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SQA Advanced Higher Physics

Advanced Higher · SQAPhysics34 notes in 4 folders, 218 KB

Notes for SQA Advanced Higher Physics (course specification C857 77, valid from session 2026-27), in a folder for each of the course's content areas in its order: rotational motion and astrophysics, quanta and waves, electromagnetism, and units, prefixes and uncertainties. Each has one note for a topic or a few closely related ones, with the equations, worked examples and the experimental methods that go with them.

Adding them puts a copy in your notes, in a folder of its own with the folders below, for you to change and turn into flashcards or a question deck. Download gives you a zip of markdown files, which opens in any notes app.

What is inside

  • Rotational motion and astrophysics
    • Kinematics with calculus6 KB
    • Angular motion6 KB
    • Circular motion and centripetal force5 KB
    • Moment of inertia5 KB
    • Torque and angular momentum6 KB
    • Rotational kinetic energy6 KB
    • Gravitational fields and orbits7 KB
    • Gravitational potential and escape velocity6 KB
    • General relativity and black holes7 KB
    • Stellar radiation5 KB
    • Star formation and the proton-proton chain6 KB
    • The Hertzsprung–Russell diagram and the life cycle of stars6 KB
  • Quanta and waves
    • Quantum theory and the Bohr atom8 KB
    • Wave–particle duality and the uncertainty principle7 KB
    • Particles from space6 KB
    • Simple harmonic motion7 KB
    • Energy in simple harmonic motion and damping6 KB
    • Travelling waves6 KB
    • Coherence and stationary waves7 KB
    • Interference by division of amplitude8 KB
    • Young's slits6 KB
    • Polarisation6 KB
  • Electromagnetism
    • Electric fields and potential7 KB
    • Charged particles in uniform electric fields7 KB
    • Magnetic fields and forces9 KB
    • Capacitors and RC circuits7 KB
    • Capacitive reactance in AC circuits5 KB
    • Inductors6 KB
    • Inductive reactance in AC circuits5 KB
    • Electromagnetic waves5 KB
  • Units, prefixes and uncertainties
    • Units, prefixes and significant figures7 KB
    • Types of uncertainty and how to estimate them7 KB
    • Combining uncertainties6 KB
    • Graphs, accuracy and evaluating an experiment7 KB

The first note

Rotational motion and astrophysics / Kinematics with calculus

## Rates of change Kinematics describes motion without asking what causes it. At Advanced Higher the quantities are treated as functions of time, and the language of calculus is used because velocity and acceleration are rates of change. Differential notation writes a rate of change as a derivative. If a quantity $y$ depends on time $t$, then $\dfrac{dy}{dt}$ is how fast $y$ is changing at that instant. It is the gradient of the graph of $y$ against $t$, taken at a single point, which is why it can be found for a curve as well as for a straight line. For straight-line motion, with displacement $s$ measured from a fixed point: $$ v = \frac{ds}{dt} \qquad a = \frac{dv}{dt} = \frac{d^2 s}{dt^2} $$ Velocity measures how quickly displacement changes as time passes, and acceleration how quickly velocity changes, so acceleration is the second derivative of displacement. $v$ is in $\mathrm{m\,s^{-1}}$ and $a$ in $\mathrm{m\,s^{-2}}$. Because displacement, velocity and acceleration are vectors, in one dimension their sign carries the direction: a negative $v$ means motion in the negative direction, and a negative $a$ with a positive $v$ means the object is slowing down. ## Deriving the equations of motion The equations for constant acceleration follow from the definitions by integration, so they do not need to be learned as separate facts. They apply only when $a$ is constant. Start from $a = \dfrac{dv}{dt}$ with $a$ constant, and let the velocity be $u$ at $t = 0$ and $v$ at time…

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