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

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SUMMARY

This discussion focuses on the relationship between frequency redshift and the proper area and flux ratio of spheres in cosmological contexts. The key equations derived include the metric for light-like geodesics, which establishes the relationship between emitted and received frequency, and the proper area of a sphere, calculated as \(A = 4\pi r^2 a^2(t_2)\). Additionally, the flux ratio is determined using the formula \(\frac{F_B}{F_A} = \frac{a(t_B)}{a(t_A)} \frac{r_a^2}{r_b^2} \frac{a^3(t_{2A})}{a^3(t_{2B})}\). The discussion concludes with a query regarding the determination of the times \(t_{2A}\) and \(t_{2B}\) for received radiation.

PREREQUISITES
  • Understanding of general relativity and cosmological metrics
  • Familiarity with the concept of redshift in astrophysics
  • Knowledge of proper area calculations in spherical coordinates
  • Basic grasp of flux and its relation to area and intensity
NEXT STEPS
  • Study the derivation of the Friedmann-Lemaître-Robertson-Walker (FLRW) metric
  • Learn about the implications of cosmological redshift on observed frequencies
  • Explore the concept of flux conservation in expanding universes
  • Investigate methods for calculating time intervals in cosmological models
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Astronomers, astrophysicists, and students of cosmology who are interested in understanding the implications of frequency redshift and flux ratios in the context of expanding universes.

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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
c\frac{1}{a(t)} dt = \frac{1}{\sqrt{1-kr^2}} dr
Since RHS is purely in terms of spatial distance, we have
\frac{1}{a(t_1)}\delta t_1 = \frac{1}{a(t_2)}\delta t_2

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

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:
\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})}

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