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Card 1 of 1661.4.1
1.4.1
Question

Define angular velocity ω.

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Card 11.4.1definition
Question

Define angular velocity ω.

Answer

The **angle turned per second** — the rate of change of θ. Unit: **rad s⁻¹**.

Card 21.4.1definition
Question

Define angular acceleration α.

Answer

The **rate of change of angular velocity** ω. Unit: **rad s⁻²**.

Card 31.4.1definition
Question

What is one radian?

Answer

The angle whose **arc length equals the radius**. A full turn = **2π rad = 360°**.

Card 41.4.1formula
Question

On an ω–t graph, slope and area give…?

Answer

Slope = **angular acceleration** α; area = **angle turned** θ.

Card 51.4.1formula
Question

Rotational version of v = u + at?

Answer

$\omega = \omega_0 + \alpha t$.

Card 61.4.1concept
Question

Convert revolutions to radians?

Answer

Multiply by **2π** (one revolution = 2π rad).

Card 71.4.1definition
Question

Define torque.

Answer

The **turning effect** of a force: $\tau = Fr\sin\theta$. Unit: **N m**.

Card 81.4.1concept
Question

When does a force give zero torque?

Answer

When it acts **through the pivot** (θ = 0, sin θ = 0).

Card 91.4.1concept
Question

Condition for rotational equilibrium?

Answer

The **total torque about any point is zero** (clockwise = anticlockwise).

Card 101.4.1process
Question

Smart choice of pivot when taking torques?

Answer

A point on an **unknown force's line**, so that force has zero torque.

Card 111.4.1concept
Question

Why is a door handle far from the hinges?

Answer

Bigger **r** → bigger torque for the same force.

Card 121.4.1definition
Question

Units: torque vs energy?

Answer

Both are N m, but torque is **N m** (a turning effect); energy is the **joule**.

Card 131.4.2definition
Question

Define moment of inertia.

Answer

Rotation's version of **mass** — resistance to angular acceleration: $I = \sum m r^{2}$. Unit: **kg m²**.

Card 141.4.2concept
Question

Why does mass far from the axis matter most?

Answer

Because r is **squared** in I = Σmr² — doubling the distance quadruples that part's contribution.

Card 151.4.2formula
Question

Rotational version of F = ma?

Answer

$\tau = I\alpha$ (torque = moment of inertia × angular acceleration).

Card 161.4.2comparison
Question

Hoop vs disc (same M, R) — bigger I?

Answer

The **hoop** (I = MR²); the disc is ½MR².

Card 171.4.2formula
Question

I of a solid disc/cylinder about its centre?

Answer

$I = \tfrac{1}{2}MR^{2}$ (given in the question).

Card 181.4.2formula
Question

I of a thin hoop about its centre?

Answer

$I = MR^{2}$ — all the mass is at radius R.

Card 191.4.2concept
Question

Do you need to memorise shape I formulas?

Answer

No — the **exam gives them**; recognise and substitute.

Card 201.4.2formula
Question

Angular acceleration from a torque?

Answer

$\alpha = \tau / I$ — rearranged from τ = Iα.

Card 211.4.2definition
Question

Rotational analogue of force?

Answer

**Torque** τ.

Card 221.4.2concept
Question

Does I depend on the axis chosen?

Answer

Yes — the same object has different I about different axes.

Card 231.4.2definition
Question

Units of moment of inertia?

Answer

**kg m²**.

Card 241.4.3definition
Question

Define angular momentum.

Answer

Rotation's version of momentum: $L = I\omega$. Unit: **kg m² s⁻¹**.

Card 251.4.3concept
Question

When is angular momentum conserved?

Answer

When there is **no external torque** on the system.

Card 261.4.3formula
Question

Conservation equation for a changing I?

Answer

$I_1\omega_1 = I_2\omega_2$.

Card 271.4.3concept
Question

Why does a skater speed up pulling arms in?

Answer

I decreases, so ω increases to keep **L = Iω** constant.

Card 281.4.3formula
Question

Rotational kinetic energy formula?

Answer

$E_k = \tfrac{1}{2}I\omega^{2}$ (the rotational ½mv²).

Card 291.4.3formula
Question

Total KE of a rolling object?

Answer

$\tfrac{1}{2}mv^{2} + \tfrac{1}{2}I\omega^{2}$ — translational **plus** rotational.

Card 301.4.3concept
Question

Double ω — what happens to rotational KE?

Answer

It **quadruples** (E_k ∝ ω²).

Card 311.4.3concept
Question

Is kinetic energy conserved when clay sticks to a disc?

Answer

**No** — angular momentum is conserved, but some kinetic energy is lost.

Card 321.4.3definition
Question

Rotational analogue of p = mv?

Answer

$L = I\omega$.

Card 331.4.3concept
Question

Add mass to a freely spinning disc — what happens to ω?

Answer

ω **decreases** (I up, L constant).

Card 341.4.3definition
Question

Units of angular momentum?

Answer

**kg m² s⁻¹** (or equivalently N m s).

Card 351.5.1definition
Question

What is a reference frame?

Answer

A coordinate grid and clock you measure motion **against**. All motion is **relative** to a chosen frame.

Card 361.5.1definition
Question

Define an inertial reference frame.

Answer

A frame moving at **constant velocity** (no acceleration). Newton's first law holds in it.

Card 371.5.1example
Question

Give one inertial and one non-inertial example.

Answer

Inertial: a train cruising in a straight line at steady speed. Non-inertial: a car going round a bend.

Card 381.5.1formula
Question

State the Galilean velocity transformation.

Answer

$u' = u - v$ — the object's velocity in the moving frame equals its ground velocity minus the frame's velocity.

Card 391.5.1formula
Question

State the Galilean position transformation.

Answer

$x' = x - vt$ — position in the moving frame, where v is the frame's speed.

Card 401.5.1concept
Question

Same direction vs opposite direction — add or subtract?

Answer

Same direction ⇒ **subtract** the speeds; opposite directions ⇒ the speeds **add**.

Card 411.5.1example
Question

A person walks at 1.5 m s⁻¹ toward the front of a train moving at 12 m s⁻¹. Ground speed?

Answer

Same direction ⇒ add: $12 + 1.5 = 13.5$ m s⁻¹.

Card 421.5.1example
Question

Velocity of car B (east, 20 m s⁻¹) seen from car A (east, 30 m s⁻¹)?

Answer

$u' = u - v = 20 - 30 = -10$ m s⁻¹, i.e. 10 m s⁻¹ westward.

Card 431.5.1concept
Question

State Galileo's principle of relativity.

Answer

The **laws of mechanics are the same in every inertial frame** — no experiment can detect uniform motion.

Card 441.5.1concept
Question

Does an absolute rest frame exist?

Answer

**No.** All inertial frames are equivalent; 'at rest' only ever means 'relative to something'.

Card 451.5.1concept
Question

Where does Galilean velocity addition break down?

Answer

Near the **speed of light** — light travels at the same speed in every frame, so simple addition fails (→ special relativity).

Card 461.5.1example
Question

Two trains approach at 25 and 30 m s⁻¹. Relative speed of approach?

Answer

Opposite directions ⇒ add: $25 + 30 = 55$ m s⁻¹.

Card 471.5.2definition
Question

State Einstein's first postulate of special relativity.

Answer

The **laws of physics are the same in all inertial (non-accelerating) reference frames**.

Card 481.5.2definition
Question

State Einstein's second postulate of special relativity.

Answer

The **speed of light in a vacuum is the same for all inertial observers**, regardless of the motion of the source or observer.

Card 491.5.2formula
Question

What is the constant value of the speed of light?

Answer

$c = 3.00 \times 10^{8}$ m s⁻¹ — the same for every inertial observer.

Card 501.5.2definition
Question

What is an inertial reference frame?

Answer

A frame moving at **constant velocity** — no acceleration (no speeding up, slowing down, or turning).

Card 511.5.2example
Question

A ship at 0.50c shines a torch forward. What speed does a planet observer measure for the light?

Answer

Exactly **c**, not 1.5c — by postulate 2 light's speed never adds on the source's speed.

Card 521.5.2comparison
Question

Classical vs relativistic: do speeds add for light?

Answer

Classically speeds add; **relativistically light always measures c** for everyone, so they do not add.

Card 531.5.2concept
Question

Name the cosmic speed limit and why it exists.

Answer

**c** — the postulates make it impossible for anything with mass to reach or exceed the speed of light.

Card 541.5.2concept
Question

What does 'simultaneity is relative' mean?

Answer

Whether two events happen **'at the same time' depends on the observer's motion** — observers in relative motion can disagree.

Card 551.5.2example
Question

Why can't two objects each at 0.90c have a relative speed of 1.80c?

Answer

Because **c is the speed limit**, so any relative speed must stay **below c**; velocities do not add the everyday way near c.

Card 561.5.2concept
Question

Are space and time absolute in special relativity?

Answer

**No** — lengths and time intervals depend on the observer's motion; only the speed of light c is the same for all.

Card 571.5.2process
Question

How do you explain why moving observers disagree on timing?

Answer

Because **both measure light at the same speed c**, they are forced to disagree about **when** events happen.

Card 581.5.2definition
Question

In the exam, how should you phrase postulate 2?

Answer

'The speed of light in a vacuum is the same for **all inertial observers, regardless of the motion of the source or observer**.'

Card 591.5.3formula
Question

State the Lorentz factor formula.

Answer

$\gamma = \dfrac{1}{\sqrt{1 - v^2/c^2}}$ — and it is **always ≥ 1**.

Card 601.5.3definition
Question

What is 'proper time' Δt₀?

Answer

The time between two events measured by a **single clock present at both** — the **shortest** possible time.

Card 611.5.3definition
Question

What is 'proper length' L₀?

Answer

The length of an object measured **in its own rest frame** — the **longest** possible length.

Card 621.5.3formula
Question

State the time-dilation formula.

Answer

$\Delta t = \gamma\,\Delta t_0$. Since γ ≥ 1, **moving clocks run slow**.

Card 631.5.3formula
Question

State the length-contraction formula.

Answer

$L = \dfrac{L_0}{\gamma}$. Since γ ≥ 1, **moving objects contract** along the motion.

Card 641.5.3process
Question

Time: multiply or divide by γ?

Answer

**Multiply** the proper time by γ ($\Delta t = \gamma\,\Delta t_0$) — the time gets bigger.

Card 651.5.3process
Question

Length: multiply or divide by γ?

Answer

**Divide** the proper length by γ ($L = L_0/\gamma$) — the length gets smaller.

Card 661.5.3example
Question

γ for v = 0.80c?

Answer

$\gamma = \dfrac{1}{\sqrt{1 - 0.80^2}} = \dfrac{1}{\sqrt{0.36}} = 1.67$.

Card 671.5.3concept
Question

Which dimension contracts in length contraction?

Answer

Only the dimension **along the direction of motion**; width and height are unchanged.

Card 681.5.3formula
Question

State the relativistic velocity-addition formula.

Answer

$u' = \dfrac{u - v}{1 - uv/c^2}$ — it always keeps the result **below c**.

Card 691.5.3example
Question

Add 0.50c and 0.50c relativistically — what do you get?

Answer

$\dfrac{1.00c}{1 + 0.25} = 0.80c$, **not** 1.0c.

Card 701.5.3comparison
Question

Time dilation vs length contraction — key difference?

Answer

Time **stretches** (Δt = γΔt₀, multiply); length **shrinks** (L = L₀/γ, divide). Both use the same γ.

Card 711.5.4concept
Question

What goes on each axis of a space-time diagram?

Answer

**ct** (speed of light × time) up the **vertical** axis, position **x** along the **horizontal** axis.

Card 721.5.4definition
Question

Define a world line.

Answer

The **path an object traces** on a space-time diagram — its position at every instant.

Card 731.5.4definition
Question

Define an event on a space-time diagram.

Answer

A single **point** — a definite **place at a definite time**.

Card 741.5.4concept
Question

What is the world line of a stationary object?

Answer

A **vertical** line — x stays fixed while ct keeps climbing.

Card 751.5.4concept
Question

At what angle is a light ray's world line, and why?

Answer

At **45°**, because light travels $x = ct$, so equal steps in x and ct.

Card 761.5.4comparison
Question

How does a faster object's world line look?

Answer

**More tilted toward the x-axis** — the faster it goes, the further it leans (but never past 45°).

Card 771.5.4formula
Question

Read speed off a world line.

Answer

$v = c\,\dfrac{\Delta x}{\Delta(ct)}$ — the more horizontal the line, the faster the object.

Card 781.5.4formula
Question

State the invariant space-time interval.

Answer

$(\Delta s)^2 = (c\Delta t)^2 - (\Delta x)^2$ — the same in every inertial frame.

Card 791.5.4concept
Question

Why is the space-time interval special?

Answer

It is **invariant**: all inertial observers measure the **same Δs**, even though Δt and Δx differ.

Card 801.5.4example
Question

Worked: Δt = 5.0 μs, Δx = 900 m, find Δs.

Answer

$(c\Delta t)^2 = 2.25\times10^6$, $(\Delta x)^2 = 8.1\times10^5$, so $(\Delta s)^2 = 1.44\times10^6$ and **Δs = 1200 m**.

Card 811.5.4concept
Question

Is simultaneity absolute?

Answer

**No** — events simultaneous in one frame need not be in another; the line of 'now' **tilts** for a moving observer.

Card 821.5.4comparison
Question

What do all observers agree on?

Answer

The **space-time interval** Δs, the cause-and-effect order of events, and that **light travels at 45°** (speed c).

Card 832.4.1definition
Question

Define internal energy U of a gas.

Answer

The **total energy of all the particles**: their random **kinetic energy** + the **potential energy** of the forces between them.

Card 842.4.1concept
Question

What does the internal energy of an **ideal gas** depend on?

Answer

**Temperature only** — an ideal gas has no inter-particle PE, so U is fixed by the random KE of the particles.

Card 852.4.1formula
Question

State the first law of thermodynamics.

Answer

$Q = \Delta U + W$ — the heat **added** equals the rise in **internal energy** plus the **work done by** the gas.

Card 862.4.1formula
Question

Rearrange the first law for ΔU.

Answer

$\Delta U = Q - W$ (heat in **minus** work done by the gas).

Card 872.4.1concept
Question

In Q = ΔU + W, what is the sign of Q when heat is **removed**?

Answer

**Negative** — Q is the heat **added** to the gas, so heat leaving makes Q < 0.

Card 882.4.1concept
Question

In Q = ΔU + W, what is the sign of W when the gas is **compressed**?

Answer

**Negative** — W is the work done **by** the gas; on compression the surroundings do work on it, so W < 0.

Card 892.4.1formula
Question

Work done by a gas at constant pressure?

Answer

$W = P\,\Delta V$ — pressure times the change in volume.

Card 902.4.1definition
Question

Units for W = PΔV?

Answer

P in **pascals (Pa)**, ΔV in **cubic metres (m³)**, giving W in **joules (J)**.

Card 912.4.1comparison
Question

Internal energy vs heat — what's the difference?

Answer

**Internal energy** is energy a gas **already has** inside; **heat** is energy **flowing** in or out due to a temperature difference.

Card 922.4.1concept
Question

For an ideal gas at **constant temperature**, what is ΔU?

Answer

**ΔU = 0** — U depends on temperature alone, so no temperature change means no change in internal energy.

Card 932.4.1example
Question

500 J heat added, gas does 200 J work — find ΔU.

Answer

$\Delta U = Q - W = 500 - 200 = 300$ J (the gas warms).

Card 942.4.1process
Question

Quick way to handle the signs in the first law?

Answer

Write each sign in **words** first ('heat removed → Q negative', 'gas compressed → W negative'), then plug into $\Delta U = Q - W$.

Card 952.4.2definition
Question

What does entropy S measure?

Answer

The **disorder** of a system — the **number of microstates** (microscopic arrangements) available. Unit: **J K⁻¹**.

Card 962.4.2definition
Question

What is a microstate?

Answer

One specific microscopic arrangement of the particles that gives the same overall (macroscopic) state. **More microstates ⇒ higher entropy**.

Card 972.4.2formula
Question

Formula for entropy change?

Answer

$\Delta S = \dfrac{\Delta Q}{T}$, with **T in kelvin**.

Card 982.4.2formula
Question

In ΔS = ΔQ/T, what are the units?

Answer

$\Delta S$ in **J K⁻¹**, $\Delta Q$ in **J**, $T$ in **K**.

Card 992.4.2concept
Question

Sign of ΔQ for heat flowing in vs out?

Answer

Heat **in** ⇒ ΔQ is **positive** (entropy rises); heat **out** ⇒ ΔQ is **negative** (entropy falls).

Card 1002.4.2definition
Question

State the second law of thermodynamics.

Answer

The **entropy of an isolated system never decreases** — it increases for any irreversible (real) process.

Card 1012.4.2concept
Question

Can one part of a system lose entropy?

Answer

Yes — but only if another part gains **more**, so the **total** entropy of the isolated system still does not decrease.

Card 1022.4.2concept
Question

Why does heat flow hot → cold by itself?

Answer

Because it **increases the total entropy** of the universe ($\Delta S_{total} > 0$); the reverse would decrease it, so it never happens unaided.

Card 1032.4.2concept
Question

What is 'time's arrow'?

Answer

The **direction** of time set by the second law: real processes always run the way that **increases total entropy**.

Card 1042.4.2process
Question

How do you test if a process is allowed?

Answer

Calculate $\Delta S_{total}$ for the isolated system. If it is **positive**, the process can occur (and is irreversible).

Card 1052.4.2concept
Question

Why is the cold body's entropy gain larger?

Answer

$\Delta S = \Delta Q/T$, and the **cold** body has the **smaller T**, so for the same ΔQ it gains **more** entropy than the hot body loses.

Card 1062.4.2comparison
Question

Entropy unit vs energy unit?

Answer

Entropy is the **joule per kelvin (J K⁻¹)**; energy is the **joule (J)** — do not confuse them.

Card 1072.4.3definition
Question

State the first law of thermodynamics.

Answer

$\Delta U = Q - W$, where **W** is the work done **by** the gas. Internal energy U depends only on temperature.

Card 1082.4.3concept
Question

Isothermal process — what is constant, and the consequence?

Answer

**T** is constant, so $\Delta U = 0$ and therefore $Q = W$.

Card 1092.4.3concept
Question

Isobaric process — what is constant, and the work?

Answer

**P** is constant; the work done by the gas is $W = P\,\Delta V$.

Card 1102.4.3concept
Question

Isovolumetric process — what is constant, and the consequence?

Answer

**V** is constant, so $W = 0$ and therefore $Q = \Delta U$.

Card 1112.4.3concept
Question

Adiabatic process — what is zero, and the consequence?

Answer

**Q = 0** (no heat flows), so $\Delta U = -W$.

Card 1122.4.3concept
Question

On a p–V diagram, what is the work done by the gas?

Answer

The **area under the curve** between the start and end volumes.

Card 1132.4.3process
Question

What does a heat engine do each cycle?

Answer

Takes in **Q_in** from the hot reservoir, does useful **work W**, and rejects **Q_out** to the cold reservoir. $W = Q_{in} - Q_{out}$.

Card 1142.4.3formula
Question

Give the efficiency formula for a heat engine.

Answer

$\eta = \dfrac{\text{useful work}}{\text{energy input}} = 1 - \dfrac{Q_{out}}{Q_{in}}$.

Card 1152.4.3formula
Question

Give the Carnot (maximum) efficiency formula.

Answer

$\eta_{Carnot} = 1 - \dfrac{T_{cold}}{T_{hot}}$, with both temperatures in **kelvin**.

Card 1162.4.3concept
Question

Why is a real engine's efficiency below the Carnot value?

Answer

Friction, turbulence and unwanted heat loss waste energy, so the real efficiency is always **lower** than the Carnot ceiling.

Card 1172.4.3example
Question

Worked example — efficiency from Q_in = 800 J, Q_out = 600 J?

Answer

$\eta = 1 - \dfrac{600}{800} = 0.25$, i.e. **25%**.

Card 1182.4.3example
Question

Worked example — Carnot efficiency between 500 K and 300 K?

Answer

$\eta_{Carnot} = 1 - \dfrac{300}{500} = 0.40$, i.e. **40%**.

Card 1194.4.1definition
Question

Define magnetic flux Φ.

Answer

How much magnetic field threads through a loop: $\Phi = BA\cos\theta$. Unit: **weber (Wb)**.

Card 1204.4.1concept
Question

In Φ = BA cos θ, what is θ measured from?

Answer

The angle between **B** and the **normal** to the loop (not the surface). Square-on ⇒ θ = 0.

Card 1214.4.1concept
Question

When is the flux through a loop zero?

Answer

When the loop is **edge-on** to the field (θ = 90°, cos 90° = 0).

Card 1224.4.1formula
Question

State Faraday's law of induction.

Answer

The induced emf equals the **rate of change** of flux linkage: $\varepsilon = -N\,\Delta\Phi/\Delta t$.

Card 1234.4.1concept
Question

What is needed to induce an emf?

Answer

A **changing** flux. A steady flux — however strong — induces **no** emf.

Card 1244.4.1definition
Question

State Lenz's law.

Answer

An induced current flows so as to **oppose the change** in flux that produced it.

Card 1254.4.1concept
Question

What does the minus sign in Faraday's law mean?

Answer

It is **Lenz's law** — the induced effect opposes the change. This is **conservation of energy**.

Card 1264.4.1comparison
Question

Faraday's law vs Lenz's law?

Answer

**Faraday** gives the **size** of the emf; **Lenz** gives its **direction**.

Card 1274.4.1formula
Question

Write the motional-emf formula.

Answer

$\varepsilon = BvL$ — for a rod of length L moving at speed v perpendicular to field B.

Card 1284.4.1example
Question

Worked: rod L = 0.40 m, v = 3.0 m s⁻¹, B = 0.50 T. emf?

Answer

$\varepsilon = BvL = 0.50\times3.0\times0.40 = 0.60$ V.

Card 1294.4.1concept
Question

Why does a moving rod produce an emf (link to Faraday)?

Answer

As it moves it **sweeps out new area**, so the flux through the circuit changes — that change induces the emf.

Card 1304.4.1process
Question

How to find the direction of an induced current?

Answer

Apply **Lenz's law**: the current opposes the change in flux (it tries to keep the flux the same).

Card 1314.4.2concept
Question

How does an AC generator work?

Answer

A **coil is spun** in a magnetic field. The changing flux induces a **sinusoidal emf** — alternating current (AC).

Card 1324.4.2concept
Question

When is the generator emf at its peak?

Answer

When the coil is **edge-on** to the field — the flux is changing **fastest** there.

Card 1334.4.2formula
Question

Peak emf of an AC generator?

Answer

$\varepsilon_0 = BAN\omega$ — increase any of **B**, **A**, **N** or **ω** to raise it.

Card 1344.4.2definition
Question

What does B, A, N, ω each stand for in ε₀ = BANω?

Answer

**B** flux density, **A** coil area, **N** turns, **ω** angular frequency of rotation.

Card 1354.4.2definition
Question

Define the rms value of an AC.

Answer

The **steady DC value** that delivers the **same average power** (same heating) as the AC.

Card 1364.4.2formula
Question

Convert peak to rms (sine wave)?

Answer

$V_{rms} = \dfrac{V_0}{\sqrt{2}}$ and $I_{rms} = \dfrac{I_0}{\sqrt{2}}$ — divide the peak by √2 (≈ 1.41).

Card 1374.4.2concept
Question

Is rms larger or smaller than the peak?

Answer

**Smaller** — rms = peak ÷ √2. The mains "230 V" is an **rms** value.

Card 1384.4.2definition
Question

What does a transformer do?

Answer

Changes an **AC voltage** up or down using two coils on a shared iron core.

Card 1394.4.2formula
Question

Transformer voltage and turns relationship?

Answer

$\dfrac{\varepsilon_p}{\varepsilon_s} = \dfrac{N_p}{N_s}$ — the **voltage ratio equals the turns ratio**.

Card 1404.4.2comparison
Question

Step-up vs step-down transformer?

Answer

**Step-up**: more secondary turns ⇒ higher V, lower I. **Step-down**: fewer secondary turns ⇒ lower V, higher I.

Card 1414.4.2concept
Question

What does an ideal transformer conserve?

Answer

**Power**: $\varepsilon_p I_p = \varepsilon_s I_s$. That is why the **current ratio is inverted**.

Card 1424.4.2process
Question

Find the secondary voltage of a transformer?

Answer

$V_s = V_p \times \dfrac{N_s}{N_p}$ — multiply the primary voltage by the turns ratio.

Card 1435.2.1definition
Question

What is a photon?

Answer

A **quantum (packet) of light energy**, E = hf.

Card 1445.2.1formula
Question

Photon energy formula?

Answer

$E = hf$ (or $E = hc/\lambda$); h = 6.63×10⁻³⁴ J s.

Card 1455.2.1definition
Question

What is the photoelectric effect?

Answer

Light ejecting **electrons** from a metal surface.

Card 1465.2.1formula
Question

The photoelectric equation?

Answer

$E_{\max} = hf - \Phi$ (max electron KE = photon energy − work function).

Card 1475.2.1definition
Question

What is the work function Φ?

Answer

The **minimum energy** needed to free an electron from the metal.

Card 1485.2.1concept
Question

What is the threshold frequency?

Answer

The lowest frequency that ejects electrons: $f_0 = \Phi/h$ (where E_max = 0).

Card 1495.2.1concept
Question

Increase the light's intensity (same frequency) — effect?

Answer

**More** electrons ejected per second; their max KE is **unchanged**.

Card 1505.2.1concept
Question

Increase the light's frequency — effect on max KE?

Answer

Max KE **increases** (E_max = hf − Φ).

Card 1515.2.1concept
Question

Why does the photoelectric effect need photons?

Answer

One electron absorbs **one photon**; a sharp threshold can't be explained by a smooth wave.

Card 1525.2.1comparison
Question

Which effects show light's WAVE nature?

Answer

**Diffraction** and **interference**.

Card 1535.2.1comparison
Question

Which effect shows light's PARTICLE nature?

Answer

The **photoelectric effect**.

Card 1545.2.1concept
Question

What is wave–particle duality?

Answer

Light (and matter) behaves as **both** a wave and a particle depending on the experiment.

Card 1555.2.2definition
Question

What is a matter wave?

Answer

The **wave** behaviour of a moving particle, with wavelength λ = h/p.

Card 1565.2.2formula
Question

De Broglie wavelength formula?

Answer

$\lambda = h/p$ (p = mv for a slow particle).

Card 1575.2.2concept
Question

How does λ depend on momentum?

Answer

**Inversely** — bigger momentum gives a **shorter** wavelength.

Card 1585.2.2concept
Question

What is the evidence for matter waves?

Answer

**Electron diffraction** — electrons make diffraction patterns off crystals.

Card 1595.2.2concept
Question

Why does a cricket ball not diffract?

Answer

Its momentum is huge, so λ = h/p is far too small (~10⁻³⁴ m) to notice.

Card 1605.2.2process
Question

Steps to find a de Broglie wavelength?

Answer

Find **p = mv** first, then **λ = h/p**.

Card 1615.2.2formula
Question

State Heisenberg's uncertainty principle.

Answer

$\Delta x\,\Delta p \ge h/4\pi$ — position and momentum can't both be exact.

Card 1625.2.2concept
Question

Is uncertainty due to poor instruments?

Answer

**No** — it is a fundamental limit of nature, not a measurement fault.

Card 1635.2.2concept
Question

Why do electrons diffract off crystals but not big slits?

Answer

Their λ (~10⁻¹⁰ m) matches the **atomic spacing**.

Card 1645.2.2concept
Question

Double a particle's speed — effect on λ?

Answer

λ is **halved** (p doubles, λ = h/p).

Card 1655.2.2definition
Question

Units of de Broglie wavelength?

Answer

**metres (m)**.

Card 1665.2.2concept
Question

Wave–particle duality for matter means…

Answer

Particles like electrons show **both** particle and wave behaviour.

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