My calculation of the density of the universe at (10^60)th of its present age

In summary, the conversation discusses calculations involving the distance traveled by light since the Big Bang, the Planck length, and the density of the universe. It also raises questions about the properties of the universe at early time epochs and the accuracy of these calculations.
  • #1
kmarinas86
979
1
If you divide the distance light traveled since the Big Bang by the Planck length, you get a factor of 8.17722722*10^60.

((1 / (70 ((km / s) / Mpc))) * (1 (light year / year))) / sqrt(((h / (2 * pi)) * G) / (c^3)) = 8.17722722 * 10^60

If you cube this value, you get the factor by which the volume was smaller.

(((1 / (70 ((km / s) / Mpc))) * (1 (light year / year))) / sqrt(((h / (2 * pi)) * G) / (c^3)))^3 = 5.4678702 * 10^182

Try dividing the Planck density by the current density of the universe.

(5.1 * ((10^96) (kg / (m^3)))) / (5 * ((10^(-30)) (g / (cm^3)))) = 1.02 × 10^123

Presumably, the density of the universe would have to be greater than the Planck density at Planck time, by almost 60 orders of magnitude. But scientists say otherwise. Knowing that the scientists are more likely to be right than I, can somebody explain why this result is different by almost 60 orders of magnitude? Does the Planck density ignore radiation and only consider massive particles?

As an aside question, how would you calculate the electric permittivity and magnetic permeability of the universe at Planck time?
 
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  • #2
You are reaching back to the Planck wall, where all bets are off regarding the properties of the universe.
 
  • #3

1. What is the significance of calculating the density of the universe at 10^60th of its present age?

Calculating the density of the universe at this particular time allows us to understand the evolution and expansion of the universe. It gives us insights into the early stages of the universe and helps us better understand its current state.

2. How is the density of the universe at 10^60th of its present age calculated?

The density of the universe is calculated by using various observations and measurements, such as the cosmic microwave background radiation, the distribution of galaxies, and the expansion rate of the universe. These data are then plugged into mathematical models and equations to determine the density at a specific time.

3. What is the current estimated density of the universe?

The current estimated density of the universe is approximately 9.9 x 10^-30 grams per cubic centimeter. This value is known as the critical density, which is the density needed for the universe to eventually stop expanding and collapse.

4. How does the density of the universe at 10^60th of its present age compare to its current density?

The density of the universe at 10^60th of its present age is significantly higher than its current density. This is because the universe was much denser in its early stages, and has been expanding and diluting over time.

5. What implications does the calculated density of the universe at 10^60th of its present age have on our understanding of the universe?

The calculated density of the universe at this time provides evidence for the Big Bang theory and supports the concept of an expanding universe. It also helps us understand the formation of structures, such as galaxies and clusters, as well as the distribution of matter in the universe.

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