Critical Density: H0=70km/s.MPC, Fate of Universe

In summary, the critical density of the universe is a measure of the amount of matter and energy needed for the universe to reach a steady state. It is calculated by dividing the actual density of the universe by the critical density at the present time, represented by H0=70km/s.MPC. This value is significant as it represents the current expansion rate of the universe and can determine its fate - whether it will collapse in a "Big Crunch" (if critical density is greater than 1) or continue to expand forever (if critical density is less than 1).
  • #1
b_o3
52
0
hello, can anyone help me with this problem please:

For H0=70 km/ S . MPC , what is the critical density (p0) for the universe in gm/cm^3? . if the average density of the universe is 5 * 10 ^ -28 gm/cm^3 , what is the fate of the universe.

thanks ,
 
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  • #2
You don't know ANY relevant equations? You need to make a start at a solution and prove you are stuck before anyone can help.
 
  • #3


Hello,

The critical density, p0, for the universe can be calculated using the formula p0 = 3H0^2/8πG, where H0 is the Hubble constant and G is the gravitational constant. Plugging in H0 = 70 km/s.MPC (where MPC stands for megaparsec, a unit of distance used in cosmology) and converting to proper units, we get p0 = 1.878 x 10^-29 gm/cm^3.

Comparing this to the average density of the universe, 5 x 10^-28 gm/cm^3, we can see that the average density is much lower than the critical density. This means that the universe is currently open, meaning that it will continue to expand forever.

If the average density were to somehow increase to match the critical density, the universe would be flat and would continue to expand at a constant rate. However, if the average density were to decrease even further, the universe would be open and would expand at an accelerating rate.

In summary, based on the given information, it seems that the fate of the universe is to continue expanding forever. However, this is subject to change if the average density were to change significantly in the future. I hope this helps!
 

What is the critical density of the universe?

The critical density of the universe is a measure of the amount of matter and energy in the universe that is required for it to eventually stop expanding and reach a steady state. It is represented by the symbol Ω and is typically measured in units of the critical density of the universe at the present time (H0=70km/s.MPC).

How is the critical density calculated?

The critical density is calculated by taking the ratio of the actual density of the universe to the critical density. This can be determined by measuring the amount of matter and energy in the universe and dividing it by the critical density at the present time (H0=70km/s.MPC).

What is the significance of H0=70km/s.MPC in relation to the critical density?

H0=70km/s.MPC represents the current expansion rate of the universe, known as the Hubble constant. By using this value in the calculation of critical density, we can determine the fate of the universe and whether it will continue to expand forever or eventually collapse.

What is the fate of the universe if the critical density is greater than 1?

If the calculated critical density is greater than 1, it means that the universe has enough matter and energy to eventually stop expanding and reach a steady state. This is known as a closed universe and it will eventually collapse in on itself in a "Big Crunch".

What is the fate of the universe if the critical density is less than 1?

If the calculated critical density is less than 1, it means that the universe does not have enough matter and energy to eventually stop expanding. This is known as an open universe and it will continue to expand forever.

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