Lifetime of the universe - FRW

In summary, the conversation discusses finding the value of A and Ω(η) and plotting them, as well as finding the maximum value of the normalized scale factor, lifetime of the universe, and the deceleration parameter. The unsolved problem is finding the lifetime of the universe. The first part of the solution involves using the FRW equation and substituting to find A and Ωm. The second part involves finding the maximum value of the normalized scale factor and using the equation for the deceleration parameter. The conversation then addresses how to find the lifetime of the universe, with various suggestions for the expression and limits of integration. Finally, it is mentioned that the problem has been solved.
  • #1
unscientific
1,734
13

Homework Statement


[/B]
(a) Find the value of A and ##\Omega(\eta)## and plot them.
(b) Find ##a_{max}##, lifetime of universe and deceleration parameter ##q_0##.
2013_B5_Q3.png


Homework Equations



Unsolved problems: Finding lifetime of universe.

The Attempt at a Solution



Part(a)[/B]
FRW equation is given by
[tex]\left( \frac{\dot a}{a}\right)^2 = H_0^2 \Omega_{m,0} a^{-3} - \frac{kc^2}{a^2} [/tex]
Subsituting and using ##dt = a d\eta##, I find that ##A = \frac{H_0^2}{c^2}\Omega_{m,0}##.
Using ##\\Omega_m = \Omega_{m,0}a^{-3}##, I find that ##\Omega_m = \frac{kc^2}{H_0^2 sin^2(\frac{\sqrt{k} c \eta}{2})}##.

Part(b)
Maximum value of normalized scale factor is
[tex]a_{max} = \frac{A}{k} = \frac{H_0^2}{kc^2}\Omega_{m,0}[/tex]
Deceleration parameter is given by
[tex]q_0 = -\frac{\ddot a_0 a_0}{\dot a_0^2}[/tex]
This can be found by using ##\sqrt {k} c \eta = sin (\sqrt {k} c \eta)##.

How do I find the lifetime of the universe? Is it simply ## \int_0^\infty t d\eta##? If I can solve for the lifetime, I can compare it to its current age and see if that is feasible.
 
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  • #2
bumpp
 
  • #3
bumpp
 
  • #4
bumpp - What is the expression for lifetime of a universe? Is it simply## \int_t^{t_0} dt = \int_0^\eta a(\eta) d\eta##?
 
  • #5
bumpp
 
  • #6
bumpp
 
  • #7
Is the lifetime simply ##\int dt = \int \frac{1}{aH} da##? If so, what are the limits of integration?
 
  • #8
If it is a closed universe, curvature eventually dominates and ##a \rightarrow 0##? so the limits would be from ##1## to ##0##?
 
  • #9
limits anyone?
 
  • #10
solved.
 

What is the FRW model of the universe?

The FRW model is a mathematical framework used to describe the large-scale structure and evolution of the universe. It is based on the work of physicists Georges Lemaître, Howard P. Robertson, and Arthur Geoffrey Walker, and is named after them.

What is the current estimated age of the universe?

According to the latest measurements and observations, the current estimated age of the universe is about 13.8 billion years. This value is based on the Planck satellite mission data and is considered to be the most accurate estimate to date.

How does the FRW model explain the expansion of the universe?

The FRW model explains the expansion of the universe through the use of Einstein's theory of general relativity. It assumes that the universe is homogeneous and isotropic on a large scale and that the expansion is driven by a mysterious force called dark energy.

What is the fate of the universe according to the FRW model?

The fate of the universe according to the FRW model depends on the amount of matter and energy in the universe. If the amount of dark energy remains constant, the universe will continue to expand indefinitely. If the amount of dark energy increases, the universe will experience a "Big Rip" where everything will be torn apart. If the amount of dark energy decreases, the universe may eventually collapse in a "Big Crunch."

Can the FRW model be tested or proven?

Yes, the FRW model can be tested and proven through observations and measurements of the universe. Scientists use various methods such as cosmic microwave background radiation, supernova surveys, and galaxy redshift surveys to gather data and test the predictions of the model. So far, the FRW model has been able to accurately explain and predict many observations of the universe.

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