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Sizzle

Subject: Sizzle
From: Jack Sarfatti
Date: Thu, 01 Dec 2005 20:57:21 GMT
Newsgroups: sci.space, sci.astro, sci.physics.relatiivity, sci.math, sci.physics
"Einstein's [static 1917] model ... was unstable like a pencil balancing on its point ... In 1929 Edwin Hubble showed that the universe was expanding." Einstein missed his big chance to have predicted what Hubble found since it was there in his theory.

"Inflation ... Alan Guth's 1981 theory ... offered an explanation for why the initial conditions in the big bang should be approximately but not exactly uniform ... the fundamental forces ... have different strengths ... in the very early universe ... the cosmological constant - the energy density of the vacuum - could also be different in that early phase." p. 165

This requires the torsion field extension of Einstein's 1915 theory because there

Guv + /\guv = 0

in vacuum before there is any real matter.

Guv^;v = 0 Bianchi identity

guv^;v = 0 metricity

Therefore

/\^,v = 0

i.e. /\ the cosmological constant is really a constant as well as being uniform.

When there is real matter we can have

(string tension)/\^,vguv  + Tuv^;v(Matter) = 0

So that creation of on-mass-shell real matter will also cause the cosmological constant to go non-uniform and dynamic, (i.e. to change it from a constant to a variable) even without torsion. However, torsion allows the cosmological constant to go non-uniform and dynamic without creating real matter that is a nuisance for the practical metric engineering of warp and wormhole. Of course the ET Aliens visiting us have figured all this out.

Guth assumed that the dark zero point energy density was positive and enormous at the creation of our local "past light cone" universe in the multiverse that has an infinity of parallel worlds.

"My Father's House has many mansions." Rabbi Yeshua

De Sitter (also in 1917) "wondered what would happen if a universe had a cosmological constant and nothing else."

That is very close to our actual universe BTW, which is 96% variable cosmological field in which 73% is positive zero point energy density and 23% is negative zero point energy density. Only 4% is real matter and radiation on mass shell and less than 1/4 of that 4% is star stuff and us. We have only really known this since 2002 with any real precision. It took all the Pundits by surprise. The DeSitter spacetime "looks like the surface of an infinite hourglass ... a closed three-sphere universe starting out in the infinite past with infinite size, contracting at nearly the speed of light. The repulsive effect of the cosmological constant causes this [space] contraction to slow down and then reverse. The universe reaches a minimum size, then starts to expand, slowly at first but then faster and faster, eventually approaching the velocity of light ... particles ... their clocks tick slower and slower ... the universe expands more and more between ticks ... the [passive test] particles "see" the circumference of the universe growing exponentially as a function of their own clock time ... Special relativity just stipulates that two objects cannot [locally in coincidence] pass each other [in near collision] faster than the speed of light. Nothing in special relativity prevents the space between two objects stretching so fast that a light beam could not ever cross the expanding distance between them. (p. 168) ... The circumference of the De Sitter space at its waist can be ... 10^-33 cm ... this universe would look just like a big bang ... Eventually the high [zero point] density decayed into the normal vacuum ... into hot thermal radiation ... Guth now understood why the big bang would be so uniform. Regions that have had time to trade light signals should equilibrate to the same temperature ... as the universe inflates ... these regions pass out of causal contact with each other [becoming space-like separated out of each other's local light cones] ... But after the inflationary vacuum decays the expansion slows and these regions come into contact again ... As ... Bill Press has noted, they say hello, goodbye, and then hello again" - like meeting an old girlfriend after many years. Will the old romantic sizzle return? Tune in to the next episode. :-)


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