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World Hologram Strong Short Range Gravity
Posted:
Sep 27, 2007 7:55 PM


Dvali's etal work on extra space dimensions arrives at Abdus Salam's 1973 fgravity 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 EinsteinCartan gravity tetrad 1form 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 noninertial frames, A^a =/= 0 in such a GNIF. A^a = 0 in a GIF.
For a GNIF R^a^b = 0 (vanishing curvature 2form) and T^a = 0 (vanishing torsion 2form)
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 etal 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 cBITS
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 11 hologram correspondance between each area hologram quantum and it's projected "volume without volume" hologram image quantum.
Conjecture
a = N^1/3
b = &r



