Originally posted by maximus
now, I'm a little confused on an important fact: how close are we now in our measurment to the critical mass for the expansion? the stuff I've been studying is from the 80's or something so I'm wondering what our current estimate is.
In the 80s and 90s it was a big issue with cosmologists
whether rho was equal to rho crit-----the so-called "spatially flat" case where the universe would continue expanding (just barely) foreever.
or whether rho was greater than rho crit-----the "closed" case where the expansion would eventually end and things would fall back together in a crunch
or whether rho was less than rho crit----the "open" case where expansion would continue forever but in a brisk manner rather than the borderline "just barely not stopping" way
The critical energy density rho
crit is easy to calculate from Hubble's parameter H
0 by a formula
(3/8pi) c
4 /G H
02
but the joke was, in the 80s and 90s they didnt know H
0 at all well. there were widely differing measurments of it.
Around 1998 it all came together and there was a terrific change, people call it a revolution, in cosmology.
They got an accurate H
0 value of 1/13.8 billion years.
And they discovered at last that the universe was spatially flat. That is the real rho is equal to the critical rho needed for flatness.
this would have been an enormous solace and relief to cosmologists except that at the same time (around 1998)
they discoverd that 73 percent of the energy density (the nice rho they had determined so carefully) was nothing anybody had ever seen so far called "dark energy". The name means nothing, they could as well call it X energy because nobody has a clue what it is. This means that cosmology is probably the greatest standup comedy act in the whole history of science---but also
in a certain way the most interesting that it could possibly be.
a contant source of headline news and entertainment.
So rho turned out to equal rho crit, after all, but 73 percent of rho is dark energy.
AFTERTHOUGHT your books may talk about Ω which is
the rieal rho divided by rho crit.
Another way to desribe the three cases is to ask if
Ω = 1 (flat case)
Ω > 1 (closed case)
Ω < 1 (open case)
it is just the same spiel but with trivially different notation