01 January 1970 24 352 Report

If it is true that space-time is expanding, how does the measure of space-time change?

The shape of space-time is the shape of the universe; how can expansion without a boundary be called expansion? If the boundary of spacetime is the boundary of the universe, can spacetime expansion with a boundary have no background? How is the boundary maintained? If the boundary of spacetime is infinite, how does it expand?

We will use these paired terms to describe spacetime: infinite/finite, absolute/relative*, flat/curved, continuous/discrete, four-dimensional†/higher-dimensional, and so on. Normally we think of these properties as opposites ‡ and only one or the other can be chosen. But the full range of properties of spacetime will be combinations between these different properties. For example, spacetime has infinite, absolute, continuous, flat, four-dimensional properties, or spacetime has finite, discrete properties, etc. In any case, none of us thinks that there is a concept of "multiple spacetimes", or that spacetime should have its own background, or that spacetime can overlap, although physics suggests that there may be local "warps" in spacetime.

Astronomical observations show that the universe is in a process of accelerated expansion [1][2][3], with all stars moving away at an accelerated rate and possibly never returning. Physics attributes the expansion of space-time to the presence of dark energy with negative pressure [4]. Dark energy has been hypothesized in various ways (including non-existence), one of which is the cosmological constant Λ in Einstein's field equations (the zero-point radiation of space [5], the energy of the vacuum, the zero-point energy [6]).

Physics has not exactly explained the exact relationship between spacetime and the various fields assumed by the Standard Model [7], but only assumes the existence of vacuum energy [8][6], and is not sure which field's vacuum energy it is, whether it is the electromagnetic field, the electron field, the muon field, or the up-quark field, the charm-quark field, the Higgs field [9], or just the sum of their respective vacuum energies. So when it is assumed that space-time is expanding, and vacuum energy is expanding, are they created in it, or are they diffused across the boundary? Are they the driving force or the result? How do they manifest within microscopic particles when expanding at high speeds on the macroscopic scale?

Physics does not explain the origin of the dynamics of the Big Bang, nor does it explain when and how all the various fields in the Standard Model were formed, how they were formed, how they were maintained in existence, and how they evolved along with, or determined, the evolution of the Universe throughout the entire evolution of the Universe from the Big Bang onward. It is not clear how the various particles were excited initially from their own fields, but the explanation of nucleosynthesis [10] to the current period is relatively clear.

Usually we think of the universe as a set of space-time and matter-energy. There are many different models of the universe, and in addition to the Standard Model, there are many cyclic universes and multiverse views [11][15]. Then, when we haven't confirmed the model of the universe, there is no confirmed goal of the evolution of the universe, and there is no confirmed shape and boundary of the universe.

Both Einstein and Hawking say that the universe is "finite and unbounded" [12]. They believe that the universe is a finite three-dimensional sphere with a finite volume but no boundary. Topological theory says, "The boundary of a region has no boundary itself. "** [13]. Wheeler's statement is, "The boundary of a boundary is zero" [14]. What is the result of the infinite extension of the three orthogonal coordinate axes for a finite three-dimensional spherical universe?

Mathematically, there are four combinations between measures and boundaries: finite bounded, infinite unbounded, finite unbounded, and infinite bounded. The first two concepts are clear, but the latter two need to be recognized carefully when translated to physics. The "singularity" is a typical example of an "infinite bounded". Usually in physics, when time or space shrinks to zero, the corresponding physical quantity tends to infinity. For example, E=hν, when ν→0; F=q1*q2/r^2, when r→0. However, we believe that this is only a trend and that there can be no state that reaches a singularity. Therefore, "infinitely bounded" is not real. The Koch Curve, often thought of as a fractal geometry expressing "finite unbounded", is one of the nth iterations of the Koch snowflake that can be implemented in the Wolfram Language as KochCurve[n]¶. The difference between physical reality and mathematics can be shown here, as n cannot be chosen to be infinite, so the Koch Curve will always be in a definite state in reality, and although it can evolve, "finite and unbounded" is a tendency, not a state. The formulation of the Mobius strip††, the irrational numbers, is another way of saying "finite unbounded". In physics, a typical example of "finite unbounded" is the electron. The electron has a fixed charge e, but the boundary of the electric field E of the charge extends infinitely (the field strength is convergent). Of course, the concept of zero-dimensional "point particles" is also a kind of abstract "finite unbounded". In short, in physical terms, finite must have boundaries.

General relativity is the basis for modeling the universe, but is there any good reason why we should be able to determine the evolutionary goals of the universe, its shape, and its boundaries through general relativity alone? Shouldn't such boundaries be "boundary conditions" of GR?

There should not be any boundary conditions, which are the conditions necessary for the model of the universe to hold correctly.

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Notes

* cf, https://www.researchgate.net/publication/373877548_Convergent_and_Disperse_Cyclic_Multiverse_Model_CDCMM.

† cf, https://www.researchgate.net/post/NO1_Can_This_Be_an_Argument_for_3-D_Space;

‡ As long as we do not have a precise definition of spacetime, viewing these properties as opposites can only be taken for granted. As with the wave-particle duality of particles, which property is presented depends on the observer's perspective; the structure of the particle itself does not change. Further characterizations of spacetime include whether it is inherently existent or generative, whether the vacuum contains energy, and so on.

¶ https:// mathworld.wolfram.com/KochSnowflake.html; Stephen Wolfram, Founder of Wolfram Language, is very interested in the question of the evolution of the universe, and is the author of the book "a new kind of science", which has been trying to find out how the universe evolves using metacellular automata.

** e.g. the two-dimensional region has as its boundary a one-dimensional loop; the loop has no end, that is, it has no boundary itself.

†† The Möbius strip is bounded as long as one does not confuse metrics with boundaries.

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References

[1] Linder, E.V., Exploring the expansion history of the universe. Physical Review Letters, 2003. 90(9): p. 091301.

[2] Riess, A.G., The expansion of the Universe is faster than expected. Nature Reviews Physics, 2020. 2(1): p. 10-12.

[3] Freedman, W.L., The Hubble constant and the expansion age of the Universe. Physics Reports, 2000. 333: p. 13-31.

[4] "Dark Energy Survey, Collaboration." from https://www.darkenergysurvey.org/the-des-project/overview/.

[5] Oks, E. (2021). "Brief review of recent advances in understanding dark matter and dark energy." New Astronomy Reviews 93: 101632.

[6] Carroll, S. M., W. H. Press and E. L. Turner (1992). "The cosmological constant." Annual review of astronomy and astrophysics 30: 499-542.

[7] Group, P. D., P. Zyla, R. Barnett, J. Beringer, O. Dahl, D. Dwyer, D. Groom, C.-J. Lin, K. Lugovsky and E. Pianori (2020). "Review of particle physics." Progress of Theoretical and Experimental Physics 2020(8): 083C001.

[8] Jaffe, R. L. (2005). "Casimir effect and the quantum vacuum." Physical Review D 72(2): 021301.

[9] Springer (2020). 100 Years of Fundamental Theoretical Physics in the Palm of Your Hand: Integrated Technical Treatment.

[10] Cyburt, R. H., B. D. Fields, K. A. Olive and T.-H. Yeh (2016). "Big bang nucleosynthesis: Present status." Reviews of Modern Physics 88(1): 015004.

[11] Carr, B. and G. Ellis (2008). "Universe or multiverse?" Astronomy & Geophysics 49(2): 2.29-22.33.

[12] Hawking, S. W. and M. Jackson (2001). A brief history of time, Bantam Books New York.

[13] Yang, C. N. (1980). "Einstein's impact on theoretical physics." Physics Today 33(6): 42-49.

[14] Misner, C. W., K. S. Thorne and J. A. Wheeler (2017). GRAVITATION, Princoten University Press.

[15] https://www.researchgate.net/publication/373877548_Convergent_and_Disperse_Cyclic_Multiverse_Model_CDCMM.

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