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Topic: World Hologram Strong Short Range Gravity
Replies: 2   Last Post: Sep 27, 2007 9:41 PM

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Jack Sarfatti

Posts: 1,942
Registered: 12/13/04
World Hologram Strong Short Range Gravity
Posted: Sep 27, 2007 7:55 PM
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Dvali's et-al work on extra space dimensions arrives at Abdus Salam's
1973 f-gravity that in the static Newtonian limit is simply for the
gravity potential energy per unit test particle

V(r) = -(GM/r)(1 + ae^-r/b)

In my world hologram tetrad model, the Einstein-Cartan gravity tetrad
1-form field is conjectured to be

e^a = I^a + N^-1/3A^a

ds^2(1916GR) = e^ae^a = guvdx^udx^v

I^aIa is ds^2(1905SR) in which only global inertial frame (GIF)
transformations are allowed.

As soon as one allows global non-inertial frames, A^a =/= 0 in such a
GNIF. A^a = 0 in a GIF.

For a GNIF R^a^b = 0 (vanishing curvature 2-form) and T^a = 0 (vanishing
torsion 2-form)

In 1916 GR localize rigid T4 to elastic T4(x) and now in general R^a^b
=/= 0 but T^a = 0 still.

In the Jack Ng et-al world hologram conjecture for simple SSS vacuum model

4pir^2 = NLp^2/4

r = Schwarzschild radial coordinate for static LNIF observers when r >
2GM/c^2, M = source mass energy

Lp^2 = hG/c^3

N = number of Bekenstein c-BITS

r = N^1/2Lp/16pi

The size of the quantum gravity foam bubble is

&r ~ (Lp^2r)^1/3 ~ N^1/6Lp/16pi

Therefore r^3/&r^3 ~ N^3/2/N^1/2 ~ N

Therefore, there is a 1-1 hologram correspondance between each area
hologram quantum and it's projected "volume without volume" hologram
image quantum.


a = N^1/3

b = &r

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