} F(x) = 1$. For a continuous variable, $f(x) = \dfrac{dF(x)}{dx}$.
Define the expected value of a discrete and a continuous random variable.
Discrete: $E[X] = \sum_i x_i\,P(X = x_i)$. Continuous: $E[X] = \int_{-\infty}^{\infty} x\,f(x)\,dx$.
Give the two equivalent formulas for the variance of a random variable.
$$\operatorname{Var}(X) = E\big[(X - E[X])^{2}\big] = E[X^{2}] - \big(E[X]\big)^{2}.$$
How do linear transformations affect the mean and variance? Give $E[aX+b]$ and $\operatorname{Var}(aX+b)$.
$E[aX + b] = aE[X] + b$ and $\operatorname{Var}(aX + b) = a^{2}\operatorname{Var}(X)$. Adding a constant shifts the mean but not the variance.
Define skewness and kurtosis, and state the kurtosis of a normal distribution.
Skewness is the standardized third moment $\dfrac{E[(X-\mu)^{3}]}{\sigma^{3}}$, measuring asymmetry. Kurtosis is the standardized fourth moment $\dfrac{E[(X-\mu)^{4}]}{\sigma^{4}}$, measuring tail heaviness. The normal distribution has kurtosis $= 3$; excess kurtosis $=$ kurtosis $- 3$.
For the covariance of two random variables, give the definition and the variance of a sum $X + Y$.
$\operatorname{Cov}(X, Y) = E[(X - \mu_X)(Y - \mu_Y)] = E[XY] - E[X]E[Y]$. Then $\operatorname{Var}(X + Y) = \operatorname{Var}(X) + \operatorname{Var}(Y) + 2\operatorname{Cov}(X, Y)$.
Describe a Bernoulli random variable and give its mean and variance.
A Bernoulli variable takes value $1$ (success) with probability $p$ and $0$ (failure) with probability $1-p$. Mean $E[X] = p$; variance $\operatorname{Var}(X) = p(1-p)$.
State the PMF, mean, and variance of a binomial random variable.
$P(X = k) = \binom{n}{k} p^{k}(1-p)^{n-k}$ for $k = 0,1,\ldots,n$. Mean $= np$; variance $= np(1-p)$. It counts successes in $n$ independent Bernoulli trials.
State the PMF, mean, and variance of a Poisson random variable.
$P(X = k) = \dfrac{\lambda^{k} e^{-\lambda}}{k!}$ for $k = 0,1,2,\ldots$. Both the mean and the variance equal $\lambda$. It models the number of events in a fixed interval given an average rate $\lambda$.
When can the Poisson distribution approximate the binomial distribution?
When $n$ is large and $p$ is small, the binomial is well approximated by a Poisson with $\lambda = np$. The Poisson is the limiting case of the binomial as $n \to \infty$ and $p \to 0$ with $np$ held constant.
Give the PDF, mean, and variance of a continuous uniform distribution on $[a, b]$.
$f(x) = \dfrac{1}{b - a}$ for $a \leq x \leq b$. Mean $= \dfrac{a + b}{2}$; variance $= \dfrac{(b - a)^{2}}{12}$.
Write the PDF of the normal distribution and state its key shape properties.
$$f(x) = \frac{1}{\sigma\sqrt{2\pi}}\exp\!\left(-\frac{(x - \mu)^{2}}{2\sigma^{2}}\right).$$ It is symmetric and bell-shaped, fully described by $\mu$ and $\sigma^{2}$, with skewness $0$ and kurtosis $3$.
How do you standardize a normal random variable, and what fraction of observations lie within $\pm 1.96\sigma$?
Standardize via $Z = \dfrac{X - \mu}{\sigma} \sim N(0,1)$. About $95\%$ of observations lie within $\mu \pm 1.96\sigma$ (and roughly $99\%$ within $\pm 2.58\sigma$).
Define the lognormal distribution and explain why it is used for asset prices.
If $\ln(X) \sim N(\mu, \sigma^{2})$, then $X$ is lognormal. It is right-skewed and bounded below by zero, making it suitable for asset prices and other variables that cannot be negative.
What characterizes a fat-tailed (leptokurtic) distribution relative to the normal?
A fat-tailed distribution has excess kurtosis $> 3$ (positive excess kurtosis), meaning more probability mass in the tails and a higher peak. Extreme outcomes are more likely than the normal would predict, which is important for risk modeling.
Show the other 31 Quantitative Analysis flashcards
Describe the Student's t-distribution and how it relates to the normal as degrees of freedom increase.
The Student's t is symmetric and bell-shaped but has fatter tails than the normal, controlled by degrees of freedom $\nu$. Its variance is $\dfrac{\nu}{\nu - 2}$ for $\nu > 2$. As $\nu \to \infty$, the t-distribution converges to the standard normal.
State the Central Limit Theorem.
For i.i.d. random variables with mean $\mu$ and finite variance $\sigma^{2}$, the sample mean's distribution approaches normal as $n$ grows: $$\frac{\bar{X} - \mu}{\sigma / \sqrt{n}} \xrightarrow{d} N(0, 1).$$ This holds regardless of the underlying distribution's shape.
State the law of large numbers and contrast it with the CLT.
The (weak) law of large numbers states the sample mean converges in probability to the population mean: $\bar{X} \xrightarrow{p} \mu$ as $n \to \infty$. The LLN concerns convergence of the mean to a constant, whereas the CLT describes the distributional shape (normality) of the standardized mean.
What is the standard error of the sample mean, and how does it scale with sample size?
$\text{SE}(\bar{X}) = \dfrac{\sigma}{\sqrt{n}}$ (estimated as $\dfrac{s}{\sqrt{n}}$). It decreases proportionally to $\dfrac{1}{\sqrt{n}}$, so quadrupling the sample size halves the standard error.
Define an unbiased estimator and give the bias formula.
An estimator $\hat{\theta}$ is unbiased if $E[\hat{\theta}] = \theta$. Bias is $E[\hat{\theta}] - \theta$; an unbiased estimator has zero bias. The sample mean is an unbiased estimator of the population mean.
List the desirable properties of an estimator: efficiency, consistency, and BLUE.
Efficiency: smallest variance among unbiased estimators. Consistency: $\hat{\theta} \xrightarrow{p} \theta$ as $n \to \infty$. Linearity. BLUE = Best Linear Unbiased Estimator, the minimum-variance unbiased estimator within the class of linear estimators (per Gauss-Markov).
Why is the sample variance divided by $n - 1$ rather than $n$?
Dividing by $n - 1$ (Bessel's correction) makes the sample variance an unbiased estimator of the population variance: $s^{2} = \dfrac{1}{n-1}\sum_{i=1}^{n}(X_i - \bar{X})^{2}$. Dividing by $n$ would systematically underestimate $\sigma^{2}$.
Outline the steps of the hypothesis testing framework.
State the null $H_0$ and alternative $H_1$; choose a significance level $\alpha$; compute a test statistic; determine the critical value(s) / rejection region or the p-value; reject $H_0$ if the statistic falls in the rejection region (or $p < \alpha$), otherwise fail to reject.
Distinguish Type I and Type II errors and define the power of a test.
Type I error: rejecting a true $H_0$, with probability $\alpha$ (the significance level). Type II error: failing to reject a false $H_0$, with probability $\beta$. Power $= 1 - \beta$, the probability of correctly rejecting a false null.
What is a p-value, and how is it used in a decision rule?
The p-value is the probability of obtaining a test statistic at least as extreme as the observed one, assuming $H_0$ is true. Reject $H_0$ if the p-value $< \alpha$; a smaller p-value indicates stronger evidence against the null.
Contrast a one-tailed and a two-tailed hypothesis test.
A two-tailed test ($H_1: \theta \neq \theta_0$) splits $\alpha$ between both tails and detects deviations in either direction. A one-tailed test ($H_1: \theta > \theta_0$ or $\theta < \theta_0$) places all of $\alpha$ in one tail and detects deviation in only the specified direction.
Describe maximum likelihood estimation (MLE).
MLE chooses parameter values that maximize the likelihood function $L(\theta) = \prod_i f(x_i; \theta)$ (or equivalently the log-likelihood $\ell(\theta) = \sum_i \ln f(x_i; \theta)$). The MLE is the parameter set that makes the observed data most probable; it is consistent and asymptotically efficient and normal.
Describe the method of moments estimation procedure.
The method of moments equates population (theoretical) moments to their corresponding sample moments and solves for the parameters. For example, set the population mean equal to the sample mean and the population variance equal to the sample variance, then solve.
Write the population simple linear regression model and identify each term.
$$Y_i = \beta_0 + \beta_1 X_i + \varepsilon_i,$$ where $\beta_0$ is the intercept, $\beta_1$ is the slope, $X_i$ is the regressor, $\varepsilon_i$ is the error term, and $Y_i$ is the dependent variable.
Give the OLS estimator of the slope $\hat{\beta}_1$ in simple regression.
$$\hat{\beta}_1 = \frac{\operatorname{Cov}(X, Y)}{\operatorname{Var}(X)} = \frac{\sum_{i}(X_i - \bar{X})(Y_i - \bar{Y})}{\sum_{i}(X_i - \bar{X})^{2}}.$$ The intercept is $\hat{\beta}_0 = \bar{Y} - \hat{\beta}_1 \bar{X}$.
What does OLS minimize, and what is the residual?
OLS minimizes the sum of squared residuals $\sum_i \hat{\varepsilon}_i^{2} = \sum_i (Y_i - \hat{Y}_i)^{2}$. The residual is $\hat{\varepsilon}_i = Y_i - \hat{Y}_i$, the difference between the observed and the fitted value.
Define $R^{2}$ and explain what it measures.
$R^{2} = \dfrac{\text{ESS}}{\text{TSS}} = 1 - \dfrac{\text{SSR}}{\text{TSS}}$, the fraction of total variation in $Y$ explained by the regression. It ranges from $0$ to $1$; higher values indicate a better in-sample fit.
Write the multiple regression model and explain how slope coefficients are interpreted.
$$Y_i = \beta_0 + \beta_1 X_{1i} + \beta_2 X_{2i} + \cdots + \beta_k X_{ki} + \varepsilon_i.$$ Each $\beta_j$ is the expected change in $Y$ for a one-unit increase in $X_j$, holding all other regressors constant (the partial/ceteris paribus effect).
List the key OLS (Gauss-Markov) assumptions for the classical linear regression model.
Linearity in parameters; the error has zero conditional mean $E[\varepsilon \mid X] = 0$; homoskedasticity (constant error variance); no autocorrelation of errors; no perfect multicollinearity among regressors. Under these, OLS is BLUE. Normality of errors is added for exact inference.
Why is adjusted $R^{2}$ preferred over $R^{2}$ in multiple regression?
$R^{2}$ never decreases when regressors are added, even useless ones. Adjusted $R^{2} = 1 - \dfrac{(1 - R^{2})(n - 1)}{n - k - 1}$ penalizes for the number of regressors $k$, so it can fall when an added variable does not improve fit enough to justify the lost degree of freedom.
Define multicollinearity and describe its consequences in OLS.
Multicollinearity is a high correlation among regressors. Perfect multicollinearity makes OLS estimates non-identifiable. Imperfect multicollinearity inflates coefficient standard errors, making individual coefficients statistically insignificant and unstable even when the overall regression fits well.
Define heteroskedasticity and explain its effect on OLS inference.
Heteroskedasticity is non-constant error variance, $\operatorname{Var}(\varepsilon_i \mid X) \neq \text{constant}$. OLS coefficients remain unbiased and consistent but are no longer efficient, and the usual standard errors are biased, invalidating t- and F-tests. Remedy: use robust (White) standard errors.
Explain omitted variable bias and the two conditions required for it.
Omitting a relevant variable biases the included coefficients if the omitted variable is both (1) a determinant of $Y$ and (2) correlated with an included regressor. This violates $E[\varepsilon \mid X] = 0$, making OLS biased and inconsistent.
How do you test the significance of a single regression coefficient?
Use a t-test: $t = \dfrac{\hat{\beta}_j - \beta_{j,0}}{\text{SE}(\hat{\beta}_j)}$, typically with $\beta_{j,0} = 0$. Compare $|t|$ to the critical value with $n - k - 1$ degrees of freedom (or check the p-value); reject if it exceeds the critical value.
What does the F-test assess in a multiple regression, and what is its null hypothesis?
The F-test assesses the joint significance of a group of (or all) slope coefficients. For overall significance the null is $H_0: \beta_1 = \beta_2 = \cdots = \beta_k = 0$. A large F-statistic relative to its critical value rejects the null that the regressors jointly have no explanatory power.
Define a stationary (covariance-stationary) time series.
A series is covariance-stationary if its mean, variance, and autocovariances are constant over time and the autocovariance depends only on the lag $h$, not on time $t$: $E[Y_t] = \mu$, $\operatorname{Var}(Y_t) = \sigma^{2}$, and $\operatorname{Cov}(Y_t, Y_{t-h}) = \gamma_h$.
Define white noise and autocorrelation.
White noise is a series of uncorrelated random variables with constant mean (usually zero) and constant variance, with no autocorrelation at any nonzero lag. Autocorrelation is the correlation of a series with its own lagged values: $\rho_h = \dfrac{\operatorname{Cov}(Y_t, Y_{t-h})}{\operatorname{Var}(Y_t)}$.
Write the AR(1) model and state its stationarity condition.
$$Y_t = c + \phi Y_{t-1} + \varepsilon_t,$$ where $\varepsilon_t$ is white noise. It is covariance-stationary if $|\phi| < 1$. Its unconditional mean is $\dfrac{c}{1 - \phi}$, and the autocorrelation function decays geometrically as $\phi^{h}$.
Write an MA(1) model and contrast MA and AR processes.
$$Y_t = \mu + \varepsilon_t + \theta\,\varepsilon_{t-1}.$$ An MA process expresses $Y_t$ as a finite linear combination of current and past white-noise shocks and always has finite memory (autocorrelations cut off after lag $q$). An AR process depends on past values of $Y$ and has infinite, geometrically decaying memory. An ARMA(p,q) combines both.
Compare the EWMA and GARCH(1,1) approaches to volatility estimation.
EWMA: $\sigma_t^{2} = \lambda\sigma_{t-1}^{2} + (1 - \lambda)r_{t-1}^{2}$, weighting recent returns more (no long-run mean). GARCH(1,1): $\sigma_t^{2} = \omega + \alpha r_{t-1}^{2} + \beta\sigma_{t-1}^{2}$, which adds a constant $\omega$ and mean-reverts to a long-run variance $\dfrac{\omega}{1 - \alpha - \beta}$ when $\alpha + \beta < 1$. EWMA is the special case with $\omega = 0$, $\alpha = 1-\lambda$, $\beta = \lambda$.
Define the Pearson correlation coefficient and contrast it with a copula's role in dependence modeling.
Pearson correlation $\rho_{X,Y} = \dfrac{\operatorname{Cov}(X, Y)}{\sigma_X \sigma_Y}$ measures only linear dependence and lies in $[-1, 1]$. A copula links marginal distributions into a joint distribution, capturing the full dependence structure (including nonlinear and tail dependence) separately from the marginals, per Sklar's theorem. This is important because correlation alone can miss joint extreme (tail) events.
Financial Risk Manager (FRM) Quantitative Analysis FAQ
What is in the Financial Risk Manager (FRM) Quantitative Analysis syllabus?
Financial Risk Manager (FRM) Quantitative Analysis is split into 6 chapters: Probability and Random Variables, Common Probability Distributions, Statistical Inference and Hypothesis Testing, Regression Analysis, Time Series Analysis and Volatility Modeling and Simulation and Numerical Methods. Together they contain 21 topics and 24 sub-topics.
How many chapters are in Financial Risk Manager (FRM) Quantitative Analysis?
6 chapters, containing 21 topics and 24 sub-topics. The largest chapter is Common Probability Distributions, with 4 topics.
Are there flashcards for Financial Risk Manager (FRM) Quantitative Analysis?
Yes — a 51-card Quantitative Analysis deck, printed in full in the flashcards section of this page and available in the Examius app with spaced repetition. The free plan covers one exam of your choice, including its flashcards; Examius Pro, a one-time purchase, unlocks every other exam and deck.