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Hubble constant |
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| Jun8-03, 02:46 PM | #1 |
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Hubble constant
I see often that rhocrit(the critical density of matter), is expressed this way:
rhocrit=(3*(H^2))/(8*pi*G) This is not correct because a cosmological constant is missed. This is the Friedmann Equation: H^2=((8*pi*G*rhocrit)/3)+(lambda/3)-(k/(a^2)) Since it is known that the curvature(k)of the universe is zero, the Friedmann equation can be reduced to this: H^2=((8*pi*G*rhocrit)/3)+(lambda/3) and rhocrit is: rhocrit=(3*((H^2)-(lambda/3)))/(8*pi*G) Now, i would like to solve this equation. I have a value for rhocrit of 10^(-26)kg/m^3, but i need the value of the cosmological constant to complete the equation. You know the value? (in SI units, please) also given that H=((da/dt)/da), being a the scale factor and H=Hubble constant, it would be nice to know the current value of the scale factor [:D] |
| Jun8-03, 03:32 PM | #2 |
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It can be written as a mass density equivalent------kilograms per cubic meter Or, by including a c^2, it can be written as an energy density----joules per cubic meter. The actual energy density of the universe is now believed to be equal to rho crit---or very nearly---so that the universe is spatially flat. The cosmological constant (sometimes referred to as dark energy term) is believed to represent around 73 percent of the total rho. |
| Jun8-03, 03:42 PM | #3 |
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Last time I looked at rho crit in SI units it was, I believe,
0.83 joules per cubic kilometer. the cosmological constant is usually given as a percentage----nowadays typically 73 percent of that. So you just do 0.73 of 0.83 and get 0.61 joules per cubic kilometer. Your figure is probably just 0.83 joules divided by the square of the speed of light (to give a kilogram equivalent) and rounded off---which is fine since there is plenty of uncertainty. |
| Jun8-03, 05:09 PM | #4 |
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Hubble constant |
| Jun8-03, 06:06 PM | #5 |
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| Jun8-03, 09:03 PM | #6 |
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if the "Hubble Constant" were in fact constant the Universe would expand in an exponential fashion. Which doesn't seem very likely! So I just call it the Hubble Value.
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| Jun8-03, 09:09 PM | #7 |
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| Jun8-03, 10:34 PM | #8 |
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The Hubble parameter is a variable thing. The Hubble constant is the value of the Huble parameter at the present moment
H^2=((8*pi*G*rho)/3)+(lambda/3)-(k/(a^2)) http://super.colorado.edu/~michaele/Lambda/evol.html http://www.blackwell-synergy.com/lin...2.43110.x/html What represents rho in this equation? |
| Jun8-03, 11:16 PM | #9 |
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| Jun8-03, 11:50 PM | #10 |
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H^2=((8*pi*G*rho)/3)+(lambda/3)-(k/(R^2)) and here, rho represents the TRUE density of energy but not the CRITICAL density of energy. Ok? I don't know what you mean with "unnecesary". Do you mean that if I erase (lambda/3) of the equation, then it all remains good? |
| Jun9-03, 12:06 AM | #11 |
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| Jun9-03, 12:32 AM | #13 |
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One thing, Marcus use to write the critical energy density in this way:
rhocrit=(3*(c^2)*(H^2))/(8*pi*g) but if you look at the Friedmann equation, eliminating (lambda/3) and eliminating (k/(R^2)), because k is zero, then the Friedmann equation is simply: rho=(3*(H^2))/(8*pi*g) and given that omega=rho/rhocrit=1 I think that Marcus should erase c^2 of the formula |
| Jun9-03, 07:12 AM | #14 |
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| Jun9-03, 02:50 PM | #15 |
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Bravo A+ and thanks for responding to Meteor about my post. I had to be off the net for much of yesterday and was glad to see you were taking care of business.
*********** |
| Jun9-03, 09:40 PM | #16 |
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The olive branch lives. |
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