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The Spacetime Interval Calculator computes the Lorentz-invariant spacetime interval between two events in special relativity. The interval is defined as:
$$s^2 = c^2 \Delta t^2 - \Delta x^2 - \Delta y^2 - \Delta z^2$$
Unlike spatial distances or time intervals alone — which change depending on the observer's reference frame — the spacetime interval $$s^2$$ is the same for all inertial observers. This invariance makes it one of the most fundamental quantities in relativity, encoding the causal structure of spacetime itself.
The sign of $$s^2$$ classifies the relationship between two events: timelike ($$s^2 > 0$$) means a massive particle could travel between them; spacelike ($$s^2 < 0$$) means no signal can connect them; lightlike ($$s^2 = 0$$) means only light can bridge the gap. This classification is absolute — all observers agree on it.
In Minkowski spacetime, the geometry is described by the metric:
$$ds^2 = c^2\,dt^2 - dx^2 - dy^2 - dz^2$$
This is the flat-spacetime analog of the Pythagorean theorem, but with a crucial sign difference: the time component enters with a positive sign and spatial components with negative signs (using the +−−− convention). For finite separations between two events:
$$s^2 = c^2(\Delta t)^2 - (\Delta x)^2 - (\Delta y)^2 - (\Delta z)^2$$
The three interval types have distinct physical meanings:
The invariance of $$s^2$$ under Lorentz transformations is the geometric foundation of special relativity. Just as rotations preserve spatial distance $$d^2 = x^2 + y^2 + z^2$$, Lorentz boosts preserve the spacetime interval. This is why the Minkowski metric is sometimes called a "pseudo-Euclidean" metric — it measures a generalized "distance" in 4D spacetime.
The Interval Type tells you the causal relationship between the two events. For timelike intervals, the Proper Time gives the elapsed time on a clock moving inertially between the events — this is the shortest possible time separation. For spacelike intervals, the Proper Distance gives the spatial separation measured in a frame where both events are simultaneous. A lightlike interval means the events lie on each other's light cone. These classifications are observer-independent and form the backbone of causality in relativity.
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With Δt = 2 s and Δx = 100,000 km, the interval is timelike (s² > 0). A massive particle could travel between these events, with proper time τ ≈ 1.97 s.
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With Δt = 0.5 s and Δx = 300,000 km (≈ 1 light-second), the spatial separation exceeds what light can traverse. No signal can connect these events.
The spacetime interval $$s^2 = c^2\Delta t^2 - \Delta x^2 - \Delta y^2 - \Delta z^2$$ is the relativistic generalization of distance. Unlike ordinary distance or time, which change between reference frames, the spacetime interval is Lorentz invariant — every inertial observer computes the same value. It encodes both the separation and the causal relationship between two events.
A timelike interval ($$s^2 > 0$$) means the two events are close enough in space (relative to their time separation) that a massive particle traveling slower than light could be present at both. There exists a frame where both events happen at the same place, separated only by time. The proper time $$\tau = \sqrt{s^2}/c$$ is the time elapsed on a clock traveling between them.
A spacelike interval ($$s^2 < 0$$) means the spatial separation exceeds what any signal — even light — could traverse in the given time. No causal influence can pass between the events. There exists a frame where both events are simultaneous, separated only by space. The ordering (which happened first) is frame-dependent.
A lightlike interval ($$s^2 = 0$$) means $$c\Delta t = \sqrt{\Delta x^2 + \Delta y^2 + \Delta z^2}$$ — the events are exactly connected by a light signal. Light cones, formed by all null intervals from a given event, divide spacetime into causally connected (timelike) and disconnected (spacelike) regions.
The invariance follows from the postulates of special relativity: the laws of physics are the same in all inertial frames, and the speed of light is constant. Mathematically, Lorentz transformations mix space and time coordinates while preserving the quantity $$c^2\Delta t^2 - \Delta x^2 - \Delta y^2 - \Delta z^2$$, just as rotations mix x and y while preserving $$x^2 + y^2$$.
The sign convention determines whether $$s^2 = c^2\Delta t^2 - \Delta r^2$$ (+−−−, used here) or $$s^2 = -c^2\Delta t^2 + \Delta r^2$$ (−+++). Both are standard in physics. With +−−−, timelike intervals are positive and spacelike are negative. Particle physicists often use −+++. The physics is identical; only the sign of $$s^2$$ flips.
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