Calculating the critical density

The 3.086 in the denominator is squared, so it becomes 3.086^2 = 9.52. 0.08769/9.52 = 0.00921. Hope that helps!In summary, the conversation is about calculating a value using the small h parameter, which is defined as H0 = h(100 km/s/Mpc). However, in this problem, small h has a subscript of h70, which means that H0 = h70(70 km/s/Mpc). The calculation involves converting units and cancelling out terms to obtain a final value of (0.921 x 10^-26)h70^2 kg/m^3.
  • #1
robertjford80
388
0

Homework Statement



Screenshot2012-06-01at100825PM.png



I can't get how they calculate that.

I'm not sure if there including H0 which I think is 70 or not but I've tried with and without and both don't work.

I get (3 * 70^2)/(8pi*6.67 * 10^-11) which is way off.


I also can't get the units that they arrive at

I get

km/s/Mpc * s^2/m^3kg which is

km(s)/Mpc/kg*m^3
 
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  • #2
robertjford80 said:

Homework Statement



Screenshot2012-06-01at100825PM.png
I can't get how they calculate that.

I'm not sure if there including H0 which I think is 70 or not but I've tried with and without and both don't work.

I get (3 * 70^2)/(8pi*6.67 * 10^-11) which is way off. I also can't get the units that they arrive at

I get

km/s/Mpc * s^2/m^3kg which is

km(s)/Mpc/kg*m^3

The definition of small h that I'm familiar with is that H0 = h(100 km/s/Mpc), which is useful, because now you have dimensionless constant that you can set to different values depending on how different you think H0 is in value from 100 km/s/Mpc. I think that this was especially relevant back in the day when there was a lot of uncertainty in the value of H0, and introducing this parameter allowed you to express theoretical results in terms of a dimensionless constant that could then be set to the desired value whenever this was well-determined. So in other words, you had your answer "up to" a multiplicative constant. Now we know with a fair amount of certainty that h = 0.71 (I think, or maybe 0.72, not sure what the latest and greatest value is). In other words, H0 = 71 or 72 km/s/Mpc.

All that having been said, I notice that the small h in THIS problem has a subscript: h70, which suggests to me that its definition is given by H0 = h70(70 km/s/Mpc). I.e. the assumed base value is 70 rather than 100. In fact, I have very good reason to believe that this is the case. So let's proceed with the calculation under that assumption. THen we have:$$\rho_c = \frac{3h_{70}^2}{8\pi} \frac{(70~\textrm{km} \cdot \textrm{s}^{-1} \cdot \textrm{Mpc}^{-1})^2}{G}$$ $$= \frac{3h_{70}^2}{8\pi} \frac{(7.0\times 10^4)^2~\textrm{m}^2 \cdot \textrm{s}^{-2} \cdot \textrm{Mpc}^{-2}}{6.67 \times 10^{-11}~\textrm{N}\cdot\textrm{m}^2\cdot\textrm{kg}^{-2}}$$Let's convert Newtons into SI base units:$$= \frac{3h_{70}^2}{8\pi} \frac{4.9\times10^9~\textrm{m}^2 \cdot \textrm{s}^{-2} \cdot \textrm{Mpc}^{-2}}{6.67 \times 10^{-11}~\textrm{kg}\cdot\textrm{m}\cdot\textrm{s}^{-2}\cdot\textrm{m}^2\cdot\textrm{kg}^{-2}}$$Now let's get rid of the mess of numbers by multiplying them all together. Let's also simply the units by doing as many cancellations as we can:$$=(0.08769\times 10^{20}) h_{70}^2 \frac{ \textrm{Mpc}^{-2}}{\textrm{m}\cdot\textrm{kg}^{-1}}$$The final thing that is going to be a bit of a pain in the butt is to convert square megaparsecs to square metres. I will leave it as an exercise for you to show that 1 Mpc = 3.086e22 m. Therefore, we have:$$=(0.08769\times 10^{20}) h_{70}^2 \frac{ \textrm{kg}}{\textrm{m}\cdot (3.086\times 10^{22}~\textrm{m})^{2}}$$Now, notice that the power of 10 in the numerator is 10^20, and in the denominator we have (10^22)^2 = 10^44. When we divide them, we get 10^-24. I've also multiplied all the numbers together again to obtain:

$$= (0.00921 \times 10^{-24}) h_{70}^2 \frac{ \textrm{kg}}{\textrm{m}\cdot \textrm{m}^{2}}$$Multiply by 100 and subtract 2 from the exponent (these two operations cancel each other out):$$=(0.921 \times 10^{-26}) h_{70}^2 \frac{ \textrm{kg}}{\textrm{m}^{3}}$$Close enough if you ask me!
 
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  • #3
Wow! Excellent help! You really rock! I'm just having trouble with one step:


$$=(0.08769\times 10^{20}) h_{70}^2 \frac{ \textrm{kg}}{\textrm{m}\cdot (3.086\times 10^{22}~\textrm{m})^{2}}$$

$$= (0.00921 \times 10^{-24}) h_{70}^2 \frac{ \textrm{kg}}{\textrm{m}\cdot \textrm{m}^{2}}$$

right off the bat 8.7/3.1 = 2.8 not .92 (ignoring the orders of magnitude) So it must be the case that you're doing something extra there.
 
  • #4
The 3.086 in the denominator appears squared. So we get 0.08769/3.0862=0.0092
 
  • #5
robertjford80 said:
Wow! Excellent help! You really rock! I'm just having trouble with one step:


$$=(0.08769\times 10^{20}) h_{70}^2 \frac{ \textrm{kg}}{\textrm{m}\cdot (3.086\times 10^{22}~\textrm{m})^{2}}$$

$$= (0.00921 \times 10^{-24}) h_{70}^2 \frac{ \textrm{kg}}{\textrm{m}\cdot \textrm{m}^{2}}$$

right off the bat 8.7/3.1 = 2.8 not .92 (ignoring the orders of magnitude) So it must be the case that you're doing something extra there.

Glad to be of help. As far as the above, yeah, what kloptok said.
 

Related to Calculating the critical density

What is critical density?

Critical density refers to the amount of matter and energy needed to determine the fate of the universe, specifically whether it will continue to expand or eventually collapse.

How is critical density calculated?

Critical density is calculated by dividing the average density of matter and energy in the universe by the critical density, which is approximately 10^-29 grams per cubic centimeter.

Why is calculating critical density important?

Calculating critical density can help scientists understand the structure and evolution of the universe and make predictions about its future. It can also provide insight into the amount and distribution of dark matter and dark energy.

What is the current estimated value of critical density?

The current estimated value of critical density is approximately 5 x 10^-30 grams per cubic centimeter. This value is constantly being refined as new data and observations are collected.

How does critical density relate to the concept of the "flat" universe?

If the actual density of the universe is equal to the critical density, it is considered a "flat" universe. This means that the universe will continue to expand at a steady rate and will not collapse or expand too quickly.

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