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On Topological Invariants of Inner Sheaf and Outer Sheaf Universe

POSTER

Abstract

We found there exist important topological dimensionless parameters, which control all evolution and deformation of the Universe. These topological invariants include:

(i) Newton's gravitational constant G = 2/3 = 0.666666..., its physically measured value G' = 0.667428 × 10-10 m3 kg-1 s-2;

(ii) reduced Planck constant h = 2π√3 = 10.882796..., its physically measured value h' = 10.54571817 × 10-35 joule. s ;

(iii) Boltzmann constant kB = 8√3 = 13.856406..., its physically measured value kB' = 13.80649 ×10-24 joule K-1;

(iv) recently we found that the Quantum Speed Limit Θ = 4.

These topological parameters construct the theoretical framework of modern quantum physics, and govern all evolution and deformation of inner-outer sheaf universe.

We know that ratio kB / h = 8√3 / 2π√3 = 4/π which means that there exists a zero section with a circle S1 (perimeter is 2π√3) and with a square (perimeter is 8√3). Then its maximum span is a called great circle with radius R = 2 which leads to a short proof on the QSL = 4. In fact, the QSL is an important criterion associated with inner-outer sheaf universe. For example, if a coherent radius rcoh < 2 = √Θ, there is a canonical retract deformation √3 which has a characteristc equation: u2 - u + 1= 0. Its solutions are u =1/2 ± i √3, then u1 - u2 = rcoh=√3. According the General Newton's Lows (Zhi-An Luan, 2019 CAP Congress), its mass m = √(1- rcoh2) = √(1 - 3/4) = 1/2. Since Gmv = Id =1, then G = 1/(3/2)= 2/3 = 0.666666.... This is a case of the Solar system.

if rcoh > 2 = √Θ, there is a exotic escape deformation √5 which has a characterestic equation: φ2 - φ - 1 = 0. Its solutions are φ = 1/2 ± √5 /2, e.i. φ1 = 1.618, φ2 = - 0.618 which are called golden ratio. Notes that escape velocity from the Earth vescape= √5 /2 = 1.11804, its physically measured value v'escape = 1.1186 km/s. rcoh= √5 or v = 5 means that its mass m = √(1- 5/4) = √(-1/4) = i/2 which is a complex number as Tachiyon particles. This Black-Hole is called energy-over class v > 4. We have another Black-Hole which is called mass-over class: m = √5 /2 greater than critical mcrit = √3 /2. The mass-over Black-Hole has velocity: vBH = 4(1- mBH2) = 4√(1-5/4) = 4×(-1/4) = -1, which means the mass-over escape Black-Hole has an opposite direction. We can compute escape angle of Black-Hole: θ1 = tan-1(√5) = 65o9 > tan-1(√3) = 60o. Another escape angle of Black-Hole: θ2 = tan-1(1/√5) = 24o1 < tan-1(1/√3) = 30o.

Presenters

  • Zhi an Luan

    China University of Petroleum, East China

Authors

  • Zhi an Luan

    China University of Petroleum, East China