General relativity

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Concept 1

Frames of reference and the equivalence principle

Special relativity only deals with inertial frames. General relativity is what you need once a frame is accelerating.

An inertial frame of reference moves at constant velocity — it is not accelerating. A non-inertial frame is one that is accelerating with respect to an inertial frame.

Throw a ball across a cabin moving at constant velocity and it travels in a straight line. Throw the same ball across a cabin that is accelerating and, to someone inside, it curves — even though no force acts on it sideways. The curve is the frame accelerating out from under the ball.

Now seal the cabin. Inside, that curved path is exactly what you would see if the cabin were sitting still in a gravitational field. There is no measurement you can make inside to tell the two apart.

A ball thrown across an inertial and a non-inertial cabin In a cabin moving at constant velocity the ball crosses in a straight line. In a cabin that is accelerating, shown by three motion arrows of increasing length, the same ball follows a curved path down towards the far corner. Inertial frame constant velocity ball goes straight Non-inertial frame accelerating ball curves
Sealed inside the right-hand cabin, the curved path of the ball is indistinguishable from the path it would take in a uniform gravitational field.
Learn this word for word

The equivalence principle: “It is not possible to distinguish between the effects on a body of uniform acceleration and a uniform gravitational field.”

Watch out: the marking instructions say “effects must be implied”. An answer that says acceleration and gravity are the same thing does not get the mark — it is their effects that cannot be told apart.

And the other definition: a non-inertial frame of reference is “a frame of reference that is accelerating with respect to an inertial frame”. That one is asked directly too.

Practice 1

Explain why a pupil sealed inside a windowless cabin, who drops a ball and watches it fall to the floor at 9.8 m s−2, cannot tell whether the cabin is resting on the surface of the Earth or accelerating through deep space. 2 marks

Answer
The effects of a uniform gravitational field and of uniform acceleration cannot be distinguished (1) (the equivalence principle) so every measurement made inside the sealed cabin gives the same result in both cases (1)
Concept 2

Spacetime, world lines and geodesics

Mass tells spacetime how to curve; the curve of spacetime tells matter how to move.

Spacetime is the three dimensions of space and one of time taken together as a single four-dimensional structure. An object’s path through it is its world line.

  • An object at rest has a vertical straight world line — time passes, but its position does not change.
  • An object at constant velocity has a straight sloping world line.
  • An accelerating object has a curved world line, because its velocity is changing.

Plot spacetime diagrams the way the exam does: time up the vertical axis, position across the horizontal axis.

World lines of a stationary, a constant-velocity and an accelerating object A spacetime diagram with time on the vertical axis in seconds and position on the horizontal axis in metres. The stationary object's world line is vertical, the constant-velocity object's is a straight sloping line, and the accelerating object's is a curve that becomes less steep as time increases. 0 position (m) time (s) stationary constant velocity accelerating
Time runs up the page and position across it, as in the exam papers. Straight means constant velocity; curved means accelerating.

A mass curves the spacetime around it. The more mass, and the more concentrated it is, the greater the curvature.

A geodesic is the shortest path between two points in that curved spacetime — and it is the path a freely moving object follows. So a planet is not being pulled off a straight line by a force; it is following the straightest path available through spacetime that the Sun’s mass has curved.

Two pieces of evidence you should be able to name: the precession of the perihelion of Mercury (its orbit slowly rotates, by more than Newtonian gravity predicts), and gravitational lensing (light from a distant galaxy is bent as it passes a massive object, so we see it stretched into arcs or rings).

A mass curving spacetime, and a geodesic across it A sheet representing spacetime sags where a mass sits on it. A path drawn across the sheet bends round the dip rather than running straight, showing the geodesic a freely moving object follows. spacetime mass geodesic — the path a free object takes
Mass curves spacetime, and a freely moving object runs along a geodesic in it — no sideways force required.
Practice 2

Describe the world line of an object that stays at rest, and explain how the world line of an object moving at constant velocity differs from that of an accelerating object. Time is on the vertical axis and position on the horizontal axis. 3 marks

Answer
At rest: a vertical straight line (1) (time passes but position does not change) Constant velocity: a straight sloping line (1) Accelerating: a curved line, because the velocity is changing (1)
Concept 3

Black holes and the Schwarzschild radius

Every mass has a Schwarzschild radius — the Earth included. What makes a black hole is being squeezed inside your own.

The Schwarzschild radius is the distance from the centre of a mass such that the escape velocity at that distance equals the speed of light. Equivalently, it is the distance from the centre of a mass to the event horizon. Either wording gets the mark.

The event horizon is the boundary at that radius. Nothing — not even light — can escape from inside it, so no information ever reaches us from within. At the very centre lies the singularity, where the mass is concentrated.

A mass becomes a black hole only when its physical radius shrinks to less than its own Schwarzschild radius. The Sun’s Schwarzschild radius is about 3 km and its actual radius is about 700 000 km, so it is nowhere near one — and an answer that says so must compare the two radii to score.

Singularity, event horizon and Schwarzschild radius A dark disc bounded by a dashed circle. The dashed circle is the event horizon. An arrow runs from the singularity at the centre out to the horizon, and that distance is the Schwarzschild radius. singularity rS event horizon nothing escapes from inside
The Schwarzschild radius rS is measured from the singularity out to the event horizon, drawn dashed because it is a boundary, not a surface.
Schwarzschild radius
rS = 2GM c2
the radius of the event horizon of a mass M
What each symbol means
SymbolQuantityUnit
rSSchwarzschild radiusm
Ggravitational constant, 6.67 × 10−11m3 kg−1 s−2
Mmass of the objectkg
cspeed of light, 3.00 × 108m s−1
Substitute & solve
Determine the Schwarzschild radius of a neutron star of mass 1.4 solar masses. (1 solar mass = 2.0 × 1030 kg) 3 marks
Convert first
M = 1.4 × 2.0 × 1030 solar masses → kg
M = 2.8 × 1030 kg
rS=2GM ÷ c2
rS=2 × 6.67 × 10−11 × 2.8 × 1030 ÷ (3.00 × 108)2numbers in
rS=3.74 × 1020 ÷ 9.00 × 1016square the c
rS=4.2 × 103 m
Rearrange — numbers in first
A black hole has a Schwarzschild radius of 1.2 × 104 m. Determine its mass. 3 marks
rS=2GM ÷ c2
1.2 × 104=2 × 6.67 × 10−11 × M ÷ (3.00 × 108)2numbers in first
1.2 × 104=1.482 × 10−27 × M
M=1.2 × 104 ÷ 1.482 × 10−27now rearrange
M=8.1 × 1030 kg
Practice 3

Calculate the Schwarzschild radius of a star of mass 15 solar masses. (1 solar mass = 2.0 × 1030 kg) 3 marks

Answer
M = 15 × 2.0 × 10³⁰ = 3.0 × 10³¹ kg (solar masses → kg) r_S = 2GM ÷ c² r_S = 2 × 6.67 × 10⁻¹¹ × 3.0 × 10³¹ ÷ (3.00 × 10⁸)² r_S = 4.00 × 10²¹ ÷ 9.00 × 10¹⁶ r_S = 4.4 × 10⁴ m
Watch out — the mark you keep losing

Clocks run at different rates in different gravitational fields: the weaker the field, the faster a clock runs. Three separate marking instructions punish the same habit here.

  • Say it as a rate. “Time passes faster” on its own is not accepted — it must refer to the rate at which time passes.
  • Always justify, and justify in terms of general relativity, because the GR effect dominates the SR one in these situations.
  • A correction stated as a bare negative number is not accepted — say what it is: “reduced by 39 µs per day”, not “−39 µs”.

Glossary

Every word on this page that the exam can ask you to define, with its picture.

Inertial frame of reference

A frame moving at constant velocity — it is not accelerating.

Non-inertial frame of reference

A frame that is accelerating with respect to an inertial frame.

=

Equivalence principle

It is not possible to distinguish between the effects on a body of uniform acceleration and a uniform gravitational field.

World line

The path an object takes through spacetime. Straight means constant velocity; curved means accelerating.

Geodesic

The shortest path between two points in curved spacetime — and the path a freely moving object follows.

Event horizon

The boundary at the Schwarzschild radius. Nothing, not even light, escapes from inside it.

Schwarzschild radius, rS

The distance from the centre of a mass at which the escape velocity equals the speed of light — the distance from the centre out to the event horizon.

Singularity

The point at the centre of a black hole where the mass is concentrated.

Check yourself

Mixed multiple choice

Exam-style multiple choice, 1 mark each.

Rate your confidence

Red = not yet, Amber = getting there, Green = confident. Saved on this device.

Sources & credits: notes and diagrams written and drawn by Mr Stewart. The linked class slides reproduce past-paper figures, questions and marking-instruction wording for educational use, © Qualifications Scotland (SQA), and name Institute of Physics Scotland and Perimeter Institute as the authors of material used in class. R Stewart - September 2026.