Submitted:
11 August 2023
Posted:
14 August 2023
Read the latest preprint version here
Abstract
Keywords:
1. Background and Introduction
2. Materials and Method
2.1. Curved area of λm,n-vacuum

x′1(а) = α10(а)x0(а) + α11(а)x1(а) + α12(а)x2(а) + α13(а)x3(а);
x′2(а) = α20(а)x0(а) + α21(а)x1(а) + α22(а)x2(а) + α23(а)x3(а);
x′3 (а) = α30(а)x0(а) + α31(а)x1(а) + α32(а)x2(а) + α33(а)x3(а),
e′1(a) = β10(a) e0(a) + β11(a) e1(a) + β12(a) e2(a) + β13(a) e3(a);
e′2(a) = β20(a) e0(a) + β21(a) e1(a) + β22(a) e2(a) + β23(a) e3(a);
e′3(a) = β30(a) e0(a) + β31(a) e1(a) + β32(a) e2(a) + β03(a) e3(a),
2.2. Curved metric 4-spaces
2.3. The first stage of compactification of curved measurements
<ds(– – + –)2> <ds(+ + – –)2> <ds(– + – –)2> <ds(+ – + –)2>
<ds(– + + +)2> <ds(– – – – )2> <ds(+ + + –)2> <ds (– + + –)2>
<ds(+ + – +)2> <ds(– – + +)2> <ds(+ – + +)2> <ds(– + – +)2>,
Recall that the “vacuum balance condition” was formulated in the introduction of the article [1], and this is the basic statement that, in particular, no matter what convex-concave curvatures (fluctuations) occur with the local area of the λm,n-vacuum, on average over the entire area they are equal to zero.
2.4. The second stage of compactification of curved mathematical measurements
(– – – +) + (+ + + –) =0
(+ – – +) + (– + + –) =0
(– – + –) + (+ + – +) =0
(+ + – –) + (– – + +) =0
(– + – –) + (+ – + +) =0
(+ – + –) + (– + – +) =0
(+ – – –)+ + (– + + +)+ =0
Recall that the two-sided model of λm,n-vacuum, that is, the result of averaging complex metric-dynamic fluctuations of λm,n-vacuum to a two-sided level of consideration, is called in §2.7 in [2] “23-λm,n-vacuum”, because in this case, only 4 + 4 = 8 = 23 mathematical measurements remain within the framework of consideration.
- -
- subcont (i.e., the substantial continuum or the outer side of the 23-λm,n-vacuum with the averaged metric (30) and with the signature (+ – – –) of the Minkowski space);
- -
- antisubcont (i.e., antisubstantial continuum or inner side of 23-λm,n-vacuum with averaged metric (33) and signature (– + + +) of Minkowski antispace).


Reference systemsХУ orХ′У′ on two opposite sides of a sheet of paper have different stignatures, respectively {+ +} and {+ –}. To understand this, take a sheet of paper and draw on it the XY reference system (as inFigure 8a). Then turn the sheet over, and on its reverse side depict theХ′У′ reference system in the same way in the same place. If you compare these reference systems, you will find that the X and X′ axes are directed in different directions, so their stignatures are different.
2.5. Four-strain tensor of 23-λm,n-vacuum in the case of a simplified two-sided consideration
2.5.1. Four-strain tensors of two sides of 23-λm,n-vacuum
2.5.2. The 4-strain tensor of 23-λm,n-vacuum in the case of two-sided consideration
Below, a k-braid is the result of averaging metrics with different signatures (where k is the number of averaged metrics, i.e., the number of “threads” in the “braid”). For example, the averaged metric (61) is called a 2-braid, since it is “twisted” from 2 lines (“threads”): ds(+) = ds (+ – – –) and ds(–) = ds(– + + +).
2.5.3. The 4-strain tensor of a curved 26-λm,n-vacuum in the case of sixteen-sided consideration
+ ds(– – + –)2 + ds(+ + – –)2 + ds(– + – –)2 + ds(+ – + –)2 +
+ ds(– + + +)2 + ds(– – – – )2 + ds(+ + + –)2 + ds(– + + –)2 +
+ ds(+ + – +)2 + ds(– – + +)2 + ds(+ – + +)2 + ds(– + – +)2).
+ η5 ds(– – + –) + η6 ds(+ + – –) + η7 ds(– + – –) + η8 ds(+ – + –) +
+ η9 ds(– + + +) + η10 ds(– – – –) + η11 ds(+ + + –) + η12 ds (– + + –) +
+ η13 ds(+ + – +) + η14 ds(– – + +) + η15 ds(+ – + +) + η16 ds(– + – +).
Yellow (– – – +) + (+ + + –) Аnti-yellow
Orange (+ – – +) + (– + + –) Аnti-orange
Green (– – + –) + (+ + – +) Аnti-green
Blue (+ + – –) + (– – + +) Аnti-blue
Dark blue (– + – –) + (+ – + +) Аnti-dark blue
Violet (+ – + –) + (– + – +) Аnti-violet
White (+ – – –)+ + (– + + +)+ BlackBlack
6. Physical meaning of the components of the metric tensor
6.1. Nonzero components of the metric tensor

2.6.2. Zero components of the metric tensor
Under the kinematics of vacuum layers is meant such a section of geometrized vacuum physics based on the Algebra of Signatures (Alsigna), in which the displacements (movements) of different sides of theλm,n-vacuum are considered independently of their deformations. With a more consistent approach, i.e. during the development of the dynamics of vacuum layers in subsequent articles of this cycle, it turns out that any displacement of the local region of one layer ofλm,n-vacuum is inevitably accompanied by its curvature. This, in turn, sets in motion the curvature of other adjacent layers of theλm,n-vacuum. At the same time, and vice versa, the curvature of the local region of one layer of theλm,n-vacuum is necessarily accompanied by its displacement (i.e., flow), which leads to a disturbance of all adjacent layers. In what follows, interconnected flows and curvatures of local sections of different layers of theλm,n-vacuum are considered as multidimensional 4-deformations using the mathematical apparatus of the general theory of relativity.
| i | j | k | (88) | |
| i | –1 | k | –j | |
| j | –k | 1 | i | |
| k | j | –i | –1 |
t′′ = t, x′′ = x cosΩ t – y sinΩ t,
z′′ = z, y′′ = x sinΩ t + y cosΩ t.
2.7. Predictions of the kinetics of vacuum layers
2.7.1. The limiting speed of movement of 23-λm,n-vacuum layers
2.7.2. Inert properties of layers of 23-λm,n-vacuum
2.7.3. Kinematics of the rupture of the local section of the 23-λm,n-vacuum
3. Conclusions
Acknowledgments
References
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- Batanov-Gaukhman, M. (2023) “Geometrized vacuum physics. Part II. Algebra of Signatures“. [CrossRef]
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