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Define angular velocity ω.
The **angle turned per second** — the rate of change of θ. Unit: **rad s⁻¹**.
Define angular acceleration α.
The **rate of change of angular velocity** ω. Unit: **rad s⁻²**.
What is one radian?
The angle whose **arc length equals the radius**. A full turn = **2π rad = 360°**.
On an ω–t graph, slope and area give…?
Slope = **angular acceleration** α; area = **angle turned** θ.
Rotational version of v = u + at?
$\omega = \omega_0 + \alpha t$.
Convert revolutions to radians?
Multiply by **2π** (one revolution = 2π rad).
Define torque.
The **turning effect** of a force: $\tau = Fr\sin\theta$. Unit: **N m**.
When does a force give zero torque?
When it acts **through the pivot** (θ = 0, sin θ = 0).
Condition for rotational equilibrium?
The **total torque about any point is zero** (clockwise = anticlockwise).
Smart choice of pivot when taking torques?
A point on an **unknown force's line**, so that force has zero torque.
Why is a door handle far from the hinges?
Bigger **r** → bigger torque for the same force.
Units: torque vs energy?
Both are N m, but torque is **N m** (a turning effect); energy is the **joule**.
Define moment of inertia.
Rotation's version of **mass** — resistance to angular acceleration: $I = \sum m r^{2}$. Unit: **kg m²**.
Why does mass far from the axis matter most?
Because r is **squared** in I = Σmr² — doubling the distance quadruples that part's contribution.
Rotational version of F = ma?
$\tau = I\alpha$ (torque = moment of inertia × angular acceleration).
Hoop vs disc (same M, R) — bigger I?
The **hoop** (I = MR²); the disc is ½MR².
I of a solid disc/cylinder about its centre?
$I = \tfrac{1}{2}MR^{2}$ (given in the question).
I of a thin hoop about its centre?
$I = MR^{2}$ — all the mass is at radius R.
Do you need to memorise shape I formulas?
No — the **exam gives them**; recognise and substitute.
Angular acceleration from a torque?
$\alpha = \tau / I$ — rearranged from τ = Iα.
Rotational analogue of force?
**Torque** τ.
Does I depend on the axis chosen?
Yes — the same object has different I about different axes.
Units of moment of inertia?
**kg m²**.
Define angular momentum.
Rotation's version of momentum: $L = I\omega$. Unit: **kg m² s⁻¹**.
When is angular momentum conserved?
When there is **no external torque** on the system.
Conservation equation for a changing I?
$I_1\omega_1 = I_2\omega_2$.
Why does a skater speed up pulling arms in?
I decreases, so ω increases to keep **L = Iω** constant.
Rotational kinetic energy formula?
$E_k = \tfrac{1}{2}I\omega^{2}$ (the rotational ½mv²).
Total KE of a rolling object?
$\tfrac{1}{2}mv^{2} + \tfrac{1}{2}I\omega^{2}$ — translational **plus** rotational.
Double ω — what happens to rotational KE?
It **quadruples** (E_k ∝ ω²).
Is kinetic energy conserved when clay sticks to a disc?
**No** — angular momentum is conserved, but some kinetic energy is lost.
Rotational analogue of p = mv?
$L = I\omega$.
Add mass to a freely spinning disc — what happens to ω?
ω **decreases** (I up, L constant).
Units of angular momentum?
**kg m² s⁻¹** (or equivalently N m s).
What is a reference frame?
A coordinate grid and clock you measure motion **against**. All motion is **relative** to a chosen frame.
Define an inertial reference frame.
A frame moving at **constant velocity** (no acceleration). Newton's first law holds in it.
Give one inertial and one non-inertial example.
Inertial: a train cruising in a straight line at steady speed. Non-inertial: a car going round a bend.
State the Galilean velocity transformation.
$u' = u - v$ — the object's velocity in the moving frame equals its ground velocity minus the frame's velocity.
State the Galilean position transformation.
$x' = x - vt$ — position in the moving frame, where v is the frame's speed.
Same direction vs opposite direction — add or subtract?
Same direction ⇒ **subtract** the speeds; opposite directions ⇒ the speeds **add**.
A person walks at 1.5 m s⁻¹ toward the front of a train moving at 12 m s⁻¹. Ground speed?
Same direction ⇒ add: $12 + 1.5 = 13.5$ m s⁻¹.
Velocity of car B (east, 20 m s⁻¹) seen from car A (east, 30 m s⁻¹)?
$u' = u - v = 20 - 30 = -10$ m s⁻¹, i.e. 10 m s⁻¹ westward.
State Galileo's principle of relativity.
The **laws of mechanics are the same in every inertial frame** — no experiment can detect uniform motion.
Does an absolute rest frame exist?
**No.** All inertial frames are equivalent; 'at rest' only ever means 'relative to something'.
Where does Galilean velocity addition break down?
Near the **speed of light** — light travels at the same speed in every frame, so simple addition fails (→ special relativity).
Two trains approach at 25 and 30 m s⁻¹. Relative speed of approach?
Opposite directions ⇒ add: $25 + 30 = 55$ m s⁻¹.
State Einstein's first postulate of special relativity.
The **laws of physics are the same in all inertial (non-accelerating) reference frames**.
State Einstein's second postulate of special relativity.
The **speed of light in a vacuum is the same for all inertial observers**, regardless of the motion of the source or observer.
What is the constant value of the speed of light?
$c = 3.00 \times 10^{8}$ m s⁻¹ — the same for every inertial observer.
What is an inertial reference frame?
A frame moving at **constant velocity** — no acceleration (no speeding up, slowing down, or turning).
A ship at 0.50c shines a torch forward. What speed does a planet observer measure for the light?
Exactly **c**, not 1.5c — by postulate 2 light's speed never adds on the source's speed.
Classical vs relativistic: do speeds add for light?
Classically speeds add; **relativistically light always measures c** for everyone, so they do not add.
Name the cosmic speed limit and why it exists.
**c** — the postulates make it impossible for anything with mass to reach or exceed the speed of light.
What does 'simultaneity is relative' mean?
Whether two events happen **'at the same time' depends on the observer's motion** — observers in relative motion can disagree.
Why can't two objects each at 0.90c have a relative speed of 1.80c?
Because **c is the speed limit**, so any relative speed must stay **below c**; velocities do not add the everyday way near c.
Are space and time absolute in special relativity?
**No** — lengths and time intervals depend on the observer's motion; only the speed of light c is the same for all.
How do you explain why moving observers disagree on timing?
Because **both measure light at the same speed c**, they are forced to disagree about **when** events happen.
In the exam, how should you phrase postulate 2?
'The speed of light in a vacuum is the same for **all inertial observers, regardless of the motion of the source or observer**.'
State the Lorentz factor formula.
$\gamma = \dfrac{1}{\sqrt{1 - v^2/c^2}}$ — and it is **always ≥ 1**.
What is 'proper time' Δt₀?
The time between two events measured by a **single clock present at both** — the **shortest** possible time.
What is 'proper length' L₀?
The length of an object measured **in its own rest frame** — the **longest** possible length.
State the time-dilation formula.
$\Delta t = \gamma\,\Delta t_0$. Since γ ≥ 1, **moving clocks run slow**.
State the length-contraction formula.
$L = \dfrac{L_0}{\gamma}$. Since γ ≥ 1, **moving objects contract** along the motion.
Time: multiply or divide by γ?
**Multiply** the proper time by γ ($\Delta t = \gamma\,\Delta t_0$) — the time gets bigger.
Length: multiply or divide by γ?
**Divide** the proper length by γ ($L = L_0/\gamma$) — the length gets smaller.
γ for v = 0.80c?
$\gamma = \dfrac{1}{\sqrt{1 - 0.80^2}} = \dfrac{1}{\sqrt{0.36}} = 1.67$.
Which dimension contracts in length contraction?
Only the dimension **along the direction of motion**; width and height are unchanged.
State the relativistic velocity-addition formula.
$u' = \dfrac{u - v}{1 - uv/c^2}$ — it always keeps the result **below c**.
Add 0.50c and 0.50c relativistically — what do you get?
$\dfrac{1.00c}{1 + 0.25} = 0.80c$, **not** 1.0c.
Time dilation vs length contraction — key difference?
Time **stretches** (Δt = γΔt₀, multiply); length **shrinks** (L = L₀/γ, divide). Both use the same γ.
What goes on each axis of a space-time diagram?
**ct** (speed of light × time) up the **vertical** axis, position **x** along the **horizontal** axis.
Define a world line.
The **path an object traces** on a space-time diagram — its position at every instant.
Define an event on a space-time diagram.
A single **point** — a definite **place at a definite time**.
What is the world line of a stationary object?
A **vertical** line — x stays fixed while ct keeps climbing.
At what angle is a light ray's world line, and why?
At **45°**, because light travels $x = ct$, so equal steps in x and ct.
How does a faster object's world line look?
**More tilted toward the x-axis** — the faster it goes, the further it leans (but never past 45°).
Read speed off a world line.
$v = c\,\dfrac{\Delta x}{\Delta(ct)}$ — the more horizontal the line, the faster the object.
State the invariant space-time interval.
$(\Delta s)^2 = (c\Delta t)^2 - (\Delta x)^2$ — the same in every inertial frame.
Why is the space-time interval special?
It is **invariant**: all inertial observers measure the **same Δs**, even though Δt and Δx differ.
Worked: Δt = 5.0 μs, Δx = 900 m, find Δs.
$(c\Delta t)^2 = 2.25\times10^6$, $(\Delta x)^2 = 8.1\times10^5$, so $(\Delta s)^2 = 1.44\times10^6$ and **Δs = 1200 m**.
Is simultaneity absolute?
**No** — events simultaneous in one frame need not be in another; the line of 'now' **tilts** for a moving observer.
What do all observers agree on?
The **space-time interval** Δs, the cause-and-effect order of events, and that **light travels at 45°** (speed c).
Define internal energy U of a gas.
The **total energy of all the particles**: their random **kinetic energy** + the **potential energy** of the forces between them.
What does the internal energy of an **ideal gas** depend on?
**Temperature only** — an ideal gas has no inter-particle PE, so U is fixed by the random KE of the particles.
State the first law of thermodynamics.
$Q = \Delta U + W$ — the heat **added** equals the rise in **internal energy** plus the **work done by** the gas.
Rearrange the first law for ΔU.
$\Delta U = Q - W$ (heat in **minus** work done by the gas).
In Q = ΔU + W, what is the sign of Q when heat is **removed**?
**Negative** — Q is the heat **added** to the gas, so heat leaving makes Q < 0.
In Q = ΔU + W, what is the sign of W when the gas is **compressed**?
**Negative** — W is the work done **by** the gas; on compression the surroundings do work on it, so W < 0.
Work done by a gas at constant pressure?
$W = P\,\Delta V$ — pressure times the change in volume.
Units for W = PΔV?
P in **pascals (Pa)**, ΔV in **cubic metres (m³)**, giving W in **joules (J)**.
Internal energy vs heat — what's the difference?
**Internal energy** is energy a gas **already has** inside; **heat** is energy **flowing** in or out due to a temperature difference.
For an ideal gas at **constant temperature**, what is ΔU?
**ΔU = 0** — U depends on temperature alone, so no temperature change means no change in internal energy.
500 J heat added, gas does 200 J work — find ΔU.
$\Delta U = Q - W = 500 - 200 = 300$ J (the gas warms).
Quick way to handle the signs in the first law?
Write each sign in **words** first ('heat removed → Q negative', 'gas compressed → W negative'), then plug into $\Delta U = Q - W$.
What does entropy S measure?
The **disorder** of a system — the **number of microstates** (microscopic arrangements) available. Unit: **J K⁻¹**.
What is a microstate?
One specific microscopic arrangement of the particles that gives the same overall (macroscopic) state. **More microstates ⇒ higher entropy**.
Formula for entropy change?
$\Delta S = \dfrac{\Delta Q}{T}$, with **T in kelvin**.
In ΔS = ΔQ/T, what are the units?
$\Delta S$ in **J K⁻¹**, $\Delta Q$ in **J**, $T$ in **K**.
Sign of ΔQ for heat flowing in vs out?
Heat **in** ⇒ ΔQ is **positive** (entropy rises); heat **out** ⇒ ΔQ is **negative** (entropy falls).
State the second law of thermodynamics.
The **entropy of an isolated system never decreases** — it increases for any irreversible (real) process.
Can one part of a system lose entropy?
Yes — but only if another part gains **more**, so the **total** entropy of the isolated system still does not decrease.
Why does heat flow hot → cold by itself?
Because it **increases the total entropy** of the universe ($\Delta S_{total} > 0$); the reverse would decrease it, so it never happens unaided.
What is 'time's arrow'?
The **direction** of time set by the second law: real processes always run the way that **increases total entropy**.
How do you test if a process is allowed?
Calculate $\Delta S_{total}$ for the isolated system. If it is **positive**, the process can occur (and is irreversible).
Why is the cold body's entropy gain larger?
$\Delta S = \Delta Q/T$, and the **cold** body has the **smaller T**, so for the same ΔQ it gains **more** entropy than the hot body loses.
Entropy unit vs energy unit?
Entropy is the **joule per kelvin (J K⁻¹)**; energy is the **joule (J)** — do not confuse them.
State the first law of thermodynamics.
$\Delta U = Q - W$, where **W** is the work done **by** the gas. Internal energy U depends only on temperature.
Isothermal process — what is constant, and the consequence?
**T** is constant, so $\Delta U = 0$ and therefore $Q = W$.
Isobaric process — what is constant, and the work?
**P** is constant; the work done by the gas is $W = P\,\Delta V$.
Isovolumetric process — what is constant, and the consequence?
**V** is constant, so $W = 0$ and therefore $Q = \Delta U$.
Adiabatic process — what is zero, and the consequence?
**Q = 0** (no heat flows), so $\Delta U = -W$.
On a p–V diagram, what is the work done by the gas?
The **area under the curve** between the start and end volumes.
What does a heat engine do each cycle?
Takes in **Q_in** from the hot reservoir, does useful **work W**, and rejects **Q_out** to the cold reservoir. $W = Q_{in} - Q_{out}$.
Give the efficiency formula for a heat engine.
$\eta = \dfrac{\text{useful work}}{\text{energy input}} = 1 - \dfrac{Q_{out}}{Q_{in}}$.
Give the Carnot (maximum) efficiency formula.
$\eta_{Carnot} = 1 - \dfrac{T_{cold}}{T_{hot}}$, with both temperatures in **kelvin**.
Why is a real engine's efficiency below the Carnot value?
Friction, turbulence and unwanted heat loss waste energy, so the real efficiency is always **lower** than the Carnot ceiling.
Worked example — efficiency from Q_in = 800 J, Q_out = 600 J?
$\eta = 1 - \dfrac{600}{800} = 0.25$, i.e. **25%**.
Worked example — Carnot efficiency between 500 K and 300 K?
$\eta_{Carnot} = 1 - \dfrac{300}{500} = 0.40$, i.e. **40%**.
Define magnetic flux Φ.
How much magnetic field threads through a loop: $\Phi = BA\cos\theta$. Unit: **weber (Wb)**.
In Φ = BA cos θ, what is θ measured from?
The angle between **B** and the **normal** to the loop (not the surface). Square-on ⇒ θ = 0.
When is the flux through a loop zero?
When the loop is **edge-on** to the field (θ = 90°, cos 90° = 0).
State Faraday's law of induction.
The induced emf equals the **rate of change** of flux linkage: $\varepsilon = -N\,\Delta\Phi/\Delta t$.
What is needed to induce an emf?
A **changing** flux. A steady flux — however strong — induces **no** emf.
State Lenz's law.
An induced current flows so as to **oppose the change** in flux that produced it.
What does the minus sign in Faraday's law mean?
It is **Lenz's law** — the induced effect opposes the change. This is **conservation of energy**.
Faraday's law vs Lenz's law?
**Faraday** gives the **size** of the emf; **Lenz** gives its **direction**.
Write the motional-emf formula.
$\varepsilon = BvL$ — for a rod of length L moving at speed v perpendicular to field B.
Worked: rod L = 0.40 m, v = 3.0 m s⁻¹, B = 0.50 T. emf?
$\varepsilon = BvL = 0.50\times3.0\times0.40 = 0.60$ V.
Why does a moving rod produce an emf (link to Faraday)?
As it moves it **sweeps out new area**, so the flux through the circuit changes — that change induces the emf.
How to find the direction of an induced current?
Apply **Lenz's law**: the current opposes the change in flux (it tries to keep the flux the same).
How does an AC generator work?
A **coil is spun** in a magnetic field. The changing flux induces a **sinusoidal emf** — alternating current (AC).
When is the generator emf at its peak?
When the coil is **edge-on** to the field — the flux is changing **fastest** there.
Peak emf of an AC generator?
$\varepsilon_0 = BAN\omega$ — increase any of **B**, **A**, **N** or **ω** to raise it.
What does B, A, N, ω each stand for in ε₀ = BANω?
**B** flux density, **A** coil area, **N** turns, **ω** angular frequency of rotation.
Define the rms value of an AC.
The **steady DC value** that delivers the **same average power** (same heating) as the AC.
Convert peak to rms (sine wave)?
$V_{rms} = \dfrac{V_0}{\sqrt{2}}$ and $I_{rms} = \dfrac{I_0}{\sqrt{2}}$ — divide the peak by √2 (≈ 1.41).
Is rms larger or smaller than the peak?
**Smaller** — rms = peak ÷ √2. The mains "230 V" is an **rms** value.
What does a transformer do?
Changes an **AC voltage** up or down using two coils on a shared iron core.
Transformer voltage and turns relationship?
$\dfrac{\varepsilon_p}{\varepsilon_s} = \dfrac{N_p}{N_s}$ — the **voltage ratio equals the turns ratio**.
Step-up vs step-down transformer?
**Step-up**: more secondary turns ⇒ higher V, lower I. **Step-down**: fewer secondary turns ⇒ lower V, higher I.
What does an ideal transformer conserve?
**Power**: $\varepsilon_p I_p = \varepsilon_s I_s$. That is why the **current ratio is inverted**.
Find the secondary voltage of a transformer?
$V_s = V_p \times \dfrac{N_s}{N_p}$ — multiply the primary voltage by the turns ratio.
What is a photon?
A **quantum (packet) of light energy**, E = hf.
Photon energy formula?
$E = hf$ (or $E = hc/\lambda$); h = 6.63×10⁻³⁴ J s.
What is the photoelectric effect?
Light ejecting **electrons** from a metal surface.
The photoelectric equation?
$E_{\max} = hf - \Phi$ (max electron KE = photon energy − work function).
What is the work function Φ?
The **minimum energy** needed to free an electron from the metal.
What is the threshold frequency?
The lowest frequency that ejects electrons: $f_0 = \Phi/h$ (where E_max = 0).
Increase the light's intensity (same frequency) — effect?
**More** electrons ejected per second; their max KE is **unchanged**.
Increase the light's frequency — effect on max KE?
Max KE **increases** (E_max = hf − Φ).
Why does the photoelectric effect need photons?
One electron absorbs **one photon**; a sharp threshold can't be explained by a smooth wave.
Which effects show light's WAVE nature?
**Diffraction** and **interference**.
Which effect shows light's PARTICLE nature?
The **photoelectric effect**.
What is wave–particle duality?
Light (and matter) behaves as **both** a wave and a particle depending on the experiment.
What is a matter wave?
The **wave** behaviour of a moving particle, with wavelength λ = h/p.
De Broglie wavelength formula?
$\lambda = h/p$ (p = mv for a slow particle).
How does λ depend on momentum?
**Inversely** — bigger momentum gives a **shorter** wavelength.
What is the evidence for matter waves?
**Electron diffraction** — electrons make diffraction patterns off crystals.
Why does a cricket ball not diffract?
Its momentum is huge, so λ = h/p is far too small (~10⁻³⁴ m) to notice.
Steps to find a de Broglie wavelength?
Find **p = mv** first, then **λ = h/p**.
State Heisenberg's uncertainty principle.
$\Delta x\,\Delta p \ge h/4\pi$ — position and momentum can't both be exact.
Is uncertainty due to poor instruments?
**No** — it is a fundamental limit of nature, not a measurement fault.
Why do electrons diffract off crystals but not big slits?
Their λ (~10⁻¹⁰ m) matches the **atomic spacing**.
Double a particle's speed — effect on λ?
λ is **halved** (p doubles, λ = h/p).
Units of de Broglie wavelength?
**metres (m)**.
Wave–particle duality for matter means…
Particles like electrons show **both** particle and wave behaviour.
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