Four-vectors and Minkowski contractions
Fix a spacetime convention, lower indices correctly, and use invariant contractions to distinguish physical measurements from frame components.
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The question for today
What you’ll understand
- Apply one explicit metric and boost convention consistently.
- Compute invariant norms and distinguish them from Euclidean lengths.
- Relate proper time, four-velocity, and observer-measured energy.
Covariant electrodynamics starts with a bookkeeping decision that has physical consequences: which signs belong to time and which belong to space? We will keep one answer throughout this module. Once the convention is fixed, contractions provide quick tests of calculations that would otherwise require many component equations. The aim is to recognize what changes when an observer moves and what remains a property of the same event separation, particle, or field.
Declare the geometry before calculating
Use Cartesian inertial coordinates and the metric . Greek indices run from zero through three; spatial indices run from one through three. Time is multiplied by the vacuum light speed so every coordinate has units of metres. A four-vector is defined by its Lorentz transformation law, rather than by the fact that somebody has arranged four numbers in a column. This distinction will matter when electric and magnetic components are assembled into a tensor.
Lowering an index means contracting with the metric. Thus the spatial components change sign, while the time component does not. A repeated index is summed when it appears once up and once down. Two upper indices do not define a scalar contraction without an additional metric. These rules prevent an accidental Euclidean sum from being mistaken for an invariant. They also tell us that the derivative has lower components ; raising its index changes the spatial derivative signs.
Boost components while preserving the interval
Let the primed observer move at speed along positive x relative to the unprimed observer. Our passive boost has and negative off-diagonal entries. The inverse boost replaces beta by its negative. Stating which observer moves avoids the common mistake of using a correct boost matrix for the opposite transformation. Expanding the two transformed squares shows that the cross terms cancel and the remaining coefficient is . This algebra explains interval preservation directly.
With this signature a positive squared interval is timelike, a negative one spacelike, and zero null. Along an infinitesimal timelike worldline displacement, . For a finite endpoint separation, its norm divided by c equals elapsed clock time only on the connecting inertial worldline. An accelerated clock requires integrating the proper-time increments along its actual path. A spacelike separation cannot be turned into a timelike one by boosting. Its coordinate time may change sign, but its causal classification cannot. Null separation does not mean the events coincide: a light signal can connect different events with zero interval.
Normalize motion using a physical clock
For a massive particle define , where tau is its own proper time. Its norm is always , even when its ordinary velocity changes. Four-momentum is for fixed rest mass m. The invariant mass shell follows by contraction. Differentiating the fixed four-velocity norm also gives . Four-acceleration is orthogonal to four-velocity in Minkowski geometry; it need not be perpendicular to ordinary velocity in a spatial diagram.
An observer with normalized four-velocity measures particle energy . In that observer's rest coordinates this reduces to c times the particle's temporal momentum component. Energy is therefore an observer-dependent contraction involving two physical objects, whereas rest mass belongs to the particle alone. Massless particles still have meaningful four-momentum and zero momentum norm, but cannot be assigned a rest-frame proper-time four-velocity. Applying the massive definition to a photon would divide by a vanishing clock increment.
Work it through
Find an event's rest separation
Relative to the origin an event has , , and . Transform it using and find the proper time of the inertial clock connecting the events. Use .
The boost factor is . Before transforming, compute the squared interval , so the separation is timelike.
The time coordinate becomes . The spatial coordinate becomes , so the primed clock is at rest between these events.
The invariant proper length is . Dividing by c gives ; the transformed squared interval is again sixteen square metres.
The events are separated by 13.3 nanoseconds on the connecting inertial clock, although the unprimed coordinate time is 16.7 nanoseconds.
The living notebook
Explore the model
Interactive lab · spacetime
An invariant with changing components
For each fresh comparison, Reset and set BOTH controls: first Relative velocity β = 0 and Event time ct = 1, then Reset and set β = 0.6 and ct = 1. Predict that the fixed x = 0.6 event moves to x′ = 0, ct′ = 0.8 while its interval stays 0.64. Inspect the paused frames or Step.
- Lorentz factor γ
- 1.12
- Event x′
- 0.168
- Event ct′
- 0.817
A fixed x = 0.6 event is Lorentz transformed with c = 1. Playback highlights the relation between coordinate descriptions; it does not move the event. Parameter changes pause playback and recompute the model at the current elapsed time. Reset restores both parameters and returns time to zero. Playback starts paused. Adjust either parameter, then choose Play or Step.
Look forThe instrument uses c = 1 and one fixed spatial coordinate. It tests a Lorentz transformation, not charged-particle dynamics or curved spacetime.
Pause & reason
Check your understanding
Your turn
Try it yourself
Two events have and , with no transverse separation. Find a boost making them simultaneous, then calculate their spatial separation in that frame.
Take a moment to make a prediction or work it out on paper. Open a hint when you need one.
Give me a hint
Set the transformed time component to zero before evaluating gamma. Check the interval rather than trying to assign a proper time.
Compare with the solution
The simultaneity condition is , giving and . Then . The squared interval is initially and finally . This is a spacelike separation with a frame of simultaneity, not a massive clock's elapsed proper time.
Keep the idea
Take it with you
- Lowering one spatial index changes its sign in the declared metric.
- Lorentz boosts preserve causal type even when time and space components change.
- Proper time normalizes massive motion, while energy requires a specified observer.
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