General Relativity gravitational redshift

AI Thread Summary
The discussion focuses on deriving the expression for gravitational redshift in the context of general relativity. The equation for frequency change, Δf/f₀ = -gh/c², is established, and the user is attempting to integrate this to find the frequency change as light travels from a gravitational body to infinity. A challenge arises in expressing gravitational acceleration (g) since a photon has zero mass, complicating the use of the gravitational force equation. The user recognizes the need to integrate with respect to height (h) but seeks clarification on how to proceed with the integration and the correct expression for g. The conversation highlights the complexities of applying gravitational concepts to massless particles like photons.
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Homework Statement


The gravitational redshift tends to decrease the frequency of light as it travels upwards a distance h,\frac{\Delta{f}}{f_{0}}=\frac{-gh}{c^2}
integrate both sides of this equation (from the surface of the gravitation body out to infinity) to derive the expression for the change in frequency near a high gravitational field:\frac{f}{f_{0}}\cong{1-\frac{GM}{Rc^2}}

Homework Equations


Given above. A photon is emitted at the surface of the gravitational body (M) with radius R. It's frequency is measured distance h above the gravitational body to be f, while its frequency at the gravitational body is f0. g is the gravitational attraction of the body on the photon.

The Attempt at a Solution


Well, I've gotten far enough to see that \frac{f}{f_{0}}-1=\frac{-gh}{c^2}, which makes sense because gh is the increase in gravitational potential energy.
However, I don't know how to express g. I would use F_{g}=G\frac{Mm}{r^2}, but because a photon's mass is zero, I don't know what to do.
I guess I also need to integrate with respect to h.
Help!?
 
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