How is Frequency Redshift Related to Sphere's Proper Area and Flux Ratio?

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Homework Statement



(a) Show the relation between frequency received and emitted
(b) Find the proper area of sphere
(c) Find ratio of fluxes

2007_B5_Q4.png

Homework Equations

The Attempt at a Solution



Part (a)
Metric is ##ds^2 = -c^2dt^2 + a(t)^2 \left( \frac{dr^2}{1-kr^2}+ r^2(d\theta^2 + \sin^2\theta) \right)##. For a light-like geodesic, we have ##ds^2=0##, which means
[tex]c\frac{1}{a(t)} dt = \frac{1}{\sqrt{1-kr^2}} dr[/tex]
Since RHS is purely in terms of spatial distance, we have
[tex]\frac{1}{a(t_1)}\delta t_1 = \frac{1}{a(t_2)}\delta t_2[/tex]

Part(b)
Proper area is:
[tex]dA = \left( a r d\theta \right)\left( a r \sin\theta d\phi \right)[/tex]
[tex]A = 4\pi r^2 a^2(t_2)[/tex]

Part(c)
Let's first start with emitter at A.
From part (a), frequency observed is ##\frac{a(t_{1A})}{a(t_{2A})}f_0## where ##t_1## and ##t_2## is time emitted and received.
Area at reception is ##4\pi r_a^2 a^2(t_{2A})##.
Flux is then proportional to ##\frac{a(t_{1A})}{a(t_{2A})^3 r_a^2}##. Flux for B is then ##\frac{a(t_{1B})}{a(t_{2B})^3 r_b^2}##.

Ratio of flux is then:
[tex]\frac{F_B}{F_A} = \frac{a(t_B)}{a(t_A)} \frac{r_a^2}{r_b^2} \frac{a^3(t_{2A})}{a^3(t_{2B})}[/tex]

How do I find the time the radiation is received ##t_{2A}## and ##t_{2B}##? Clearly they are different.
 
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