DP Physics Questionbank
Option A: Relativity (Core topics)
Description
Overview of essential ideas for this option.
A.1: Einstein’s study of electromagnetism revealed inconsistencies between the theory of Maxwell and Newton's mechanics. He recognized that both theories could not be reconciled and so choosing to trust Maxwell’s theory of electromagnetism he was forced to change long-cherished ideas about space and time in mechanics.
A.2: Observers in relative uniform motion disagree on the numerical values of space and time coordinates for events, but agree with the numerical value of the speed of light in a vacuum. The Lorentz transformation equations relate the values in one reference frame to those in another. These equations replace the Galilean transformation equations that fail for speeds close to that of light.
A.3: Spacetime diagrams are a very clear and illustrative way to show graphically how different observers in relative motion to each other have measurements that differ from each other.
Directly related questions
- 16N.3.SL.TZ0.5c: In the pion reference frame, the Earth moves a distance X before the pion decays. In the Earth...
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16N.3.SL.TZ0.5b:
A charged pion decays spontaneously in a time of 26 ns as measured in the frame of reference in which it is stationary. The pion moves with a velocity of 0.96c relative to the Earth. Calculate the pion’s lifetime as measured by an observer on the Earth.
- 16N.3.SL.TZ0.6b: Draw, on the diagram, the x′-axis for the reference frame of S.
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16N.3.SL.TZ0.4b:
In the reference frame of the laboratory the force on X is magnetic.
(i) State the nature of the force acting on X in this reference frame where X is at rest.
(ii) Explain how this force arises.
- 16N.3.SL.TZ0.5a: Define proper length.
- 16N.3.SL.TZ0.7c: Draw, for the reference frame of twin A, a spacetime diagram that represents the worldlines for...
- 16N.3.SL.TZ0.7d: Suggest how the twin paradox arises and how it is resolved.
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16N.3.SL.TZ0.6a:
Calculate the angle between the worldline of S and the worldline of the Earth.
- 16N.3.SL.TZ0.6c: An event Z is shown on the diagram. Label the co-ordinates of this event in the reference frame...
- 16N.3.SL.TZ0.4a: Define frame of reference.
- 16N.3.SL.TZ0.7a: Calculate the time taken for the journey in the reference frame of twin A as measured on Earth.
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16N.3.SL.TZ0.7b:
Determine the time taken for the journey in the reference frame of twin B.
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17M.3.SL.TZ1.4b:
Calculate the speed v of the train for the ratio .
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17M.3.SL.TZ1.4d.i:
Draw the time and space axes for observer P’s reference frame on the spacetime diagram.
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17M.3.SL.TZ1.4d.ii:
Deduce, using the spacetime diagram, which light was turned on first according to observer P.
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17M.3.SL.TZ1.4e:
A second train is moving at a velocity of –0.70c with respect to the ground.
Calculate the speed of the second train relative to observer P.
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17M.3.SL.TZ1.4c:
Later the train is travelling at a speed of 0.60c. Observer P measures the length of the train to be 125 m. The train enters a tunnel of length 100 m according to observer Q.
Show that the length of the train according to observer Q is 100 m.
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17M.3.SL.TZ1.4d.iv:
Demonstrate that the spacetime interval between events B and F is invariant.
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17M.3.SL.TZ1.3a:
State what is meant by a reference frame.
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17M.3.SL.TZ1.3b.i:
State and explain whether the force experienced by P is magnetic, electric or both, in reference frame S.
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17M.3.SL.TZ1.3b.ii:
State and explain whether the force experienced by P is magnetic, electric or both, in the rest frame of P.
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17M.3.SL.TZ1.4a:
State which of the two time intervals is a proper time.
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17M.3.SL.TZ1.4d.iii:
Apply a Lorentz transformation to show that the time difference between events B and F according to observer P is 2.5 × 10–7 s.
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17M.3.SL.TZ2.5c.ii:
State and explain whether the ct coordinate in (c)(i) is less than, equal to or greater than 1.0 m.
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17M.3.SL.TZ2.3a:
State one prediction of Maxwell’s theory of electromagnetism that is consistent with special relativity.
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17M.3.SL.TZ2.3b:
A current is established in a long straight wire that is at rest in a laboratory.
A proton is at rest relative to the laboratory and the wire.
Observer X is at rest in the laboratory. Observer Y moves to the right with constant speed relative to the laboratory. Compare and contrast how observer X and observer Y account for any non-gravitational forces on the proton.
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17M.3.SL.TZ2.5a.i:
Calculate the length of the rocket according to X.
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17M.3.SL.TZ2.4:
Muons are unstable particles with a proper lifetime of 2.2 μs. Muons are produced 2.0 km above ground and move downwards at a speed of 0.98c relative to the ground. For this speed = 5.0. Discuss, with suitable calculations, how this experiment provides evidence for time dilation.
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17M.3.SL.TZ2.5a.ii:
A space shuttle is released from the rocket. The shuttle moves with speed 0.20c to the right according to X. Calculate the velocity of the shuttle relative to the rocket.
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17M.3.SL.TZ2.5b.i:
the time interval between the lamps turning on.
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17M.3.SL.TZ2.5b.ii:
which lamp turns on first.
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17M.3.SL.TZ2.5c.i:
On the diagram label the coordinates x and ct.
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17M.3.SL.TZ2.5c.iii:
Calculate the value of c 2t 2 – x 2.
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20N.3.SL.TZ0.4b(i):
Deduce the length of the probe as measured by an observer in the spaceship.
- 20N.3.SL.TZ0.3c(i): Identify the nature of the attractive force recorded by an observer stationary with respect to...
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20N.3.SL.TZ0.5a(ii):
Draw the axis for the reference frame of spaceship A.
- 20N.3.SL.TZ0.3a: Maxwell’s equations led to the constancy of the speed of light. Identify what Maxwell’s equations...
- 20N.3.SL.TZ0.3b: State a postulate that is the same for both special relativity and Galilean relativity.
- 20N.3.SL.TZ0.3c(ii): A second observer moves at the drift velocity of the electron current in the wires. Discuss how...
- 20N.3.SL.TZ0.4a: The Lorentz transformations assume that the speed of light is constant. Outline what the Galilean...
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20N.3.SL.TZ0.4b(ii):
Explain which of the lengths is the proper length.
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20N.3.SL.TZ0.5a(i):
Calculate in terms of the velocity of spaceship A relative to observer O.
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20N.3.SL.TZ0.5b(ii):
Determine the time, according to spaceship A, when light from event E was observed on spaceship A.
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20N.1.SL.TZ0.4c:
Calculate the speed of the probe in terms of , relative to Earth.
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20N.3.SL.TZ0.5b(i):
Plot the event E on the spacetime diagram and label it E.
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20N.3.SL.TZ0.4c:
Calculate the speed of the probe in terms of , relative to Earth.
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17N.3.SL.TZ0.5c:
Identify the terms in the formula.
u′ =
- 17N.3.SL.TZ0.4: Outline the conclusion from Maxwell’s work on electromagnetism that led to one of the postulates...
- 17N.3.SL.TZ0.5a: Define frame of reference.
- 17N.3.SL.TZ0.5b: Calculate, according to the observer on Earth, the time taken for A and B to meet.
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17N.3.SL.TZ0.5d:
Determine, according to an observer in A, the velocity of B.
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17N.3.SL.TZ0.5e.i:
Determine, according to an observer in A, the time taken for B to meet A.
- 17N.3.SL.TZ0.5e.ii: Deduce, without further calculation, how the time taken for A to meet B, according to an observer...
- 17N.3.SL.TZ0.6b: Draw a spacetime diagram for this situation according to an observer at rest relative to the tunnel.
- 17N.3.SL.TZ0.6c: Calculate the velocity of the train, according to an observer at rest relative to the tunnel, at...
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17N.3.SL.TZ0.6d:
For an observer on the train, it is the tunnel that is moving and therefore will appear length contracted. This seems to contradict the observation made by the observer at rest to the tunnel, creating a paradox. Explain how this paradox is resolved. You may refer to your spacetime diagram in (b).
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18M.3.SL.TZ1.4a.i:
Calculate, according to Galilean relativity, the time taken for a muon to travel to the ground.
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18M.3.SL.TZ1.4b.ii:
Discuss how your result in (b)(i) and the outcome of the muon decay experiment support the theory of special relativity.
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18M.3.SL.TZ1.5b:
Deduce, showing your working on the spacetime diagram, the value of ct according to the Earth observer at which the rocket B emitted its flash of light.
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18M.3.SL.TZ1.5a:
Draw on the spacetime diagram the worldline of B according to the Earth observer and label it B.
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18M.3.SL.TZ1.3a:
State whether the field around the wire according to observer X is electric, magnetic or a combination of both.
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18M.3.SL.TZ1.5c:
Explain whether or not the arrival times of the two flashes in the Earth frame are simultaneous events in the frame of rocket A.
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18M.3.SL.TZ1.5d:
Calculate the velocity of rocket B relative to rocket A.
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18M.3.SL.TZ1.3b.ii:
Deduce whether the overall field around the wire is electric, magnetic or a combination of both according to observer Y.
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18M.3.SL.TZ1.4b.i:
Calculate, according to the theory of special relativity, the time taken for a muon to reach the ground in the reference frame of the muon.
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18M.3.SL.TZ1.3b.i:
Discuss the change in d according to observer Y.
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18M.3.SL.TZ1.4a.ii:
Deduce why only a small fraction of the total number of muons created is expected to be detected at ground level according to Galilean relativity.
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18M.3.SL.TZ2.4a:
Calculate the velocity of the spaceship relative to the Earth.
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18M.3.SL.TZ2.3a.i:
Calculate, for the reference frame of rocket A, the speed of rocket B according to the Galilean transformation.
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18M.3.SL.TZ2.3a.ii:
Calculate, for the reference frame of rocket A, the speed of rocket B according to the Lorentz transformation.
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18M.3.SL.TZ2.3b:
Outline, with reference to special relativity, which of your calculations in (a) is more likely to be valid.
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18M.3.SL.TZ2.4b:
The spaceship passes the space station 90 minutes later as measured by the spaceship clock. Determine, for the reference frame of the Earth, the distance between the Earth and the space station.
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18M.3.SL.TZ2.4c:
As the spaceship passes the space station, the space station sends a radio signal back to the Earth. The reception of this signal at the Earth is event A. Determine the time on the Earth clock when event A occurs.
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18M.3.SL.TZ2.4d.i:
Construct event A and event B on the spacetime diagram.
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18M.3.SL.TZ2.4d.ii:
Estimate, using the spacetime diagram, the time at which event B occurs for the spaceship.
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18M.3.SL.TZ2.5b.i:
calculate the spacetime interval.
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18M.3.SL.TZ2.5a:
Explain what is meant by the statement that the spacetime interval is an invariant quantity.
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18M.3.SL.TZ2.5b.ii:
determine the time between them according to observer B.
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18M.3.SL.TZ2.5c:
Outline why the observed times are different for A and B.
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18N.3.SL.TZ0.5a.ii:
ct′ = –1.1 m.
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18N.3.SL.TZ0.4b.ii:
Determine the time it takes the probe to reach the front of the rocket according to an observer at rest on the ground.
- 18N.3.SL.TZ0.5b.i: Label, on the diagram, the space coordinate of event E in the S′ frame. Label this event with the...
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18N.3.SL.TZ0.5a.i:
x′ = 1.5 m.
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18N.3.SL.TZ0.3b.i:
explain why the time coordinate of E in frame S is .
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18N.3.SL.TZ0.4b.i:
Determine the time it takes the probe to reach the front of the rocket according to an observer at rest in the rocket.
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18N.3.SL.TZ0.3b.ii:
hence show that the space coordinate of E in frame S is .
- 18N.3.SL.TZ0.5c.i: Using the spacetime diagram, outline without calculation, why observers in frame S′ measure the...
- 18N.3.SL.TZ0.3a: State what is meant by a reference frame.
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18N.3.SL.TZ0.5b.ii:
Label, on the diagram, the event that has coordinates x′ = 1.0 m and ct′ = 0. Label this event with the letter Q.
- 18N.3.SL.TZ0.5c.ii: Using the spacetime diagram, estimate, in m, the length of this rod in the S′ frame.
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18N.3.SL.TZ0.4a:
Calculate the speed of the probe relative to the ground.
- 19M.3.SL.TZ2.5b: Explain why there is no magnetic force on each proton in its own rest frame.
- 19M.3.SL.TZ2.5c: Explain why there must be a resultant repulsive force on the protons in all reference frames.
- 19M.3.SL.TZ2.4ai: Define an inertial reference frame.
- 19M.3.SL.TZ2.5a: Outline why there is an attractive magnetic force on each proton in the laboratory frame.
- 19M.3.SL.TZ2.4aii: As the spaceship passes the Earth it emits a flash of light that travels in the same direction as...
- 19M.3.SL.TZ2.6bii: In the reference frame of the train a ball travels with speed 0.50c from the back to the front of...
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19M.3.SL.TZ2.4b:
Use your answer to (a)(ii) to describe the paradigm shift that Einstein’s theory of special relativity produced.
- 19M.3.SL.TZ2.6bi: In the reference frame of the train a ball travels with speed 0.50c from the back to the front of...
- 19M.3.SL.TZ2.6a: Define proper length.
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19M.3.SL.TZ2.7b:
Label, with the letter E, the event of the spaceship going past the planet.
- 19M.3.SL.TZ2.7cii: Determine, according to an observer on the spaceship as the spaceship passes the planet, the time...
- 19M.3.SL.TZ2.7d: On passing the planet a probe containing the spaceship’s clock and an astronaut is sent back to...
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19M.3.SL.TZ2.7a:
Show, using the spacetime diagram, that the speed of the spaceship relative to the Earth is 0.80c.
- 19M.3.SL.TZ2.7ci: Determine, according to an observer on the spaceship as the spaceship passes the planet, the time...
- 19M.3.SL.TZ1.3a: State the speed of the flash of light according to an observer on the ground using Galilean...
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19M.3.SL.TZ1.5d.ii:
Using the spacetime diagram, determine which event occurred first for the spacecraft observer, event 1 or event 2.
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19M.3.SL.TZ1.5c:
Show that the value of the invariant spacetime interval between events 1 and 2 is 9600 ly2.
- 19M.3.SL.TZ1.5a: Plot, on the axes, the point corresponding to event 2.
- 19M.3.SL.TZ1.3c: State the speed of the flash of light according to an observer on the ground using Einstein’s...
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19M.3.SL.TZ1.5b:
Suggest whether the rocket launched by the spacecraft might be the cause of the explosion of the asteroid.
- 19M.3.SL.TZ1.5d.i: An observer in the spacecraft measures that events 1 and 2 are a distance of 120 ly apart....
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19M.3.SL.TZ1.4b:
Demonstrate how an observer moving with the same velocity as the muons accounts for the answer to (a)(ii).
- 19M.3.SL.TZ1.3b: State the speed of the flash of light according to an observer on the ground using Maxwell’s...
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19M.3.SL.TZ1.4a.ii:
Estimate in the Earth frame the fraction of the original muons that will reach the Earth’s surface before decaying according to special relativity.
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19M.3.SL.TZ1.4a.i:
Estimate in the Earth frame the fraction of the original muons that will reach the Earth’s surface before decaying according to Newtonian mechanics.
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19M.3.SL.TZ1.5e:
Determine, using the diagram, the speed of the spacecraft relative to the galaxy.
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19N.3.SL.TZ0.3b(iv):
The velocity of P is 0.30c relative to the laboratory. A second particle Q moves at a velocity of 0.80c relative to the laboratory.
Calculate the speed of Q relative to P.
- 19N.3.SL.TZ0.4b: Outline why LB is the proper length of the bridge.
- 19N.3.SL.TZ0.4c(ii): Demonstrate using the diagram which lamp, according to observer A, was turned on first.
- 19N.3.SL.TZ0.3a: One of the two postulates of special relativity states that the speed of light in a vacuum is the...
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19N.3.SL.TZ0.4a(i):
Calculate, for observer A, the length LA of the bridge
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19N.3.SL.TZ0.4a(ii):
Calculate, for observer A, the time taken to cross the bridge.
- 19N.3.SL.TZ0.3b(i): State the nature of the force on the particle P in the reference frame of the laboratory.
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19N.3.SL.TZ0.3b(iii):
Explain how the force in part (b)(ii) arises.
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19N.3.SL.TZ0.3b(ii):
Deduce, using your answer to part (a), the nature of the force that acts on the particle P in the rest frame of P.
- 19N.3.SL.TZ0.4c(iii): Demonstrate, using the diagram, which lamp observer A observes to light first.
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19N.3.SL.TZ0.4c(iv):
Determine the time, according to observer A, between X and Y.
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19N.3.SL.TZ0.4c(i):
Draw, on the spacetime diagram, the space axis for the reference frame of observer A. Label this axis '.
Sub sections and their related questions
A.1 – The beginnings of relativity
- 16N.3.SL.TZ0.4a: Define frame of reference.
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16N.3.SL.TZ0.4b:
In the reference frame of the laboratory the force on X is magnetic.
(i) State the nature of the force acting on X in this reference frame where X is at rest.
(ii) Explain how this force arises.
-
17M.3.SL.TZ1.3a:
State what is meant by a reference frame.
-
17M.3.SL.TZ1.3b.i:
State and explain whether the force experienced by P is magnetic, electric or both, in reference frame S.
-
17M.3.SL.TZ1.3b.ii:
State and explain whether the force experienced by P is magnetic, electric or both, in the rest frame of P.
-
17M.3.SL.TZ2.3a:
State one prediction of Maxwell’s theory of electromagnetism that is consistent with special relativity.
-
17M.3.SL.TZ2.3b:
A current is established in a long straight wire that is at rest in a laboratory.
A proton is at rest relative to the laboratory and the wire.
Observer X is at rest in the laboratory. Observer Y moves to the right with constant speed relative to the laboratory. Compare and contrast how observer X and observer Y account for any non-gravitational forces on the proton.
- 17N.3.SL.TZ0.4: Outline the conclusion from Maxwell’s work on electromagnetism that led to one of the postulates...
-
18M.3.SL.TZ1.3a:
State whether the field around the wire according to observer X is electric, magnetic or a combination of both.
-
18M.3.SL.TZ1.3b.ii:
Deduce whether the overall field around the wire is electric, magnetic or a combination of both according to observer Y.
-
18M.3.SL.TZ1.4a.i:
Calculate, according to Galilean relativity, the time taken for a muon to travel to the ground.
-
18M.3.SL.TZ1.4a.ii:
Deduce why only a small fraction of the total number of muons created is expected to be detected at ground level according to Galilean relativity.
-
18M.3.SL.TZ2.3a.i:
Calculate, for the reference frame of rocket A, the speed of rocket B according to the Galilean transformation.
- 18N.3.SL.TZ0.3a: State what is meant by a reference frame.
-
18N.3.SL.TZ0.3b.i:
explain why the time coordinate of E in frame S is .
-
18N.3.SL.TZ0.3b.ii:
hence show that the space coordinate of E in frame S is .
-
18N.3.SL.TZ0.4b.i:
Determine the time it takes the probe to reach the front of the rocket according to an observer at rest in the rocket.
- 19M.3.SL.TZ2.4ai: Define an inertial reference frame.
- 19M.3.SL.TZ2.4aii: As the spaceship passes the Earth it emits a flash of light that travels in the same direction as...
-
19M.3.SL.TZ2.4b:
Use your answer to (a)(ii) to describe the paradigm shift that Einstein’s theory of special relativity produced.
- 19M.3.SL.TZ2.5a: Outline why there is an attractive magnetic force on each proton in the laboratory frame.
- 19M.3.SL.TZ2.5b: Explain why there is no magnetic force on each proton in its own rest frame.
- 19M.3.SL.TZ2.5c: Explain why there must be a resultant repulsive force on the protons in all reference frames.
- 19M.3.SL.TZ1.3a: State the speed of the flash of light according to an observer on the ground using Galilean...
- 19M.3.SL.TZ1.3b: State the speed of the flash of light according to an observer on the ground using Maxwell’s...
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19M.3.SL.TZ1.4a.i:
Estimate in the Earth frame the fraction of the original muons that will reach the Earth’s surface before decaying according to Newtonian mechanics.
- 19N.3.SL.TZ0.3b(i): State the nature of the force on the particle P in the reference frame of the laboratory.
-
19N.3.SL.TZ0.3b(ii):
Deduce, using your answer to part (a), the nature of the force that acts on the particle P in the rest frame of P.
-
19N.3.SL.TZ0.3b(iii):
Explain how the force in part (b)(ii) arises.
- 20N.3.SL.TZ0.3a: Maxwell’s equations led to the constancy of the speed of light. Identify what Maxwell’s equations...
- 20N.3.SL.TZ0.3b: State a postulate that is the same for both special relativity and Galilean relativity.
- 20N.3.SL.TZ0.3c(i): Identify the nature of the attractive force recorded by an observer stationary with respect to...
- 20N.3.SL.TZ0.3c(ii): A second observer moves at the drift velocity of the electron current in the wires. Discuss how...
- 20N.3.SL.TZ0.4a: The Lorentz transformations assume that the speed of light is constant. Outline what the Galilean...
A.2 – Lorentz transformations
- 16N.3.SL.TZ0.5a: Define proper length.
-
16N.3.SL.TZ0.5b:
A charged pion decays spontaneously in a time of 26 ns as measured in the frame of reference in which it is stationary. The pion moves with a velocity of 0.96c relative to the Earth. Calculate the pion’s lifetime as measured by an observer on the Earth.
- 16N.3.SL.TZ0.5c: In the pion reference frame, the Earth moves a distance X before the pion decays. In the Earth...
-
17M.3.SL.TZ1.4a:
State which of the two time intervals is a proper time.
-
17M.3.SL.TZ1.4b:
Calculate the speed v of the train for the ratio .
-
17M.3.SL.TZ1.4c:
Later the train is travelling at a speed of 0.60c. Observer P measures the length of the train to be 125 m. The train enters a tunnel of length 100 m according to observer Q.
Show that the length of the train according to observer Q is 100 m.
-
17M.3.SL.TZ1.4d.iii:
Apply a Lorentz transformation to show that the time difference between events B and F according to observer P is 2.5 × 10–7 s.
-
17M.3.SL.TZ1.4d.iv:
Demonstrate that the spacetime interval between events B and F is invariant.
-
17M.3.SL.TZ1.4e:
A second train is moving at a velocity of –0.70c with respect to the ground.
Calculate the speed of the second train relative to observer P.
-
17M.3.SL.TZ2.4:
Muons are unstable particles with a proper lifetime of 2.2 μs. Muons are produced 2.0 km above ground and move downwards at a speed of 0.98c relative to the ground. For this speed = 5.0. Discuss, with suitable calculations, how this experiment provides evidence for time dilation.
-
17M.3.SL.TZ2.5a.i:
Calculate the length of the rocket according to X.
-
17M.3.SL.TZ2.5a.ii:
A space shuttle is released from the rocket. The shuttle moves with speed 0.20c to the right according to X. Calculate the velocity of the shuttle relative to the rocket.
-
17M.3.SL.TZ2.5b.i:
the time interval between the lamps turning on.
-
17M.3.SL.TZ2.5b.ii:
which lamp turns on first.
-
17M.3.SL.TZ2.5c.iii:
Calculate the value of c 2t 2 – x 2.
- 17N.3.SL.TZ0.5a: Define frame of reference.
- 17N.3.SL.TZ0.5b: Calculate, according to the observer on Earth, the time taken for A and B to meet.
-
17N.3.SL.TZ0.5c:
Identify the terms in the formula.
u′ =
-
17N.3.SL.TZ0.5d:
Determine, according to an observer in A, the velocity of B.
-
17N.3.SL.TZ0.5e.i:
Determine, according to an observer in A, the time taken for B to meet A.
- 17N.3.SL.TZ0.5e.ii: Deduce, without further calculation, how the time taken for A to meet B, according to an observer...
-
18M.3.SL.TZ1.3b.i:
Discuss the change in d according to observer Y.
-
18M.3.SL.TZ1.4b.i:
Calculate, according to the theory of special relativity, the time taken for a muon to reach the ground in the reference frame of the muon.
-
18M.3.SL.TZ1.4b.ii:
Discuss how your result in (b)(i) and the outcome of the muon decay experiment support the theory of special relativity.
-
18M.3.SL.TZ1.5c:
Explain whether or not the arrival times of the two flashes in the Earth frame are simultaneous events in the frame of rocket A.
-
18M.3.SL.TZ1.5d:
Calculate the velocity of rocket B relative to rocket A.
-
18M.3.SL.TZ2.3a.ii:
Calculate, for the reference frame of rocket A, the speed of rocket B according to the Lorentz transformation.
-
18M.3.SL.TZ2.3b:
Outline, with reference to special relativity, which of your calculations in (a) is more likely to be valid.
-
18M.3.SL.TZ2.4a:
Calculate the velocity of the spaceship relative to the Earth.
-
18M.3.SL.TZ2.4b:
The spaceship passes the space station 90 minutes later as measured by the spaceship clock. Determine, for the reference frame of the Earth, the distance between the Earth and the space station.
-
18M.3.SL.TZ2.4c:
As the spaceship passes the space station, the space station sends a radio signal back to the Earth. The reception of this signal at the Earth is event A. Determine the time on the Earth clock when event A occurs.
-
18M.3.SL.TZ2.5a:
Explain what is meant by the statement that the spacetime interval is an invariant quantity.
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18M.3.SL.TZ2.5b.i:
calculate the spacetime interval.
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18M.3.SL.TZ2.5b.ii:
determine the time between them according to observer B.
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18M.3.SL.TZ2.5c:
Outline why the observed times are different for A and B.
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18N.3.SL.TZ0.4a:
Calculate the speed of the probe relative to the ground.
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18N.3.SL.TZ0.4b.ii:
Determine the time it takes the probe to reach the front of the rocket according to an observer at rest on the ground.
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18N.3.SL.TZ0.5a.i:
x′ = 1.5 m.
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18N.3.SL.TZ0.5a.ii:
ct′ = –1.1 m.
- 18N.3.SL.TZ0.5c.i: Using the spacetime diagram, outline without calculation, why observers in frame S′ measure the...
- 18N.3.SL.TZ0.5c.ii: Using the spacetime diagram, estimate, in m, the length of this rod in the S′ frame.
- 19M.3.SL.TZ2.6a: Define proper length.
- 19M.3.SL.TZ2.6bi: In the reference frame of the train a ball travels with speed 0.50c from the back to the front of...
- 19M.3.SL.TZ2.6bii: In the reference frame of the train a ball travels with speed 0.50c from the back to the front of...
- 19M.3.SL.TZ2.7ci: Determine, according to an observer on the spaceship as the spaceship passes the planet, the time...
- 19M.3.SL.TZ2.7cii: Determine, according to an observer on the spaceship as the spaceship passes the planet, the time...
- 19M.3.SL.TZ1.3c: State the speed of the flash of light according to an observer on the ground using Einstein’s...
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19M.3.SL.TZ1.4a.ii:
Estimate in the Earth frame the fraction of the original muons that will reach the Earth’s surface before decaying according to special relativity.
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19M.3.SL.TZ1.4b:
Demonstrate how an observer moving with the same velocity as the muons accounts for the answer to (a)(ii).
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19M.3.SL.TZ1.5c:
Show that the value of the invariant spacetime interval between events 1 and 2 is 9600 ly2.
- 19N.3.SL.TZ0.3a: One of the two postulates of special relativity states that the speed of light in a vacuum is the...
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19N.3.SL.TZ0.3b(iii):
Explain how the force in part (b)(ii) arises.
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19N.3.SL.TZ0.3b(iv):
The velocity of P is 0.30c relative to the laboratory. A second particle Q moves at a velocity of 0.80c relative to the laboratory.
Calculate the speed of Q relative to P.
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19N.3.SL.TZ0.4a(i):
Calculate, for observer A, the length LA of the bridge
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19N.3.SL.TZ0.4a(ii):
Calculate, for observer A, the time taken to cross the bridge.
- 19N.3.SL.TZ0.4b: Outline why LB is the proper length of the bridge.
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19N.3.SL.TZ0.4c(iv):
Determine the time, according to observer A, between X and Y.
- 20N.3.SL.TZ0.3b: State a postulate that is the same for both special relativity and Galilean relativity.
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20N.3.SL.TZ0.4b(i):
Deduce the length of the probe as measured by an observer in the spaceship.
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20N.3.SL.TZ0.4b(ii):
Explain which of the lengths is the proper length.
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20N.1.SL.TZ0.4c:
Calculate the speed of the probe in terms of , relative to Earth.
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20N.3.SL.TZ0.4c:
Calculate the speed of the probe in terms of , relative to Earth.
A.3 – Spacetime diagrams
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16N.3.SL.TZ0.6a:
Calculate the angle between the worldline of S and the worldline of the Earth.
- 16N.3.SL.TZ0.6b: Draw, on the diagram, the x′-axis for the reference frame of S.
- 16N.3.SL.TZ0.6c: An event Z is shown on the diagram. Label the co-ordinates of this event in the reference frame...
- 16N.3.SL.TZ0.7a: Calculate the time taken for the journey in the reference frame of twin A as measured on Earth.
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16N.3.SL.TZ0.7b:
Determine the time taken for the journey in the reference frame of twin B.
- 16N.3.SL.TZ0.7c: Draw, for the reference frame of twin A, a spacetime diagram that represents the worldlines for...
- 16N.3.SL.TZ0.7d: Suggest how the twin paradox arises and how it is resolved.
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17M.3.SL.TZ1.4d.i:
Draw the time and space axes for observer P’s reference frame on the spacetime diagram.
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17M.3.SL.TZ1.4d.ii:
Deduce, using the spacetime diagram, which light was turned on first according to observer P.
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17M.3.SL.TZ2.5c.i:
On the diagram label the coordinates x and ct.
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17M.3.SL.TZ2.5c.ii:
State and explain whether the ct coordinate in (c)(i) is less than, equal to or greater than 1.0 m.
- 17N.3.SL.TZ0.6b: Draw a spacetime diagram for this situation according to an observer at rest relative to the tunnel.
- 17N.3.SL.TZ0.6c: Calculate the velocity of the train, according to an observer at rest relative to the tunnel, at...
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17N.3.SL.TZ0.6d:
For an observer on the train, it is the tunnel that is moving and therefore will appear length contracted. This seems to contradict the observation made by the observer at rest to the tunnel, creating a paradox. Explain how this paradox is resolved. You may refer to your spacetime diagram in (b).
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18M.3.SL.TZ1.5a:
Draw on the spacetime diagram the worldline of B according to the Earth observer and label it B.
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18M.3.SL.TZ1.5b:
Deduce, showing your working on the spacetime diagram, the value of ct according to the Earth observer at which the rocket B emitted its flash of light.
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18M.3.SL.TZ2.4d.i:
Construct event A and event B on the spacetime diagram.
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18M.3.SL.TZ2.4d.ii:
Estimate, using the spacetime diagram, the time at which event B occurs for the spaceship.
- 18N.3.SL.TZ0.5b.i: Label, on the diagram, the space coordinate of event E in the S′ frame. Label this event with the...
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18N.3.SL.TZ0.5b.ii:
Label, on the diagram, the event that has coordinates x′ = 1.0 m and ct′ = 0. Label this event with the letter Q.
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19M.3.SL.TZ2.7a:
Show, using the spacetime diagram, that the speed of the spaceship relative to the Earth is 0.80c.
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19M.3.SL.TZ2.7b:
Label, with the letter E, the event of the spaceship going past the planet.
- 19M.3.SL.TZ2.7d: On passing the planet a probe containing the spaceship’s clock and an astronaut is sent back to...
- 19M.3.SL.TZ1.5a: Plot, on the axes, the point corresponding to event 2.
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19M.3.SL.TZ1.5b:
Suggest whether the rocket launched by the spacecraft might be the cause of the explosion of the asteroid.
- 19M.3.SL.TZ1.5d.i: An observer in the spacecraft measures that events 1 and 2 are a distance of 120 ly apart....
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19M.3.SL.TZ1.5d.ii:
Using the spacetime diagram, determine which event occurred first for the spacecraft observer, event 1 or event 2.
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19M.3.SL.TZ1.5e:
Determine, using the diagram, the speed of the spacecraft relative to the galaxy.
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19N.3.SL.TZ0.4c(i):
Draw, on the spacetime diagram, the space axis for the reference frame of observer A. Label this axis '.
- 19N.3.SL.TZ0.4c(ii): Demonstrate using the diagram which lamp, according to observer A, was turned on first.
- 19N.3.SL.TZ0.4c(iii): Demonstrate, using the diagram, which lamp observer A observes to light first.
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20N.3.SL.TZ0.5a(i):
Calculate in terms of the velocity of spaceship A relative to observer O.
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20N.3.SL.TZ0.5a(ii):
Draw the axis for the reference frame of spaceship A.
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20N.3.SL.TZ0.5b(i):
Plot the event E on the spacetime diagram and label it E.
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20N.3.SL.TZ0.5b(ii):
Determine the time, according to spaceship A, when light from event E was observed on spaceship A.