← Special Relativity
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Einstein's Postulates & Spacetime

In 1905 Einstein resolved the contradiction between Newtonian mechanics and Maxwell's electrodynamics with just two postulates: the laws of physics are the same in all inertial frames, and the speed of light in vacuum is the same for all inertial observers regardless of the motion of the source. These postulates force a radical revision of space and time.

Key Concepts

First Postulate
The laws of physics (including Maxwell's equations) take the same form in all inertial reference frames. No inertial frame is preferred — there is no absolute rest.
Second Postulate
The speed of light in vacuum, c=2.998×108c=2.998\times10^8 m/s, is the same for all inertial observers regardless of the motion of the source or observer. This is the key contradiction with Galilean relativity.
Relativity of Simultaneity
Two events that are simultaneous in frame SS are generally not simultaneous in frame SS' moving relative to SS. There is no universal "now" — simultaneity is frame-dependent.
Spacetime Interval
s2=c2t2x2y2z2s^2 = c^2t^2 - x^2 - y^2 - z^2. This combination is invariant — the same in all inertial frames. Positive: timelike; zero: lightlike; negative: spacelike separation.

Key Equations

Speed of light
c=2.998×108 m/s3.0×108 m/sc = 2.998\times10^8\text{ m/s} \approx 3.0\times10^8\text{ m/s}
The universal speed limit; same for all inertial observers.
Spacetime interval
s2=c2Δt2Δx2Δy2Δz2s^2 = c^2\Delta t^2 - \Delta x^2 - \Delta y^2 - \Delta z^2
Lorentz invariant; positive = timelike, zero = lightlike, negative = spacelike.
Relativistic Doppler
fobs=fsource1β1+βf_{\rm obs} = f_{\rm source}\sqrt{\frac{1-\beta}{1+\beta}}
For source receding (β = v/c > 0); redshift when moving away.
Worked Example

Relativity of Simultaneity

Problem

Two lightning strikes hit both ends of a train (length L0=300L_0=300 m in its rest frame) simultaneously in the ground frame. The train moves at v=0.60cv=0.60c. Are the strikes simultaneous for a train observer?

Solution

In the ground frame (SS): Δt=0\Delta t=0, Δx=L=L0/γ\Delta x=L=L_0/\gamma (contracted length).

For the train frame (SS') using the Lorentz transform: Δt=γ(ΔtvΔx/c2)\Delta t' = \gamma(\Delta t - v\Delta x/c^2).

With γ=1.25\gamma=1.25, Δt=0\Delta t=0, Δx=L0/γ=240\Delta x=L_0/\gamma=240 m:

Δt=1.25(00.60c×240c2)=1.25×0.60×240c=180c=600 ns\Delta t' = 1.25\left(0 - \frac{0.60c \times 240}{c^2}\right) = 1.25\times\frac{-0.60\times240}{c} = \frac{-180}{c} = -600\text{ ns}

The front strike happens 600 ns before the rear strike in the train frame — not simultaneous.

Answer No — the front strike precedes the rear strike by 600 ns in the train's frame.
Practice

Exercises

7 problems
1 of 7

A photon is emitted by a source moving at 0.80c relative to you. The simulation shows both a Galilean prediction (top) and the relativistic reality (bottom). What is the photon's speed (in m/s) as measured by you?

c invariance
Source speed β 0.00c

Notice: the photon (bottom row) always leads the source by the same amount — it doesn't matter how fast the source moves.

Photon speed
c = m/s

Enter the exact value of c in m/s (e.g. 3e8 or 300000000).

2 of 7

Two events: A at the origin, B at Δx = 9.0×10⁸ m, Δt = 4.0 s. The Minkowski diagram shows both events and the light cone. Find the spacetime interval s = √[(cΔt)² − Δx²] in metres.

spacetime diagram
Interval s
s = m

e.g. enter 7.94e8 or 794000000

3 of 7

Light from a star 4.0 light-years away is observed on Earth. How many years does it take to arrive?

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4 of 7

A star explodes (event A) and a comet passes Earth (event B), separated by Δt=5.0\Delta t=5.0 yr and Δx=6.0\Delta x=6.0 ly. Is this interval timelike, lightlike, or spacelike? Find s2|s^2| in ly². (c=1c=1 ly/yr.)

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5 of 7

A source moves away at β=v/c=0.60\beta=v/c=0.60. Find the observed frequency ratio fobs/fsource=(1β)/(1+β)f_{\rm obs}/f_{\rm source}=\sqrt{(1-\beta)/(1+\beta)}.

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6 of 7

The Lorentz factor γ=1/1β2\gamma=1/\sqrt{1-\beta^2} at β=0.60\beta=0.60. Find γ\gamma.

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7 of 7

Two events occur at the same location in frame SS separated by Δt=3.0\Delta t=3.0 ns. In frame SS' moving at β=0.80\beta=0.80, find γ\gamma first, then Δt=γΔt\Delta t'=\gamma\Delta t (in ns).

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Key Takeaways

  • Einstein's two postulates — equal laws in all inertial frames, and constant cc — force a revision of simultaneity, time, and length.
  • The spacetime interval s2=c2Δt2Δx2s^2=c^2\Delta t^2-\Delta x^2 is Lorentz-invariant; its sign classifies event pairs as timelike, lightlike, or spacelike.
  • Relativity of simultaneity: events simultaneous in SS are separated by Δt=γvΔx/c2\Delta t'=-\gamma v\Delta x/c^2 in SS'.
  • cc is the universal speed limit — no information or massive particle can reach or exceed it.