A static spherical star of mass has a weak external field
PHYSICS · Multi-part · Fermi University Physics · Relativity & Gravitation · The equivalence principle and gravity as geometry · The equivalence principle and gravity as geometry
Relativity and Gravitation, Ch Gravity as curved spacetime: redshift and local inertial frames
Problem
A static spherical star of mass M has a weak external field, GM/rc2≪1 everywhere of interest. Outside it the gravitational potential is Φ(r)=−GM/r, zero at infinity, and the local field strength is g(r)=GM/r2. Light is emitted by a source at rest at radius r1 and received by an observer at rest at radius r2>r1. Work throughout to first order in GM/rc2.
((a)) Starting from the local result Δν/ν=−gΔr/c2 for a short radial climb Δr, stack short climbs into an integral and show that νemνrec=1−c2GM(r11−r21).
((b)) Evaluate the redshift z for light leaving the Sun's photosphere and received at the Earth's orbit. Take M⊙=1.989×1030kg, R⊙=6.960×108m, r2=1.496×1011m, G=6.674×10−11Nm2kg−2 and c=2.998×108ms−1; ignore the Earth's own field and its orbital motion.
((c)) Obtain the same formula a second way, from energy conservation: a mass m is lowered slowly from r2 to r1 with the work captured by a generator, is then converted entirely into a light pulse which is beamed up to r2 and there converted entirely back into a mass at rest. Show that the cycle can create no energy only if the pulse's energy obeys the ratio derived in (a), and hence, since a pulse's energy is proportional to its frequency, that the frequency ratio is the same.