Fama-French

The Fama-French model is an asset pricing model introduced by Eugene Fama and Kenneth French in the early 1990s. It expands upon the traditional Capital Asset Pricing Model (CAPM) by incorporating size and value factors to explain stock returns better. The model is based on three key factors:

  1. Market Risk (Beta): This measures the sensitivity of a stock's returns to the overall market returns.
  2. Size (SMB): This is the "Small Minus Big" factor, representing the excess returns of small-cap stocks over large-cap stocks.
  3. Value (HML): This is the "High Minus Low" factor, capturing the excess returns of value stocks (those with high book-to-market ratios) over growth stocks (with low book-to-market ratios).

The Fama-French three-factor model can be represented mathematically as:

Ri=Rf+βi(RmRf)+siSMB+hiHML+ϵiR_i = R_f + \beta_i (R_m - R_f) + s_i \cdot SMB + h_i \cdot HML + \epsilon_i

where RiR_i is the expected return on asset ii, RfR_f is the risk-free rate, RmR_m is the return on the market portfolio, and ϵi\epsilon_i is the error term. This model has been widely adopted in finance for asset management and portfolio evaluation due to its improved explanatory power over

Other related terms

Fluctuation Theorem

The Fluctuation Theorem is a fundamental result in nonequilibrium statistical mechanics that describes the probability of observing fluctuations in the entropy production of a system far from equilibrium. It states that the probability of observing a certain amount of entropy production SS over a given time tt is related to the probability of observing a negative amount of entropy production, S-S. Mathematically, this can be expressed as:

P(S,t)P(S,t)=eSkB\frac{P(S, t)}{P(-S, t)} = e^{\frac{S}{k_B}}

where P(S,t)P(S, t) and P(S,t)P(-S, t) are the probabilities of observing the respective entropy productions, and kBk_B is the Boltzmann constant. This theorem highlights the asymmetry in the entropy production process and shows that while fluctuations can lead to temporary decreases in entropy, such occurrences are statistically rare. The Fluctuation Theorem is crucial for understanding the thermodynamic behavior of small systems, where classical thermodynamics may fail to apply.

Cournot Competition Reaction Function

The Cournot Competition Reaction Function is a fundamental concept in oligopoly theory that describes how firms in a market adjust their output levels in response to the output choices of their competitors. In a Cournot competition model, each firm decides how much to produce based on the expected production levels of other firms, leading to a Nash equilibrium where no firm has an incentive to unilaterally change its production. The reaction function of a firm can be mathematically expressed as:

qi=Ri(qi)q_i = R_i(q_{-i})

where qiq_i is the quantity produced by firm ii, and qiq_{-i} represents the total output produced by all other firms. The reaction function illustrates the interdependence of firms' decisions; if one firm increases its output, the others must adjust their production strategies to maximize their profits. The intersection of the reaction functions of all firms in the market determines the equilibrium quantities produced by each firm, showcasing the strategic nature of their interactions.

Stochastic Differential Equation Models

Stochastic Differential Equation (SDE) models are mathematical frameworks that describe the behavior of systems influenced by random processes. These models extend traditional differential equations by incorporating stochastic processes, allowing for the representation of uncertainty and noise in a system’s dynamics. An SDE typically takes the form:

dXt=μ(Xt,t)dt+σ(Xt,t)dWtdX_t = \mu(X_t, t) dt + \sigma(X_t, t) dW_t

where XtX_t is the state variable, μ(Xt,t)\mu(X_t, t) represents the deterministic trend, σ(Xt,t)\sigma(X_t, t) is the volatility term, and dWtdW_t denotes a Wiener process, which captures the stochastic aspect. SDEs are widely used in various fields, including finance for modeling stock prices and interest rates, in physics for particle movement, and in biology for population dynamics. By solving SDEs, researchers can gain insights into the expected behavior of complex systems over time, while accounting for inherent uncertainties.

Kalman Smoothers

Kalman Smoothers are advanced statistical algorithms used for estimating the states of a dynamic system over time, particularly when dealing with noisy observations. Unlike the basic Kalman Filter, which provides estimates based solely on past and current observations, Kalman Smoothers utilize future observations to refine these estimates. This results in a more accurate understanding of the system's states at any given time. The smoother operates by first applying the Kalman Filter to generate estimates and then adjusting these estimates by considering the entire observation sequence. Mathematically, this process can be expressed through the use of state transition models and measurement equations, allowing for optimal estimation in the presence of uncertainty. In practice, Kalman Smoothers are widely applied in fields such as robotics, economics, and signal processing, where accurate state estimation is crucial.

Heap Allocation

Heap allocation is a memory management technique used in programming to dynamically allocate memory at runtime. Unlike stack allocation, where memory is allocated in a last-in, first-out manner, heap allocation allows for more flexible memory usage, as it can allocate large blocks of memory that may not be contiguous. When a program requests memory from the heap, it uses functions like malloc in C or new in C++, which return a pointer to the allocated memory block. This block remains allocated until it is explicitly freed by the programmer using functions like free in C or delete in C++. However, improper management of heap memory can lead to issues such as memory leaks, where allocated memory is not released, causing the program to consume more resources over time. Thus, it is crucial to ensure that every allocation has a corresponding deallocation to maintain optimal performance and resource utilization.

Zeta Function Zeros

The zeta function zeros refer to the points in the complex plane where the Riemann zeta function, denoted as ζ(s)\zeta(s), equals zero. The Riemann zeta function is defined for complex numbers s=σ+its = \sigma + it and is crucial in number theory, particularly in understanding the distribution of prime numbers. The famous Riemann Hypothesis posits that all nontrivial zeros of the zeta function lie on the critical line where the real part σ=12\sigma = \frac{1}{2}. This hypothesis remains one of the most important unsolved problems in mathematics and has profound implications for number theory and the distribution of primes. The nontrivial zeros, which are distinct from the "trivial" zeros at negative even integers, are of particular interest for their connection to prime number distribution through the explicit formulas in analytic number theory.

Let's get started

Start your personalized study experience with acemate today. Sign up for free and find summaries and mock exams for your university.