PHYSICS · Multi-part · Fermi University Physics · Relativity & Gravitation · Schwarzschild spacetime and the tests of general relativity · Schwarzschild spacetime and the tests of general relativity
The Geometry of Gravity, Ch Solar-system tests, the PPN framework and alternative theories
Problem
A Brans-Dicke universe has ωBD=8, giving γPPN=(1+ωBD)/(2+ωBD) and βPPN=1. A radar signal travels from Earth to a transponder on a Mars orbiter while Mars is almost directly behind the Sun, so the ray grazes the solar limb. Take the Earth-Sun distance as r1=1.496×1011m, the Mars-Sun distance as r2=2.280×1011m, the impact parameter as the solar radius b=R⊙=6.96×108m, and GM⊙/c2=1.48km. The excess round-trip coordinate time (the Shapiro delay), generalised to the PPN framework, is ΔtS=c32GM⊙(1+γPPN)ln(b24r1r2).
((a)) Compute ΔtS predicted by general relativity (γPPN=1), in microseconds.
((b)) Compute ΔtS predicted by this Brans-Dicke theory, and give its difference from the general-relativistic value in microseconds.
((c)) Universality of free fall has been confirmed to a few parts in 1015. Explain why this Brans-Dicke theory, whose Shapiro delay differs measurably from general relativity's, is not already excluded by that result: state which assumption used to build the Einstein field equations in the Newtonian limit it drops, and what matter still couples to.