On 2/18/2017 10:18 AM, John Clark wrote:
On Fri, Feb 17, 2017 at 11:19 PM, Brent Meeker <meeke...@verizon.net <mailto:meeke...@verizon.net>> wrote

    ​> ​
    The cosmological constant appears as an integration constant in
    solutions to Einstein's equations.
    ​


​Yes, so mathematically it could have any value including zero. ​

    ​> ​
    It would be good to know more about the CC, but we actually "know"
    more about it than we do about dark matter.

The Cosmological Constant​​ amount
​s​
​​ to a repulsive effect that comes​ ​from space itself, and
​ ​
you can set that constant to anything and mathematically the field​ ​equations of General Relativity would still work​ just fine​. Originally Einstein​ ​saw no physical reason for that additional complication so he set it to​ ​zero. But then he noticed that if it was zero the universe could not be​ ​stable,

No, he saw that it could not be in equilibrium. He put in the CC and gave it a value that balanced the gravitational attraction of the observed matter so that the system was in equilibrium. However, he didn't notice that it was an unstable equilibrium - a very elementary mistake.

it must be expanding or contracting
​ ​
and​ at the time everybody​ ​including Einstein thought the universe was stable so he set it to a non​ ​zero value and the cosmological constant was born. However just a few​ ​years later Hubble found the universe was expanding, so Einstein​ ​thought the cosmological constant no longer had a purpose and said that​ ​changing it from zero was the greatest mistake of his life.​
​​

Right. Einstein was a genius who was so smart that when the thought he made a mistake, he was wrong.



​Then​ people working with quantum mechanics found that empty space​ ​should indeed have a repulsive effect, but the numbers were huge,​ ​gigantic astronomical, so large that the universe would blow itself
​ ​
apart in
​much​
less than a billionth of a​ trillionth of a​ nanosecond. This was clearly a nonsensical result but most felt that once a quantum theory of gravity was discovered a way would be found to cancel this out and the true value of the cosmological constant would be zero.

​But then​
just a few years ago it was observed that the universe is not just expanding but accelerating, so now theoreticians must find a way to cancel out, not the entire cosmological constant, but the vastly more difficult task of canceling it all out *EXCEPT* for one part in 10^120. There are only about 10^90 atoms in the observable universe.
​ Nobody has a clue how to do this.​

Actually there are several ideas about how to do this - but none that have been worked out to the point of being testable. One is my friend Vic Stenger's idea that one should take the Bekenstein bound on entropy seriously and apply it to the Hubble volume. The 10^120 number comes from assuming that each quantum field contributes zero-point energy down to de Broglie wavelengths as small as the Planck length, L. But the holographic principle can yield a value close the the observed.

http://journals.aps.org.secure.sci-hub.ac/prl/pdf/10.1103/PhysRevLett.89.081301

This is not generally accepted at "the solution" because it seems to imply the wrong equation of state for inflation; but there may be ways around this:

https://arxiv.org/pdf/hep-th/0403052.pdf

Sean Carroll has considered this in his review article https://arxiv.org/abs/astro-ph/0004075v2

/More generally, it is now understood that (at least in some circumstances) string theory// //obeys the “holographic principle”, the idea that a theory with gravity in D dimensions// //is equivalent to a theory without gravity in D−1 dimensions [148, 149]. In a holographic// //theory, the number of degrees of freedom in a region grows as the area of its boundary,// //rather than as its volume. Therefore, the conventional computation of the cosmological// //constant due to vacuum fluctuations conceivably involves a vast overcounting of degrees// //of freedom. We might imagine that a more correct counting would yield a much smaller// //estimate of the vacuum energy [150, 151, 152, 153], although no reliable calculation//
//has been done as yet

/Brent/
/


 John K Clark




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