A Relativistic Redshift and understanding it's approximation

Arman777
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I was reading an article, and I saw this expression.

$$
1+z=\frac{(g_{\mu\nu}k^{\mu}u^{\nu})_e}{(g_{\mu\nu}k^{\mu}u^{\nu})_o}
$$

Where ##e## represents the emitter frame, ##o## the observer frame, ##g_{\mu\nu}## is the metric, ##k^{\mu}## is the photon four-momentum and ##u^{\nu}## is the four-velocity of the source or observer.

Has anyone seen this expression before? I want to understand how we can obtain $$1+z=\frac{a_o}{a_e}$$ from this expression and understand the metric potentials etc. Any reference would be appreciated. Thanks.
 
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Arman777 said:
Where e represents the emitter frame, o the observer frame,
No, they represent the emitter and observer, respectively. The expressions themselves are invariant. However, they equal the frequencies measured by emitter/observer.

Arman777 said:
Has anyone seen this expression before?
g(k,u) is by definition the frequency of wave vector k as measured by an observer with 4-velocity u. The expression follows directly from that and the definition of the redshift parameter z.

Arman777 said:
I want to understand how we can obtain 1+z=aoae from this expression and understand the metric potentials etc. Any reference would be appreciated. Thanks.
This follows directly from making the computation for comoving observers in a Robertson-Walker spacetime.
 
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Orodruin said:
No, they represent the emitter and observer, respectively
hmm. That's what is says in the original article...not my fault. But you are also right.
Orodruin said:
This follows directly from making the computation for comoving observers in a Robertson-Walker spacetime.
In other types of metric (LTB, Bianchi) the ##1+z=a_o/a_e## will not hold then right ?
 
Arman777 said:
In other types of metric (LTB, Bianchi) the 1+z=ao/ae will not hold then right ?
The scale factors are particular for the RW spacetimes in standard coordinates.
 
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