Defining Emitter vs Observer for Schwarzschild Metric

MarkovMarakov
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Let's say we are working with the Schwarzschild metric and we have an emitter of light falling into a Schwarzschild black hole.

Suppose we define the quantity u=t- v where dv/dr= 1/(1-r_{s}/r) where r_s is the Schwarzschild radius. What is the u as observed by the emitter? I just need a *definition of u_e*. I have problems identifying the quantities as measured by an observer at large r and that of the emitter. Would I be right at least to say that t_{e}=\tau the proper time? Many thanks.

_____

In fact, I've been told that

$$du_o/d\tau=du_e/d\tau$$

Why is it?
 
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MarkovMarakov said:
Let's say we are working with the Schwarzschild metric and we have an emitter of light falling into a Schwarzschild black hole.

Suppose we define the quantity $$u=t- v$$ where $$dv/dr= 1/(1-r_{s}/r)$$ where $r_s$ is the Schwarzschild radius. What is the $u$ as observed by the emitter? I just need a *definition of $u$*.
I don't understand. You already gave the definition of u as u=t-v.
 
@DaleSpam: You are right. I have missed out the subscript e. I meant u as measured by the emitter.
 
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Well, v is just some function of r and so u is just some function of t and r. I don't see how it is something measured by anyone.

Please fix your LaTeX.
 
@DaleSpam: LaTex fixed. I suppose u_e would be in terms of t_e,r_e measured by the emitter, no? But then what is its explicit form?
 
Well, what coordinate system do you want to use for the emitter? Then you would just have to substitute in the transforms for the emitter's coordinates.
 
@DaleSpam: the proper time is that of the emitter. I am still not sure how to do the substitution though. (Sorry about my daftness. :( )
 
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