Olivia Grace
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Do we know what the critical density of the universe is? I always thought we did know, but apparently (according to friend) we don't...
The discussion centers around the critical density of the universe, exploring its calculation and implications in cosmology. Participants engage in mathematical reasoning and conceptual clarification regarding the energy density of the universe, referencing the Friedmann equation and the Hubble parameter.
Participants do not reach a consensus on the exact value of the critical density, with multiple calculations and interpretations presented. There is also disagreement regarding the implications of dark matter and dark energy in relation to the critical density.
Participants acknowledge limitations in their calculations, including assumptions about the values of constants and the implications of an expanding universe on the critical density. There are unresolved steps in the conversion processes discussed.
Olivia Grace said:Do we know what the critical density of the universe is? I always thought we did know, but apparently (according to friend) we don't...
Olivia Grace said:Thanks very much, that's really helpful!
One thing,
"the usual figure for the Hubble parameter, at present, is 71 km/second per Mpc which is a bit messy "
How did you boil this down to the 1/13.8 billion years? I'm having trouble converting the units to SI ones...
Your help is muchly appreciated!
marcus said:the inverted Hubble parameter is One Mpc/ (71 km/s)
so that is 3.0857 x 10^18 km/(71 km/s) and kilometers cancel so it's ( (3.0857 x 10^19 )/71) seconds