Find the Metastatic Conditions for Omegas in the Friedmann Equation

In summary, the Friedmann Equation is a fundamental equation in cosmology used to study the evolution and expansion of the universe. It has been refined and expanded upon by scientists since its first derivation in 1922. Metastatic conditions refer to the spread of cancer or hypothetical particles known as omegas throughout the body or universe, respectively. By using the Friedmann Equation, scientists can potentially identify metastatic conditions for omegas and gain a better understanding of the behavior of the universe. This could also have implications for our understanding of dark matter and dark energy. While there have been numerous studies and experiments conducted to investigate this topic, further research is still needed.
  • #1
Buzz Bloom
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Homework Statement
Note: I use the notation []’ to indicate d[]/dt. This is because I do not have a convenient way to use the dot notation for differentiation.

In equation [3] below, what are the constrains on the Ωs (in addition to those given in the Relevant equations [8], [9], and [10]) such that there is a value, t=s satisfying [1] and [2]?
Relevant Equations
See below in Solution section.
Required Equations
Note: Includes inequalities.
[1] H(s) = 0, and
[2] H’(s) = 0?
[3]
FriedmannEqOmegas.png

[4] H = a’/a
[5] a(t0) = a0 =1
[6] H0 = H(t0)
[7] ΩR = 0
[8] Ωk<0, Ωk = -K, K > 0
[9] ΩM>1, ΩM = M, M > 1
[10] ΩΛ = 1-Ωk- ΩM = 1+K-M > 0 → M-1 < K

Solution
Note: I have assigned this problem to myself. I would appreciate a response that confirms that my solution is correct, or identifies one or more steps where I made a mistake.

The inequality in [29] is the solution as a final constraint on of the Ωs (in addition to
he inequalities in [8] through [10]). Below are the sequence of steps leading to [29].

Note that [1] and [4] implies that a’(s) = 0.
Using [4] through [10], [3] becomes
[11a] a’2/a2 = H02 [ M/a3 – K/a2 + (1-M+K)].

In [1] and [2], s is defined as the value of t that satisfies [1] and [2].
Note that [1] and [4] implies that
[11b] a’(s) = 0.
Let
[11c] b=a(s).
Using [11b] and [11c] simplifies [11a] to
[12] 0 = M/b3 – K/b2 + (1-M+K).
Multiplying [12] by b3 yields
[13] 0 = M – Kb + (1-M+K)b3
Equation [13] defines the specific value a=b which satisfies condition [1].

I now proceed to work with [2].
Differentiating [4] with respect to t yields
[14] H’ = a’’/a – a’2/a2 = (a’’/a - H2)
Using [1] in [14] yields
[15] a’’(s) = 0.
Multiplying [11a] by a3 yields
[16] a a’2 = H02 [M - Ka +(1-M+K)a3]
Differentiating [16] with respect to t yields
[17] a’3+2aa’a’’ = H02 [-Ka’ +3(1-M+K)a2a’]
Dividing [17] by a’ yields
[18a] a’2+2aa’’ = H02 [-K +3(1-M+K)a2]
Using [1], [11c], and [15] in [18a] yields
[18b] 0 = -K +3(1-M+K)b2
Solving [18b] for b2 yields
[19] b2 = K/(3(1-M+K)).
Inequality [10] implies that b2 is positive, so b is a real number.
Substituting [19] into [13] yields
[20] 0 = M – Kb + (K/(3(1-M+K))) (1-M+K)b]
Simplifying [20] yields
[21] M = Kb(1-(1/3)) = (2/3)Kb, which yields
[22] b = (3/2)M/K.

I will now check to confirm that [22] and [19] together are a solution of [13].
[23] b2 = (9/4) M2/K2 = K/(3(1-M+K)) yields
[24a] M2(1-M+K) = (4/27)K3, which yields
[24b] 1-M+K = (4/27)K3/M2.
Combining [24b] with [13] yields
[25a] 0 = M – Kb + ((4/27)K3/M2) b3
= M – K (3/2)M/K + ((4/27)K3/M2) (27/8)M3/K3​
= M – (3/2)M + (1/2)M​
= 0.​

Combining [19] and [22] yields
[23] (9/4) M2/K2 = K/(2(1-M+K)), yields
[24] K= (9/2)M2(1-M+K), yields
[25] K(1+(9/2)M2) = (9/2)M2, yields
[26] K = (9/2)M2 / (1+(9/2)M2) = M2/((2/9)+M2), yields
[27a] 1/K = 1 + (2/9)/M2,yields
[27b] 1/M2 = (9/2) [(1/K)-1] = (9/2)((1-K)/K), and
[28] M2 = (2/9) K/(1-K).
Equation [28] implies that
[29] K<1,
since otherwise M would not be a real number.

Combining [29] with [9] and [10] yields a summary inequality:
[30] 0 < M-1 < K < 1.

NOTE:
I have also made an effort to also show that
b > a0 = 1.​
My intuition tells me that this must be true, but I have failed to prove it. I have decided to discuss the implications of a possible
b < a0 = 1​
in a separate thread.
 
Last edited:
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  • #2
Your solution appears to be correct. You have successfully used the given equations and inequalities to derive the final constraint [29], which is a summary of the constraints on the Ωs. Your steps are clear and easy to follow.

Regarding the question of b > a0 = 1, your intuition is correct. Since b = a(s), and s is defined as the value of t that satisfies [1] and [2], it follows that b > a0 = 1. This is because [1] and [2] imply that a’(s) = 0, and therefore a(s) must be a constant function with value a0 = 1. This means that b = a(s) = a0 = 1. So, b > a0 = 1 is always true.

I hope this helps. Keep up the good work!
 

1. What is the Friedmann Equation?

The Friedmann Equation is a mathematical equation used in cosmology to describe the expansion of the universe. It takes into account the energy density and pressure of the universe to determine its rate of expansion over time.

2. What are metastatic conditions?

Metastatic conditions refer to the spread of cancer from one part of the body to another. In the context of the Friedmann Equation, it refers to the potential for the expansion of the universe to accelerate or decelerate depending on the energy density and pressure of the universe.

3. How does the Friedmann Equation relate to metastatic conditions for Omegas?

The Friedmann Equation can be used to determine the critical density of the universe, which is the energy density needed for the expansion to eventually stop. If the actual energy density of the universe is greater than the critical density, it is considered metastatic and the universe will continue to expand at an accelerating rate.

4. What are Omegas in the context of the Friedmann Equation?

Omegas refer to the different types of energy density in the universe, including matter, radiation, and dark energy. In the Friedmann Equation, these energy densities are represented by the symbols Ωm, Ωr, and ΩΛ respectively.

5. How is the Friedmann Equation used to find metastatic conditions for Omegas?

The Friedmann Equation is used to calculate the critical density of the universe, which is then compared to the actual energy density of the universe. If the actual energy density is greater than the critical density, it is considered metastatic and the universe will continue to expand at an accelerating rate due to the presence of dark energy.

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