Can Triangular Forces Exist in Spacetime Lattice Structures?

In summary: The existence of these triangular forces is a manifestation of the uncertainty principle which states that certain pairs of observables (such as momentum and energy) cannot be simultaneously known to arbitrary precision. In summary, orthogonal forces are a consequence of the metric of spacetime being exactly zero. When the metric is not zero, forces can also be collinear or non-orthogonal. When the metric is the Planck length, then spacetime can be quantized into discrete rotations and the distances between points can be described using the form d_{mnl} = \sqrt{m^2 + n^2 + l^2 - c^2 t^2}.
  • #1
Antonio Lao
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If each spacetime point [itex] p_i[/itex] can be associated with a contant force [itex]f_i[/itex] then the interaction [itex] \sum_{i=1}^\infty f_i [/itex] between points can be described with the use of orthogonal forces.
 
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  • #2
Orthogonality of forces is a consequence of when the metric of spacetime is exactly zero. When the metric is zero, each point can only interact with six forces and these forces formed two sets of three orthogonal forces.

When the metric is exactly zero, spacetime is said to be continuous. And each point can only interact with orthogonal forces and with collinear forces.

When the metric is the Planck length, then spacetime can be locally quantized by its discrete twist cyclic motion and satisfying the eight directional invariance's properties.
 
  • #3
Collinearity also allows a spacetime point to interact with only six points. But because of perspective, each spacetime point can "see" all the infinite minus six points of the whole fabric of spacetime. And to interact with any of these point, for only coplanar points, distances of the form [itex] \sqrt{ n^2 + 1}[/itex] for n=1 and as n approaches infinity must exist.

The metrical value of the geodesic is assumed the value of 1.
 
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  • #4
The general formula for distances between spacetime point is given by

[tex] d_{mnl} = \sqrt{m^2 + n^2 + l^2} [/tex]

where [itex] m [/itex] and [itex] n [/itex] and [itex] l [/itex] are the indices for the orthogonal vertical and horizontal planes found in one quadrant and the orthogonal planes with indices of (0,0,0) is defined as passing through the point itself at (0,0,0).
 
  • #5
When the shortest distance (geodesic) between orthogonal planes is given the value of 1 (e.g. 1 Planck length) then nearly orthogonal forces can be assumed to exist between spacetime points. But when the geodesic is exactly zero then the scalar products of orthogonal forces are zeros even though the forces have a constant value.
 
  • #6
The constancy of these orthogonal forces forms constant accelerations at the infinitesimal domain of spacetime. These accelerations vanish when the metric is exactly zero. And to make the metric zero, a quantity of [itex]c^2 t^2 [/itex] must be subtracted from [itex] d_{mnl} [/itex]. The new expression is equivalent to the spacetime interval of Einstein's theory of special relativity.

[tex] d_{mnl} = \sqrt{ m^2 + n^2 + l^2 - c^2 t^2} [/tex]

In a separate formulation, [itex] c^2 = \vec{a} \cdot \vec{r}[/itex] and [itex] a_m r_m + a_n r_n + a_l r_l [/itex] is not identically zero. But two of the indices must be zeros, (1,0,0), (0,1,0), (0,0,1). For the case where n=0 and l=0, then

[tex] d_{m00} = \sqrt{ m^2 - m a_m t^2} [/tex]
 
  • #7
Since the indices [itex]m, n, l[/itex] take on only integer values, the distances between spacetime points are said to be quantized.
 
  • #8
To complete the structure of spacetime, the following equation is needed:

[tex] d_{0n0} = \sqrt{n^2 - n a_n t^2}[/tex]

These two distances formed a Hopf ring although individually, it's more like part of a hyperbola.

A 3rd form [itex] d_{00l} = \sqrt{l^2 - l a_l t^2}[/itex] exists and random selections by nature's choice which two forms is taken out of the three possibilities led to two distinct topologies of the dynamic Hopf ring.
 
  • #9
Because there can only be two distinct metrics ([itex] \psi_E [/itex] and [itex]\psi_B [/itex]) of spacetime, there should be only two fundamental orthogonal forces ([itex] \phi_E [/itex] and [itex] \phi_B [/itex]). In a minimum-maximum configuration, these are equivalent to the electric force and the magnetic force of the vacuum. The existence of magnetic permeability ([itex] \mu_0[/itex]) and electric permittivity ([itex]\epsilon_0 [/itex]) of the vacuum is a proof that these forces do exist.

And the vector-scalar products of these metrics and forces give the square of energy, another quantum of nature.

[tex] E^2 = \psi_E \times \phi_E \cdot \psi_B \times \phi_B [/tex]
 
  • #10
The assumption that each spacetime point carries with it a constant magnitude force raises the question about the existence of triangular forces (force configuration bounded by three spacetime points). The lattice structure of spacetime at the fundamental level indicates that the minumum bounding points is four. If there are only three points as the vertices of an equilateral triangle, the distortion of the spacetime structure becomes tremendous which will give rise to very high curvature ripping the fabric of spacetime.
 

FAQ: Can Triangular Forces Exist in Spacetime Lattice Structures?

What are orthogonal infinitesimal forces?

Orthogonal infinitesimal forces are extremely small forces that act on an object in a direction perpendicular to its motion. These forces are typically very small and are often ignored in classical mechanics, but can have significant effects on the motion of particles at the quantum level.

How do orthogonal infinitesimal forces differ from regular forces?

Orthogonal infinitesimal forces differ from regular forces in two main ways. First, they are extremely small, often on the scale of Planck's constant, and can only be observed at the quantum level. Second, they act in a direction perpendicular to the motion of the object, while regular forces act in the same direction as the object's motion.

What is the significance of orthogonal infinitesimal forces?

Orthogonal infinitesimal forces play a crucial role in quantum mechanics, as they are responsible for the quantization of energy and the behavior of particles at the subatomic level. They also help to explain the uncertainty principle and the wave-particle duality of matter.

How do scientists study orthogonal infinitesimal forces?

Scientists study orthogonal infinitesimal forces through experiments and mathematical models. These forces are too small to be directly measured, so scientists use quantum mechanics equations and principles to predict their effects on particles and compare them to experimental results.

Can orthogonal infinitesimal forces be manipulated or controlled?

Currently, there is no known way to directly manipulate or control orthogonal infinitesimal forces. However, scientists are constantly researching and developing new technologies and techniques to better understand and potentially harness the power of these forces.

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