math concept
39 topics use this
Math concept
Differential Equations (ODEs)
Core equation
$$\frac{dy}{dt} = f(t, y)$$
Ordinary differential equations describe how quantities change continuously over time. They govern population dynamics, electrical circuits, chemical reactions, and mechanical systems. Existence, uniqueness, and stability are the central theoretical concerns.
First-order linear ODEs
\[\frac{dy}{dt} + p(t)y = q(t)\]Solved by the integrating factor $\mu(t) = e^{\int p(t)\,dt}$:
\[y = \frac{1}{\mu(t)}\left[\int \mu(t)q(t)\,dt + C\right]\]Second-order linear ODEs with constant coefficients
\[ay'' + by' + cy = f(t)\]The characteristic equation $ar^2 + br + c = 0$ determines solution structure:
- Two real roots $r_1 \neq r_2$: $y_h = C_1 e^{r_1 t} + C_2 e^{r_2 t}$
- Repeated root: $y_h = (C_1 + C_2 t)e^{rt}$
- Complex roots $\alpha \pm i\beta$: $y_h = e^{\alpha t}(C_1\cos\beta t + C_2\sin\beta t)$
Stability: Lyapunov’s method
For the system $\dot{\mathbf{x}} = f(\mathbf{x})$, an equilibrium $\mathbf{x}^*$ is stable if there exists a Lyapunov function $V(\mathbf{x}) > 0$ with $\dot{V}(\mathbf{x}) \leq 0$.
Fields that use this concept
Finance & economics
Actuarial science
Interest Rate Risk
The exposure of insurance liabilities and fixed-income assets to changes in interest rates, managed through duration, convexity, immunization, and asset-liability management techniques.
Ruin Theory
The mathematical study of when an insurer's surplus process first becomes negative, providing bounds and exact formulas for the probability of ruin under the classical Cramér-Lundberg model.
Survival Models in Actuarial Science
Probabilistic models for the future lifetime of individuals and groups, including joint life, multiple decrement, and copula-based dependent mortality models used in pension and life insurance valuation.
Physical sciences
Astrophysics
Friedmann Equations and Cosmology
The dynamical equations governing the expansion history of a homogeneous, isotropic universe derived from general relativity.
Gravitational Waves
Ripples in spacetime curvature propagating at the speed of light, produced by accelerating asymmetric mass distributions.
Hubble's Law and Cosmic Expansion
The empirical relationship between a galaxy's recession velocity and its distance, forming the foundation of observational cosmology.
Nucleosynthesis
The nuclear processes that forge every element from hydrogen to uranium inside stars, supernovae, and the Big Bang.
Stellar Evolution
The life cycle of stars from gravitational collapse through nuclear burning phases to their final compact remnants.
Stellar Structure Equations
The four coupled differential equations governing the interior structure of stars in hydrostatic equilibrium.
Earth sciences
Climate modeling
Carbon Cycle Modeling
Box models of carbon exchange between the atmosphere, ocean, and land biosphere, including feedback parameters that modulate the airborne fraction of emissions.
Energy Balance Models
Zero- and one-dimensional models of Earth's temperature from the balance between absorbed solar radiation and outgoing longwave emission.
Climate Feedbacks
The physical mechanisms by which an initial warming perturbation is amplified or damped, quantified through the feedback framework and linearized forcing-response relationships.
Ocean Circulation
The physical dynamics of large-scale ocean flow, from geostrophic balance and wind-driven gyres to the thermohaline circulation and ENSO variability.
Radiative Forcing
The change in Earth's energy budget caused by an external perturbation, measured in watts per square meter, and its role in attributing observed climate change.
Sea Ice Modeling
Thermodynamic and dynamic modeling of sea ice, including the Stefan freezing condition, viscous-plastic rheology, and Arctic decline under climate change.
Physical sciences
Computational chemistry
Born-Oppenheimer Approximation
The foundational separation of nuclear and electronic motion that underlies nearly all of computational chemistry.
Molecular Dynamics
Classical simulation of atomic motion by integrating Newton's equations with empirical force fields.
Molecular Mechanics
Classical force field models that treat atoms as point masses connected by springs to simulate large biomolecular systems.
Path Integral Molecular Dynamics
Feynman's imaginary-time path integral formulation extended to finite-temperature MD, capturing nuclear quantum effects such as tunnelling and zero-point energy.
Earth sciences
Geophysics
Earthquake Seismology
Moment tensors, seismic moment, and the Gutenberg-Richter law characterise earthquake sources and their statistical recurrence.
Seismic Waves
P and S waves, the elastic wave equation, and Snell's law govern how seismic energy travels through the Earth.
Earth sciences
Meteorology
Atmospheric Thermodynamics
The thermodynamic laws governing temperature, stability, and phase change in the atmosphere.
Atmospheric Boundary Layer
The turbulent lowest kilometre of the atmosphere that mediates exchanges of heat, moisture, and momentum between the surface and free troposphere.
Mesoscale Convection
The organisation of thunderstorms into mesoscale convective systems driven by CAPE, wind shear, and cold pool dynamics.
Tropical Cyclones
The dynamics of warm-core rotating vortices that form over tropical oceans and can reach devastating intensities.
Life sciences
Quant ecology
Age-Structured Population Models
Age-structured models use matrix algebra and eigenanalysis to project population dynamics when vital rates depend on age or stage class.
Island Biogeography
MacArthur and Wilson's equilibrium theory explains species richness on islands through the balance of immigration and extinction, predicting the species-area relationship.
Logistic Population Growth
The logistic equation models density-dependent population growth toward a carrying capacity, with rich extensions including chaos, Allee effects, and generalized forms.
Lotka-Volterra Equations
A foundational system of nonlinear ODEs describing predator-prey population dynamics and their oscillatory coexistence.
Metapopulation Dynamics
The Levins metapopulation model and its extensions describe how species persist as networks of local populations connected by dispersal.
SIR Epidemic Model
The SIR compartmental model partitions a population into Susceptible, Infected, and Recovered classes to describe epidemic spread through a basic system of ODEs.
Stochastic Population Dynamics
Demographic and environmental stochasticity drive population fluctuations and extinction risk in ways that deterministic models cannot capture.
Finance & economics
Quant finance
Bond Pricing & Duration
Valuing fixed-income securities and measuring their interest rate sensitivity. Duration and convexity are the core risk metrics.
Geometric Brownian Motion
The stochastic process driving the Black-Scholes model. Ensures prices stay positive and returns are log-normally distributed.
Interest Rate Models
Stochastic models for the yield curve. Used to price bonds, swaps, caps, and swaptions.
Stochastic Volatility
Models where volatility itself is random. The Heston model gives closed-form option prices and captures the implied volatility smile.
Engineering & CS
Robotics