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The Lumenary

Practice · First-year graduate

The geometry of spacetime: special and general relativity

The geometry of spacetime: special and general relativity

Warm-upHuman

A probe travels from Earth to a star 1212 light-years away at speed v=1213v = \frac{12}{13} (units with c=1c = 1). How many years pass on the probe's clock during the trip?

The geometry of spacetime: special and general relativity

Warm-upHuman

Which separation vectors (Δt,Δx,Δy,Δz)(\Delta t, \Delta x, \Delta y, \Delta z) between two events are timelike (so that a massive particle could travel from one event to the other)? Use c=1c = 1. Select all that apply.

Choose all that apply

The geometry of spacetime: special and general relativity

CoreHuman

A spacecraft moves at 45c\frac45 c relative to Earth and fires a probe forward at 45c\frac45 c relative to itself. What is the probe's speed relative to Earth?

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The geometry of spacetime: special and general relativity

CoreHuman

The reverse triangle inequality τ(v)+τ(w)≤τ(v+w)\tau(v) + \tau(w) \le \tau(v + w) is stated for future-pointing causal vectors. Where does the proof use that both point to the future?

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The geometry of spacetime: special and general relativity

CoreHuman

Let q−pq - p be future timelike in Minkowski spacetime. Among future-directed causal curves from pp to qq, which statement about proper time is correct?

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The geometry of spacetime: special and general relativity

CoreHuman

Compute the Schwarzschild radius rs=2GM/c2r_s = 2GM/c^2 of the Sun, in kilometres, rounded to the nearest whole number. Use GM⊙=1.327×1020 m3 s−2GM_\odot = 1.327 \times 10^{20}\ \mathrm{m^3\,s^{-2}} and c=2.998×108 m s−1c = 2.998 \times 10^8\ \mathrm{m\,s^{-1}}.

The geometry of spacetime: special and general relativity

CoreHuman

Starlight grazing the Sun is deflected by 1.75′′1.75'' according to general relativity. Treating light as a Newtonian particle moving at speed cc (Soldner, 1801) gives a different value. Which?

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The geometry of spacetime: special and general relativity

CoreFormal

The lesson's Lean theorem twin_paradox has hypotheses h₁ : ‖x‖ ≤ t₁ and h₂ : ‖y‖ ≤ t₂ and conclusion √(t₁^2 - ‖x‖^2) + √(t₂^2 - ‖y‖^2) ≤ √((t₁ + t₂)^2 - ‖x + y‖^2). What would happen if both hypotheses were deleted?

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The geometry of spacetime: special and general relativity

StretchHuman

For light in the Schwarzschild metric (G=c=1G = c = 1), (drdλ)2=E2−L21−2M/rr2\big(\frac{dr}{d\lambda}\big)^2 = E^2 - L^2 \frac{1 - 2M/r}{r^2}, and the impact parameter is b=L/Eb = L/E. A ray from infinity is captured exactly when 1/b21/b^2 exceeds the maximum of (1−2M/r)/r2(1 - 2M/r)/r^2. Find the critical value of b2/M2b^2/M^2.

The geometry of spacetime: special and general relativity

CoreComputational

A polygonal worldline is given by a list of events (t, x, y, z) (with c=1c = 1). Write proper_time(events) returning the total proper time ∑kΔtk2−Δxk2−Δyk2−Δzk2\sum_k \sqrt{\Delta t_k^2 - \Delta x_k^2 - \Delta y_k^2 - \Delta z_k^2}, and raising ValueError if some step is not future-pointing causal (Δtk≤0\Delta t_k \le 0 or Δsk2>0\Delta s_k^2 > 0).

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