PHYSICS · Multi-part · Fermi University Physics · Relativity & Gravitation · Relativistic dynamics and fields in flat spacetime · Relativistic dynamics and fields in flat spacetime
The Geometry of Gravity, Ch Tensors in flat spacetime: index notation and covariant field equations
Problem
A particle of rest mass M, at rest in frame S, decays into two photons travelling along +x and −x, each carrying half the rest energy: p1μ=(Mc/2,Mc/2,0,0) and p2μ=(Mc/2,−Mc/2,0,0). In S the parent's four-momentum is pμ=(Mc,0,0,0), and p1μ+p2μ=pμ as required by conservation. A second inertial frame S′ moves at v=0.6c along x relative to S (γ=1.25).
((a)) Apply the tensor transformation law for a type (1,0) object (the Lorentz transformation) to p1μ, p2μ and pμ separately, to find their components in S′, in units of Mc.
((b)) Verify that p1′μ+p2′μ=p′μ still holds in S′, and explain why checking conservation in S alone was already enough to guarantee this, without redoing the calculation.