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

In summary, the conversation discusses showing the relation between received and emitted frequency, finding the proper area of a sphere, and finding the ratio of fluxes. The equations and solutions for each part are also provided.
  • #1
unscientific
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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

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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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  • #2
bumpp
 
  • #3
Solved.
 

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

What is redshift in frequency?

Redshift in frequency is a phenomenon in which the frequency of light emitted from objects in the universe appears to decrease as the object moves away from an observer. It is caused by the expansion of the universe, which stretches the wavelength of light and shifts it towards the red end of the spectrum.

How is redshift in frequency related to the expansion of the universe?

Redshift in frequency is directly related to the expansion of the universe. As the universe expands, the wavelength of light also expands, causing a shift towards the red end of the spectrum. This is known as cosmological redshift and is used to measure the distances of galaxies and other objects in the universe.

How is redshift in frequency measured?

Redshift in frequency is measured using spectroscopy, which involves analyzing the spectrum of light emitted from an object. The amount of redshift is determined by comparing the observed wavelength of a known spectral line to its expected wavelength. The difference between the two is used to calculate the redshift in frequency.

What can redshift in frequency tell us about the universe?

Redshift in frequency is a crucial tool for understanding the universe. By studying redshift, scientists can measure the distances of galaxies and other objects, determine the expansion rate of the universe, and gain insights into the evolution and structure of the universe.

Is redshift in frequency the same as redshift in wavelength?

Yes, redshift in frequency and redshift in wavelength are two ways of describing the same phenomenon. As the wavelength of light expands, its frequency decreases, resulting in a shift towards the red end of the spectrum. Both terms are used interchangeably in scientific studies of the universe.

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