Mathematics for Undergraduate Physics

Maintained UY1 mathematical methods module surface: recommended core sequence, optional extensions, and notes-first assessment bridges into active UY1 module practice.

  • University Physics Year 1
  • 14 lessons

Before you begin

These lessons build the mathematical methods for first-year physics. The aim is to pick the right tool quickly: gradients for field problems, differential equations for dynamics and transients, and complex numbers for phase and A.C. systems.

Learning goals
  • Use complex numbers, linear algebra, and differential equations to solve coupled physical models.
  • Use vector and differential or integral calculus to express physical change and accumulation.
  • Choose an efficient mathematical method and validate the result physically.

Lessons

Work through them in order.

  1. Complex Numbers (Euler’s Formula and Phasors)Use complex numbers for phasors and amplitude–phase algebra.
  2. Differentiation TechniquesDifferentiate fluently, including the chain rule.
  3. Integration TechniquesChoose and apply the main integration methods.
  4. Integration without integrationUse a shortcut for repeated trigonometric–exponential integrals.
  5. Partial Derivatives (Multivariable Calculus)Differentiate functions of several variables for gradients and Jacobians.
  6. Bernoulli Differential EquationsReduce a nonlinear Bernoulli equation to a linear one.
  7. Basics of Second-Order Differential EquationsSolve constant-coefficient second-order equations from the characteristic equation, with and without forcing.
  8. First Order Differential EquationsSolve first-order equations for RC, drag and relaxation models.
  9. First-Order Linear Differential EquationsSolve first-order linear equations with an integrating factor.Supporting
  10. Second-Order Differential EquationsSolve second-order equations for oscillating systems.
  11. Steps for Solving First-Order Differential EquationsFollow a standard procedure for solving first-order equations.Supporting
  12. Separable Differential EquationsSolve separable equations by direct integration.
  13. Vector Calculus (Integral Theorems)Use Gauss's and Stokes's theorems for field integrals.
  14. Matrices and Linear Algebra (Physics Basics)Use matrices and eigenvalues for coupled systems.

Practise and check

Topic reference

Quick references

Method-selection checkpoint

Choose a method before opening the answer. For each prompt, state the mathematical tool, the physical reason it fits, and one check you would make on the result.

  1. A cooling model obeys dT/dt = -k(T-Tᵣₒₒₘ). You need T(t) from an initial temperature.
  2. A spherically symmetric electric field is known on a closed surface. You need the enclosed charge.
  3. Two coupled small oscillations are written as Mx double dot + Kx = 0. You need the normal-mode frequencies.
Checkpoint answers — compare the decision, not just the algebra
  1. Use separation of variables or a first-order linear ODE method. The temperature difference is the dependent quantity; check the initial condition, units of k, and the long-time limit T → Tᵣₒₒₘ.
  2. Use Gauss’s law as a surface integral. Symmetry makes the flux integral efficient; check the surface orientation, dimensions, and whether the assumed symmetry really makes E constant on the surface.
  3. Use linear algebra and an eigenvalue condition such as det(K-ω²M) = 0. Check that ω² has units of inverse time squared and that identical uncoupled oscillators recover the expected limiting frequencies.