Past exam of the symmetry and relativity course of the University of Oxford 2019 1 c iii Solution 2026-10-25
Outside both light cones, the separation from the origin is spacelike. Thus the events in neither the causal past nor the causal future areNo causal curve can connect either endpoint to the other. These are the two green side regions in part c; the strict inequality excludes the causally reachable null boundaries.
Past exam of the symmetry and relativity course of the University of Oxford 2019 1 c Solution 2026-10-25
The upper-left panel shows the three causal structure regions, with null boundaries included in the appropriate causal future and causal past. For the charged trajectory, use part b with , choosing the direction so that . The electric field gives the constant three-force and hence the shifted hyperbolaIt starts with a vertical tangent at the origin, stays strictly inside the future light cone, and asymptotes to . The other panels implement the coordinate and topology changes used below; they are original spacetime diagrams, not copies of source artwork.
Causal regions in Minkowski spacetime and in spatially or temporally periodic flat spacetimes
. Blue denotes the causal future, orange the causal past, green events in neither, and purple membership in both. The top panels use ordinary and boosted inertial coordinates. The spatial quotient identifies vertical edges and shows the accelerated worldline wrapping across them. The temporal quotient identifies horizontal edges; every event belongs to both causal sets. Details. Past exam of the symmetry and relativity course of the University of Oxford 2019 1 d iii Solution 2026-10-25
The invariant spacelike condition is . Hence the primed-coordinate events in neither the causal future nor the causal past obeyThe green regions in part c retain their shape in primed coordinates. A particular spacelike event's coordinate time may change sign, but it never enters either light cone.
Past exam of the symmetry and relativity course of the University of Oxford 2019 1 d ii Solution 2026-10-25
The same Lorentz transformation maps the past light cone to itself. In the primed axes the causal past isthe orange region in the upper-right spacetime diagram of part c. Future and past are not interchanged by the standard boost.
Past light cone Created 2026-10-03 Updated 2026-10-14
The past light cone of a spacetime event is the past-directed part of its light cone. In Minkowski spacetime, its spacetime events satisfy with . They are the possible emission events of light rays arriving at . The interior also contains events that can send slower signals to . The retarded potential of a moving point electric charge, given by the Liénard–Wiechert potential, uses the emission event where the source's world line intersects this boundary.
Positive-energy spectrum condition 2026-10-13
The joint energy-momentum spectrum lies in the closed forward light cone. In axiomatic quantum field theory, this condition permits analytic continuation of Wightman functions in suitable complex spacetime domains. Together with Lorentz invariance, microcausality and the positivity of the physical state space, it is one of the hypotheses behind the CPT theorem.
Proper orthochronous Lorentz transformation 2026-10-25
A Lorentz transformation with determinant that preserves future-directed timelike four-vectors. Equivalently, it belongs to the identity component of the Lorentz group. For the Minkowski metric , its matrix satisfies and . Such transformations preserve the future light cone, so the retarded Green function of the d'Alembert operator transforms as a Lorentz scalar.
Shrinking cone energy argument Created 2026-10-06 Updated 2026-10-14
For the homogeneous speed-one wave equation, integrate its wave energy density over . The moving boundary contributes , while the usual flux contributes . Their sum is . Zero Cauchy data in the initial ball therefore force zero solution in its backward light cone.
