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PU-105 / L09 · lecture

Resolving the Paradoxes: Twins, Pole and Barn

~9 min read · Tier toggle changes depth (T1 plain · T2 standard · T3 rigour)

BEFORE YOU START

You must be comfortable with the Lorentz transformation, the definition of the Lorentz factor \(\gamma\), and the basic statements of time dilation and length contraction. Familiarity with inertial frames and the standard configuration is assumed.

Why this matters

Special relativity often feels like a collection of counter-intuitive tricks, but the "paradoxes" are actually tests of our ability to apply the geometry of spacetime consistently.

The twin paradox and the pole-barn paradox are not contradictions in the theory; they are failures of our classical intuition about simultaneity. By resolving them, we demonstrate that time dilation and length contraction are not optical illusions or mechanical effects, but fundamental properties of the spacetime interval. Understanding these scenarios is crucial because they force us to abandon the absolute notion of "now" and accept that different observers slice spacetime into space and time differently. This lecture bridges the gap between the mathematical formalism of the Lorentz transformation and the physical reality experienced by observers in relative motion.

The Geometry of Disagreement

Imagine two friends, Alice and Bob, who are initially together. Alice stays on Earth, while Bob travels in a spaceship at a constant high speed to a distant star and then returns. When they reunite, Alice notices that Bob is younger than she is. This is the twin paradox. The "paradox" arises because, from Bob's perspective during the outbound leg, it seems like Alice is the one moving, so Alice should be the one aging slower. If both see the other as moving, why is only Bob younger?

The resolution lies in the fact that the situation is not symmetric. Bob changes inertial frames when he turns around, while Alice remains in a single inertial frame (approximately). In the geometry of spacetime, the path taken by Bob is not a straight line in the spacetime diagram; it is bent. The straightest path between two events in spacetime (the inertial path) is actually the one that maximizes the proper time, whereas the bent path (the accelerated one) has less proper time. Thus the "paradox" is resolved by noting that the twins follow different worldlines between the same two events: only Alice's is straight (inertial), and the straight worldline is the one with the most proper time. The key is not just who is moving, but who changes their state of motion.

The Twin Paradox: Proper Time and Frame Switching

To resolve the twin paradox quantitatively, we must calculate the proper time \(\Delta\tau\) experienced by each twin. Proper time is the time measured by a clock that is present at both events. For an inertial observer, the proper time is simply the coordinate time in their rest frame. For a moving observer, we use the time dilation result from D-093.

Let the distance to the star be \(L\) in Alice's frame \(S\). Bob travels at speed \(v\). The time for the round trip in Alice's frame is \(\Delta t_A = 2L/v\). Since Alice is at rest in \(S\), her proper time is \(\Delta\tau_A = \Delta t_A\). For Bob, the time in his frame for each leg is dilated. However, a more robust method is to use the invariant interval. The proper time for Bob is given by \(\Delta\tau_B = \int \sqrt{1 - v^2/c^2} \, dt\). Since \(v\) is constant during the legs, \(\Delta\tau_B = \Delta t_A / \gamma\). Since \(\gamma > 1\), \(\Delta\tau_B < \Delta\tau_A\). Bob ages less. The apparent symmetry is broken by Bob's acceleration at the turnaround point, which changes his inertial frame and thus his definition of simultaneity.

\[ \Delta\tau_B = \frac{\Delta t_A}{\gamma} = \Delta t_A \sqrt{1 - \frac{v^2}{c^2}} \]

The Pole and Barn: Simultaneity is Relative

Consider a pole of proper length \(L_0\) moving at speed \(v\) towards a barn of proper length \(L_{\text{barn}}\). Suppose \(L_0 > L_{\text{barn}}\), so the pole is longer than the barn in its rest frame. However, due to length contraction (D-094), the pole's length in the barn's frame is \(L = L_0/\gamma\). If \(v\) is high enough such that \(L < L_{\text{barn}}\), an observer in the barn's frame sees the pole fit inside the barn. They can close the front and back doors simultaneously and trap the pole inside.

From the pole's frame, the barn is moving and is length-contracted to \(L_{\text{barn}}/\gamma\). Since \(L_0 > L_{\text{barn}}\), the barn is even shorter than the pole. How can the pole fit? The resolution is the relativity of simultaneity (D-092). The events "close front door" and "close back door" are simultaneous in the barn's frame but not in the pole's frame. In the pole's frame, the front door closes first, then the pole passes through, and then the back door closes. The pole never fits inside the barn in its own frame, but it is not broken because the doors do not close at the same time in that frame. The "fitting" is a frame-dependent description of the same set of spacetime events.

\[ \Delta t' = -\gamma \frac{v \Delta x}{c^2} \]

Consistency of the Lorentz Transformation

Both paradoxes highlight that length contraction and time dilation are not independent phenomena but are linked by the relativity of simultaneity. The Lorentz transformation mixes space and time coordinates. When we measure the length of a moving object, we must measure the positions of its ends at the same time in our frame. But "same time" is not invariant. This is why the pole-barn paradox works: the definition of "length" depends on the simultaneity of the endpoint measurements. Similarly, in the twin paradox, the comparison of ages depends on the proper time along the worldlines, which is invariant, but the intermediate comparisons of "current age" depend on the observer's frame and their notion of simultaneity. The physics is consistent because the spacetime interval \(ds^2 = c^2 dt^2 - dx^2\) is invariant for all observers.

The derivations

◆ DERIVATION EMBED · D-093 · not re-derived here

Time Dilation

Let a single ideal clock be at rest at a fixed spatial point in an inertial frame \(S'\) that moves with constant velocity \(v\) along the common \(x\)-axis of a second inertial frame \(S\) (standard configuration). If the clock advances by a proper-time interval \(\Delta\tau\) between two of its own ticks — two events that occur at the same place in \(S'\), so \(\Delta x' = 0\) — then the coordinate-time interval \(\Delta t\) assigned to those same two events in \(S\) is \(\Delta t = \gamma\,\Delta\tau\), with \(\gamma = \left(1 - v^2/c^2\right)^{-1/2} \ge 1\). Since \(\gamma \ge 1\), the moving clock runs slow: it is observed from \(S\) to advance by only \(1/\gamma\) seconds for each second of \(S\)-time.

\[ \Delta t = \gamma\,\Delta\tau, \qquad \gamma = \frac{1}{\sqrt{1 - v^2/c^2}} \ge 1 \]
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◆ DERIVATION EMBED · D-094 · not re-derived here

Length Contraction

The length of a rigid object measured along its direction of motion is shorter than its proper length \(L_0\) (the length measured in the object's rest frame) by the Lorentz factor: \(L = L_0/\gamma\), where \(\gamma = 1/\sqrt{1 - v^2/c^2}\) and \(v\) is the relative speed of the two inertial frames.

\[ \boxed{\,L = \frac{L_0}{\gamma} = L_0\sqrt{1 - \frac{v^2}{c^2}}\,} \]
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◆ DERIVATION EMBED · D-092 · not re-derived here

Relativity of Simultaneity

In two inertial frames \(S\) and \(S'\) in standard configuration (relative speed \(v\) along the common \(x\)-axis), two events that are simultaneous in \(S\) but separated by a spatial interval \(\Delta x\) along the direction of motion have, in \(S'\), a nonzero time separation \(\Delta t' = -\gamma v\,\Delta x/c^2\). Equivalently, two clocks synchronised in their common rest frame and separated there by proper distance \(L_0\) along the motion are, in any frame through which they move at speed \(v\), out of synchronisation: the leading clock lags the trailing clock by the leading-clocks-lag relation \(\Delta t = L_0 v/c^2\).

\[ \boxed{\;\Delta t_{\text{lag}} = \frac{L_0\, v}{c^2}\;}\qquad\qquad \Delta t'\big|_{\Delta t=0} = -\,\frac{\gamma\, v\, \Delta x}{c^2} \]
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Tier 3 · watch out

A common mistake is to assume that length contraction is a physical compression of the object. It is not. The object is not squashed; rather, the measurement of its length involves different spacetime slices. In the pole-barn paradox, if the pole is rigid, the stresses that would arise from a physical compression are avoided because the doors do not close simultaneously in the pole's frame. The "paradox" is purely kinematic, not dynamic. C

Worked example

Problem. A spaceship has a proper length of \(L_0 = 100\ \mathrm{m}\). It travels towards a space station with a proper length of \(L_{\text{station}} = 80\ \mathrm{m}\). The spaceship moves at a speed \(v = 0.8c\) relative to the station. Determine if the spaceship can fit inside the station in the station's frame, and calculate the time difference between the closing of the front and back doors in the spaceship's frame if the station closes them simultaneously in its own frame.

  1. Calculate the Lorentz factor \(\gamma\) for \(v = 0.8c\). \[ \gamma = \frac{1}{\sqrt{1 - 0.8^2}} = \frac{1}{\sqrt{1 - 0.64}} = \frac{1}{\sqrt{0.36}} = \frac{1}{0.6} = \frac{5}{3} \approx 1.67 \]
  2. Calculate the length of the spaceship in the station's frame using length contraction. \[ L_{\text{ship}} = \frac{L_0}{\gamma} = \frac{100}{5/3} = 60\ \mathrm{m} \]
  3. Compare \(L_{\text{ship}}\) with \(L_{\text{station}}\). Since \(60\ \mathrm{m} < 80\ \mathrm{m}\), the spaceship fits inside the station in the station's frame.
  4. Calculate the time difference in the spaceship's frame. In the station's frame, the doors close simultaneously, so \(\Delta t = 0\). The spatial separation between the doors in the station's frame is \(\Delta x = L_{\text{station}} = 80\ \mathrm{m}\). Using the relativity of simultaneity formula: \[ \Delta t' = -\gamma \frac{v \Delta x}{c^2} \] Substitute the values: \[ \Delta t' = -\frac{5}{3} \frac{(0.8c)(80)}{c^2} = -\frac{5}{3} \frac{64}{c} = -\frac{320}{3c} \]
  5. Convert to seconds. \(c \approx 3 \times 10^8\ \mathrm{m/s}\). \[ \Delta t' = -\frac{320}{3 \times 3 \times 10^8} = -\frac{320}{9 \times 10^8} \approx -3.56 \times 10^{-7}\ \mathrm{s} \]
\[ \boxed{\, \Delta t' \approx -3.56 \times 10^{-7}\ \mathrm{s} \,} \]

Units check. The term \(\frac{v \Delta x}{c^2}\) has units \(\frac{(\mathrm{m/s}) \cdot \mathrm{m}}{\mathrm{m^2/s^2}} = \frac{\mathrm{m^2/s}}{\mathrm{m^2/s^2}} = \mathrm{s}\). The result is in seconds, which is correct.

CHECK YOURSELF

Three quick tests

  1. Why is the twin paradox not a true paradox?
    AnswerThe situation is asymmetric because the traveling twin changes inertial frames, breaking the symmetry of the time dilation effect.
  2. In the pole-barn paradox, why does the pole not break in its own frame?
    AnswerBecause the doors do not close simultaneously in the pole's frame; the exit door closes (and reopens) before the entrance door closes behind the pole, so in the pole's frame there is never an instant when both doors are shut with the pole inside.
  3. What is the key invariant quantity in special relativity that ensures consistency between frames?
    AnswerThe spacetime interval \(ds^2 = c^2 dt^2 - dx^2\), which is the same for all inertial observers.
PROBLEMS

Problem set for PU-105 →

Each derivation in this unit ends with five graded problems with full solutions.

NOTES

Lecture notes drafted with a local model and checked line by line by the editor; every number in the worked example was recomputed.

Derivations cited: D-093 · D-094 · D-092 · Threads: force, energy, light