| 3 equations and 1 inequality -
11-05-2007, 02:11 PM
equation 1: P = K|a| – N/S
equation 2: a·r=c=|a||r|cosq=c
equation 3: E=F1´r1·F2´r2= F1·r2F2·r1-F1·F2r1·r2= -(F1·F2r1·r2- F1·r2F2·r1)
inequality 1:Dr·Dp³h/2p
P is the gravity pressure; K is the dimensional ratio of local acceleration of gravity g and the universal constant of gravitation G, a is the generalized absolute acceleration of spacetime, N is the normal force which is also equal to mg, where m is the inertial mass, S is the surface area to the normal, r is the infinitesimal spacetime metric, c is the speed of light, E is the energy and F is the primary force, p is the linear momentum, and h is Planck’s constant of action.
The purpose of this set of equations and inequality is to unify general relativity and quantum mechanics to which a simple theoretical computation agrees with the observed radius of the visible universe.
Time independence: [∂E(g)]²=[∂F(a)×∂r(a)]·[∂F(b)×∂r(b)] and Mass independence: ¶a(t)·¶r(t)=c²
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