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A Novel Framework for Characterizing Spacetime Microstructure with Scaling

Weihu Ma(马维虎) ID [email protected]    Yu-Gang Ma(马余刚) ID [email protected] Key Laboratory of Nuclear Physics and Ion-beam Application (MOE), Institute of Modern Physics, Fudan University, Shanghai 200433, China Shanghai Research Center for Theoretical Nuclear Physics, NSFC and Fudan University, Shanghai 200438, China
Abstract

The study of physics at the Planck scale has garnered significant attention due to its implications for understanding the fundamental nature of the universe. At the Planck scale, quantum fluctuations challenge the classical notion of spacetime as a smooth continuum, revealing a complex microstructure that defies traditional models. This study introduces a novel scaling-based framework to investigate the properties of spacetime microstructures. By deriving a scaling-characterized metric tensor and reformulating fundamental equations—including the geodesic, Einstein field, Klein-Gordon, and Dirac equations—into scaling forms, the research reveals new properties of local spacetime dynamics. Remarkably, the golden ratio emerges naturally in linear scale measurements, offering a potential explanation for the role of the Planck length in resolving ultraviolet (UV) divergence. Furthermore, the study demonstrates how scale invariance in spacetime can restore classical geometric stability through the renormalization group equations. These findings significantly revise classical geometric intuitions, providing a fresh lens for understanding quantum fluctuations and offering promising insights for advancing quantum gravity theories.

Planck scale\sepspacetime Microstructure\sepQuantum fluctuation\sepscaling-characterized metric tensor\sepgolden section

I Introduction

The Planck length is particularly significant, as it is the scale at which quantum gravitational effects are expected to become apparent, thus interactions require a working theory of quantum gravity to be studied. It is also a natural estimate for the fundamental string length scale and the characteristic size of compact extra dimensions bibitem1 . At the Planck scale, current models fail to describe the universe effectively, and a scientific model to explain the behavior of the physical universe has yet to be established. Our current understanding suggests that the universe began 1043\sim 10^{-43} seconds after the Big Bang. At this scale, the uncertainty principle reveals the quantum fluctuations of spacetime, which are integral to elucidating the original structure of the universe, the center of a black hole, and the structure of nature at a very short scale, in a framework of quantum gravity bibitem2 .

Many studies seek to address these challenges in quantum gravity, including two of the most potential of them, i.e., Loop Quantum Gravity (LQG) and String Theory. LQG is an approach to quantum gravity that quantizes spacetime itself by describing it in terms of discrete loops or spin networks bibitem2 ; Gambini ; Ashtekar ; Thiemann ; Pullin . It provides a non-perturbative and background-independent framework, where space is quantized, and the geometry emerges from the quantum states of the gravitational field. LQG introduces a new set of variables and applies loop quantization techniques, leading to finite areas and volumes, and avoiding singularities such as those in black holes Gambini2 . String Theory posits that the fundamental constituents of the universe are not point particles, but rather one-dimensional “strings” that vibrate at different frequencies to produce different particles. It provides a unified framework for all fundamental forces, including gravity, by incorporating the concept of extra dimensions and supersymmetry Zwiebach ; bibitem1 ; LeBihan . String Theory has successfully incorporated gravity into quantum mechanics, offering a potential solution to the problem of quantum gravity and explaining the existence of different particle types through string vibrations Vaid . Recent research in quantum gravity reveals various new approaches and theories Klauder ; Oriti ; Berenstein ; Pullin ; Shojai ; Carlip ; Harlow ; Pawlowski ; Braunstein ; Giesel ; King ; Bajardi ; Chakraborty ; Saueressig ; Bianchi . Although these studies have greatly improved our understanding of physics at the Planck scale, they are obviously not exhaustive.

Due to its incompleteness, quantum gravity imposes constraints on our understanding of spacetime at the smallest scales. This challenge has piqued the interest of many researchers who are drawn to the field in pursuit of unraveling its mysteries. At this scale, spacetime is hypothesized to deviate from the classical notion of a smooth continuum, potentially exhibiting a foam-like, fluctuating structure bibitem3 ; bibitem4 . This concept is rooted in the idea that the Heisenberg uncertainty principle could give rise to microscopic irregularities, as postulated by Wheeler. Additionally, Tryon’s hypothesis suggests that our universe may have originated from a quantum vacuum fluctuation, similar to the Big Bang scenario bibitem5 . Quantum fluctuations are not just theoretical curiosities but integral to the fabric of the universe’s microstructure. The significance of these fluctuations is underscored by ongoing research that highlights the necessity for a deeper exploration into the foundational characteristics of spacetime at the Planck scale. This quest for understanding is driven by the goal of reconciling the principles of quantum mechanics with the geometry of spacetime, with the ultimate goal of revealing the true nature of reality at its most fundamental level.

The Planck scale represents a frontier in theoretical physics, where quantum fluctuations dominate, and classical descriptions of spacetime become inadequate. The present work aims to explore the microstructure of spacetime at the Planck scale through micro-measurements of spacetime characterized by scaling functions. By examining the scaling behavior of micro-geometry, the research aims to provide a new perspective for exploring the nature of spacetime microstructures and offer valuable insights into fundamental spacetime properties. We develop a novel scaling-characterized metric tensor derived from the Lorentz scalar line element, enabling the analysis of spacetime microstructure. The differential operators are transformed into scaling form, providing a mathematical framework for examining fluctuation properties. The content is structured as follows: II. Micro-measuring principle and Scaling Characterization; III. Scaling Characterization in Metric; IV. The Lorentz Factor at the micro-scale; V. Micro Measurement in Spacetime with Schwarzschild Metric; VI. Scaling Geodesic Equations and Einstein Field Equations; VII. The Golden Ratio at the micro-scale; VIII. Scaling Klein-Gordon Equation and Dirac Equation; IX. Summary.

II Micro-measuring Principle and Scaling Characterization

Heisenberg’s principle suggests that spacetime exhibits quantum fluctuations on a microscopic scale. These fluctuations result in uncertainties in the positions of points within spacetime coordinates and cause variations in microlengths. At the Planck scale, traditional concepts of spacetime geometry become inadequate due to quantum fluctuations. These fluctuations imply that spacetime is not a smooth manifold but has a more intricate structure.

We model the spacetime fluctuations using the differential dxαdx^{\alpha}, representing spacetime microelements as microlength measurements relative to a reference length dx0αdx^{\alpha}_{0}. Here, α\alpha (equal to 0, 1, 2, 3, …) denotes the coordinate index in orthonormal frames. The microelements represent small segments of spacetime, making it a natural choice for modeling fluctuations at quantum scales, where spacetime might exhibit complex, non-continuous behavior. In quantum mechanics, uncertainty and fluctuations are inherent due to the Heisenberg uncertainty principle. Modeling spacetime at quantum scales involves accounting for these uncertainties, which microelements naturally accommodate by allowing for the representation of small changes and variations. Defining spacetime quantum fluctuations using differentials dxαdx^{\alpha} is a rational choice that fits well with current theoretical frameworks in physics. It allows for a coherent description of spacetime at very small scales, integrating principles of general relativity and quantum mechanics. This definition provides a useful starting point for exploring the quantum nature of spacetime.

The measurements of dxαdx^{\alpha} relative to dx0αdx^{\alpha}_{0} is introduced by arbitrary scaling functions:

rlα=dxαdx0α=Lα(Xα(τ)).r_{l^{\alpha}}=\frac{dx^{\alpha}}{dx^{\alpha}_{0}}=L^{\alpha}(X^{\alpha}(\tau)). (1)

These scaling functions Lα(Xα(τ))L^{\alpha}(X^{\alpha}(\tau)) suggest a way to quantify these quantum fluctuations, denoted by spacetime scales XαX^{\alpha}, and quantify how the microlength measurements deviate from their reference lengths due to quantum fluctuations. dx0αdx^{\alpha}_{0} are micro reference lengths, serving as the baseline measurements in the absence of fluctuations. It establishes a well-defined reference scale that allows us to measure the deviations. To measure the micro proper length, scaling function τ\tau(X(s)) is introduced and defined as

rl=dλdλ0=τ(X(s))\displaystyle r_{l}=\frac{d\lambda}{d\lambda_{0}}=\tau(X(s)) (2)

in a similar way, where dλd\lambda is the proper length microelement, dλ0d\lambda_{0} is the reference length, and ss is defined as the proper time scale.

Consequently, the measurements of dxαdx^{\alpha} relative to proper length dλd\lambda is given by

dxαdλ=Lα(Xα(τ))τ(X(s))dx0αdλ0=Lα(Xα(τ))τ(X(s)),\displaystyle\frac{dx^{\alpha}}{d\lambda}=\frac{L^{\alpha}(X^{\alpha}(\tau))}{\tau(X(s))}\cdot\frac{dx^{\alpha}_{0}}{d\lambda_{0}}=\frac{L^{\alpha}(X^{\alpha}(\tau))}{\tau(X(s))}, (3)

which involves choosing consistent reference lengths for dx0αdx^{\alpha}_{0} = dλ0d\lambda_{0}. The Planck length is considered the optimal reference length as it represents the smallest measurable length scale in quantum gravity, making it a natural choice for investigating spacetime at this scale.

With these definitions, there are three types of spacetime micro measurements:

(a), When Lα=constantL^{\alpha}=constant (τ=constant\tau=constant), indicating that micro length measurements are conducted in a static mode (trivial measurement) without fluctuations, independent of XαX^{\alpha}(XX), indicating a perfectly stable spacetime region. When measurements are performed exclusively along a single dimension, the non-fluctuating mode can be represented as Lα=1L^{\alpha}=1 as the constantconstant can be incorporated into the reference length through appropriate scaling.

(b), When Lα=K1αXα+K2αL^{\alpha}=K^{\alpha}_{1}X^{\alpha}+K^{\alpha}_{2} (τ=K1X+K2\tau=K_{1}X+K_{2}), micro length measurements are generally performed in a linear fluctuating mode, where Kα(K)K^{\alpha}(K) are coefficients. This suggests a linear relation between the microlength and their fluctuation. When measurements are performed exclusively along a single dimension, the linear fluctuating mode can be represented as Lα=XαL^{\alpha}=X^{\alpha} as the coefficients can be incorporated into the reference length through translation and scaling.

(c), When Lα=Lα(Xα)L^{\alpha}=L^{\alpha}(X^{\alpha}) (τ=τ(X)\tau=\tau(X)) are nonlinear functions, micro length measurements occur in a nonlinear fluctuating mode.

Micro measurements might involve complex scaling functions, or even discrete rather than continuous measurements, leading to distinct spacetime structures. The exploration of these forms is crucial for a more comprehensive view of spacetime microstructure.

In this framework, spacetime fluctuation measurement can be described by the scaling function with non-trivial measurement. Additionally, the fluctuation induced by XαX^{\alpha} signifies micro structures along the α\alpha-axis. If the given LαL^{\alpha} is the same for all axes, it indicates an isotropic structure.

Define dx¯α=L¯αdx0α=Lα(ζαXα)dx0αd\bar{x}^{\alpha}=\bar{L}^{\alpha}dx^{\alpha}_{0}=L^{\alpha}(\zeta^{\alpha}X^{\alpha})dx^{\alpha}_{0} with ζα(τ)\zeta^{\alpha}(\tau) being the αaxis\alpha-axis rescaling factor of scale transformation. And also define dλ¯=τ¯dλ0=τ(χX)dλ0d\bar{\lambda}=\bar{\tau}d\lambda_{0}=\tau(\chi X)d\lambda_{0} with χ(s)\chi(s) being the rescaling scale transformation on X(s)X(s). Then we can get

d2xαdλ2\displaystyle\frac{d^{2}x^{\alpha}}{d\lambda^{2}} =ddλ(dxαdλ)=1dλ(dx¯αdλdxαdλ)\displaystyle=\frac{d}{d\lambda}(\frac{dx^{\alpha}}{d\lambda})=\frac{1}{d\lambda}(\frac{d\bar{x}^{\alpha}}{d\lambda}-\frac{dx^{\alpha}}{d\lambda}) (4)
=L¯αLατ21dλ0,\displaystyle=\frac{\bar{L}^{\alpha}-L^{\alpha}}{\tau^{2}}\frac{1}{d\lambda_{0}},

and the change of rlαr_{l^{\alpha}} relative to rlr_{l} is

drlαdrl\displaystyle\frac{dr_{l^{\alpha}}}{dr_{l}} =dx¯αdxαdλ¯dλ=L¯αLατ¯τ.\displaystyle=\frac{d\bar{x}^{\alpha}-dx^{\alpha}}{d\bar{\lambda}-d\lambda}=\frac{\bar{L}^{\alpha}-L^{\alpha}}{\bar{\tau}-\tau}. (5)

From d(dxα)=dx¯αdxα=(dx¯αdxα1)dxα=(L¯αLα1)dxαd(dx^{\alpha})=d\bar{x}^{\alpha}-dx^{\alpha}=(\frac{d\bar{x}^{\alpha}}{dx^{\alpha}}-1)dx^{\alpha}=(\frac{\bar{L}^{\alpha}}{L^{\alpha}}-1)dx^{\alpha} and d(dxα)=dLαdXαdXαdx0αd(dx^{\alpha})=\frac{dL^{\alpha}}{dX^{\alpha}}dX^{\alpha}dx_{0}^{\alpha}, we get

dXαdxα=a^α1dx0α\displaystyle\frac{dX^{\alpha}}{dx^{\alpha}}=\hat{a}_{\alpha}\frac{1}{dx_{0}^{\alpha}} (6)

with

a^α=L¯α/Lα1dLα/dXα,\displaystyle\hat{a}_{\alpha}=\frac{\bar{L}^{\alpha}/L^{\alpha}-1}{dL^{\alpha}/dX^{\alpha}}, (7)

thus we have the first and second-order partial differential operators transformed in scaling form by

xν=dXνdxνXν=1dx0νa^νXν,\displaystyle\frac{\partial}{\partial x^{\nu}}=\frac{dX^{\nu}}{dx^{\nu}}\frac{\partial}{\partial X^{\nu}}=\frac{1}{dx_{0}^{\nu}}\hat{a}_{\nu}\frac{\partial}{\partial X^{\nu}}, (8)
2xμxν\displaystyle\frac{\partial^{2}}{\partial x^{\mu}\partial x^{\nu}} =dXμdxμXμ(xν)=1dx0μ1dx0ν\displaystyle=\frac{dX^{\mu}}{dx^{\mu}}\frac{\partial}{\partial X^{\mu}}(\frac{\partial}{\partial x^{\nu}})=\frac{1}{dx_{0}^{\mu}}\frac{1}{dx_{0}^{\nu}} (9)
(a^μa^ν2XμXνa^μb^νXνXμXν),\displaystyle\cdot(\hat{a}_{\mu}\hat{a}_{\nu}\frac{\partial^{2}}{\partial X^{\mu}\partial X^{\nu}}-\hat{a}_{\mu}\hat{b}_{\nu}\frac{\partial X^{\nu}}{\partial X^{\mu}}\frac{\partial}{\partial X^{\nu}}),

where

b^ν=da^νdXν.\displaystyle\hat{b}_{\nu}=-\frac{d\hat{a}_{\nu}}{dX^{\nu}}. (10)

Eq. (8) and (9) connect with the differential operators to scaling functions, which are introduced to describe how the fluctuation of spacetime microelement can be adjusted according to a scaling factor ζν\zeta^{\nu}. These equations introduce the factors a^ν\hat{a}_{\nu} and b^ν\hat{b}_{\nu} that modify the behavior of differential operators to account for changes in scale.

Similarly, introduce a scale transformation factor χ\chi acting on X(s)X(s). And from d(dλ)=dλ¯dλ=(τ¯τ1)dλd(d\lambda)=d\bar{\lambda}-d\lambda=(\frac{\bar{\tau}}{\tau}-1)d\lambda and d(dλ)=dτdXdXdλ0d(d\lambda)=\frac{d\tau}{dX}dXd\lambda_{0}, we can get dXdλ=a^1dλ0\frac{dX}{d\lambda}=\hat{a}\frac{1}{d\lambda_{0}}. Thus, we get the first and second-order differential operators transformed in scaling form by

ddλ=dXdλddX=1dλ0a^ddX,\displaystyle\frac{d}{d\lambda}=\frac{dX}{d\lambda}\frac{d}{dX}=\frac{1}{d\lambda_{0}}\hat{a}\frac{d}{dX}, (11)
d2dλ2=dXdλddX(ddλ)=1[dλ0]2(a^2d2dX2a^b^ddX),\displaystyle\frac{d^{2}}{d\lambda^{2}}=\frac{dX}{d\lambda}\frac{d}{dX}(\frac{d}{d\lambda})=\frac{1}{[d\lambda_{0}]^{2}}(\hat{a}^{2}\frac{d^{2}}{dX^{2}}-\hat{a}\hat{b}\frac{d}{dX}), (12)

where a^=τ¯/τ1dτ/dX\hat{a}=\frac{\bar{\tau}/\tau-1}{d\tau/dX} and b^=da^dX\hat{b}=-\frac{d\hat{a}}{dX}.

Introducing the scale transformation X¯α=ζαXα\bar{X}^{\alpha}=\zeta^{\alpha}X^{\alpha} with rescaling factor ζα=ζα(Xα)\zeta^{\alpha}=\zeta^{\alpha}(X^{\alpha}), we obtain dX¯αdXα=ζα+XαdζαdXα\frac{d\bar{X}^{\alpha}}{dX^{\alpha}}=\zeta^{\alpha}+X^{\alpha}\frac{d\zeta^{\alpha}}{dX^{\alpha}} and dXαdX¯α=1ζα\frac{dX^{\alpha}}{d\bar{X}^{\alpha}}=\frac{1}{\zeta^{\alpha}}. Subsequently, this leads to the derivation of

X¯α=dXαdX¯αXα=1ζαXα;\displaystyle\frac{\partial}{\partial\bar{X}^{\alpha}}=\frac{dX^{\alpha}}{d\bar{X}^{\alpha}}\frac{\partial}{\partial X^{\alpha}}=\frac{1}{\zeta^{\alpha}}\frac{\partial}{\partial X^{\alpha}}; (13)
2X¯βX¯α=dXβdX¯βXβ(X¯α)\displaystyle\frac{\partial^{2}}{\partial\bar{X}^{\beta}\partial\bar{X}^{\alpha}}=\frac{dX^{\beta}}{d\bar{X}^{\beta}}\frac{\partial}{\partial X^{\beta}}(\frac{\partial}{\partial\bar{X}^{\alpha}}) (14)
=1ζβ1ζα2XβXα{1ζβ[ζα]2dζαdXα}XαXβXα.\displaystyle=\frac{1}{\zeta^{\beta}}\frac{1}{\zeta^{\alpha}}\frac{\partial^{2}}{\partial X^{\beta}\partial X^{\alpha}}-\{\frac{1}{\zeta^{\beta}[\zeta^{\alpha}]^{2}}\frac{d\zeta^{\alpha}}{dX^{\alpha}}\}\frac{\partial X^{\alpha}}{\partial X^{\beta}}\frac{\partial}{\partial X^{\alpha}}.

Eq. (13) and (14) use the idea of scale transformations by focusing on partial derivatives of scaled coordinates. These equations describe how spacetime coordinates are rescaled using the factor ζα\zeta^{\alpha}. This rescaling is crucial for analyzing how measurements adapt in transitioning between a linear and a nonlinear scaling regime when considering together Eq. (8) and (9), which will be further explained in the following sections VI-VIII.

Similarly, the transformation can be introduced for X¯=χX\bar{X}=\chi X with rescaling factor χ=χ(X)\chi=\chi(X). Thus dX¯dX=χ+XdχdX\frac{d\bar{X}}{dX}=\chi+X\frac{d\chi}{dX} and dXdX¯=1χ\frac{dX}{d\bar{X}}=\frac{1}{\chi}. Subsequently, we obtain

ddX¯=dXdX¯ddX=1χddX;\displaystyle\frac{d}{d\bar{X}}=\frac{dX}{d\bar{X}}\frac{d}{dX}=\frac{1}{\chi}\frac{d}{dX}; (15)
d2dX¯2=dXdX¯ddX(ddX¯)=1[χ]2d2dX21[χ]3dχdXddX.\displaystyle\frac{d^{2}}{d\bar{X}^{2}}=\frac{dX}{d\bar{X}}\frac{d}{dX}(\frac{d}{d\bar{X}})=\frac{1}{[\chi]^{2}}\frac{d^{2}}{dX^{2}}-\frac{1}{[\chi]^{3}}\frac{d\chi}{dX}\frac{d}{dX}. (16)

The introduction of these transformations establishes a mathematical framework for investigating the nature of spacetime at the micro-scale, which is further explored in the subsequent sections.

Micro-measuring principle at micro-scale: the distance between two infinitesimally close points in spacetime is denoted by dxdx, and its distance measurement requires definition through a comparison with a reference length. If dxdx remains unchanging, the measured value only relies on the chosen reference length. We can establish a consistent spacetime measurement and facilitate comparisons of their respective lengths by selecting an appropriate fixed-length reference for measuring the distance. In cases where the micro distance dxdx in spacetime undergoes fluctuations for some reason, the measurement of dxdx, relative to the reference length, is introduced as the scaling function. In the framework of quantum gravity theory, the reason for the fluctuations of spacetime microelements is considered to come from the quantum effects of spacetime at the microscopic scale, which can be inferred through the Heisenberg uncertainty principle. The measurement of microelements in quantum gravitational spacetime can be defined as fluctuating, including linear and nonlinear fluctuations. The spacetime microelement, defined by scaling functions, allows for the exploration of spacetime microstructure. This conceptualization enables the development of new mathematical tools and theories to investigate the nature of spacetime at the micro-scale.

III Scaling Characterization in Metric

The Lorentz scalar line element, also known as the spacetime invariant interval, is a fundamental concept in the theory of relativity. It measures the infinitesimal distance between two events in spacetime. It is significant due to its invariance under Lorentz transformations, meaning it remains constant for all observers, regardless of their relative motion. This invariance is a cornerstone of Einstein’s theory of relativity, ensuring that the laws of physics are the same in all inertial frames of reference.

The Lorentz scalar line element is crucial for maintaining the consistency of physical laws across all scales. It provides a foundational framework for understanding both macroscopic and microscopic phenomena, preserving spacetime’s geometric and causal properties across different observational perspectives. Kothawala Kothawala introduces the concept of a ”zero-point” length, suggesting that even at the smallest scales, the Lorentz scalar line element plays a significant role in defining the geometric properties of spacetime. As described by Volovik Volovik , it is linked to fundamental constants like the Planck length, acting as a natural ”zero-point” length. This connection is vital for exploring theories that aim to unify general relativity and quantum mechanics at the Planck scale. The Lorentz scalar line element helps characterize quantum fluctuations by providing a consistent metric that remains invariant under transformations, aiding in the interpretation of quantum behaviors.

The most general form of the Lorentz scalar line element is given by

dλ2\displaystyle d\lambda^{2} =gαβdxαdxβ,\displaystyle=g_{\alpha\beta}dx^{\alpha}dx^{\beta}, (17)

where gαβg_{\alpha\beta} is the metric tensor, and the Einstein notation is used. The potential fluctuating nature of spacetime at small scales can be studied using the invariant interval. Utilizing the scaling representation defined in previous equations, we derive an equation for the metric tensor related to micro-measurements of spacetime fluctuations

τ2(s)dλ02\displaystyle\tau^{2}(s)d\lambda^{2}_{0} =gαβLα(τ)Lβ(τ)dx0αdx0β\displaystyle=g_{\alpha\beta}L^{\alpha}(\tau)L^{\beta}(\tau)dx^{\alpha}_{0}dx^{\beta}_{0} (18)

with Einstein notation used. When τ=τC\tau=\tau_{C}, Lα=LCαL^{\alpha}=L^{\alpha}_{C}, and Lβ=LCβL^{\beta}=L^{\beta}_{C} are ConstantsConstants respectively, we define a static measurement as

τC2\displaystyle\tau_{C}^{2} =gαβLCαLCβ,\displaystyle=g_{\alpha\beta}L^{\alpha}_{C}L^{\beta}_{C}, (19)

in a consistent choice of dλ0=dx0α=dx0βd\lambda_{0}=dx^{\alpha}_{0}=dx^{\beta}_{0}. This indeed corresponds to the definition of the classical Lorentz scalar line element. Consequently, for a non-static measurement, we have

τ2(X(s))\displaystyle\tau^{2}(X(s)) =gαβLα(Xα(τ))Lβ(Xβ(τ)),\displaystyle=g_{\alpha\beta}L^{\alpha}(X^{\alpha}(\tau))L^{\beta}(X^{\beta}(\tau)), (20)

with the consistent choice of dλ0=dx0α=dx0βd\lambda_{0}=dx^{\alpha}_{0}=dx^{\beta}_{0}.

Define the micro measurement of proper time to be rt=dtdt0=rt(s)r_{t}=\frac{dt}{dt_{0}}=r_{t}(s) with reference time length dt0dt_{0}. Here ss is the defined proper time scale. Introduce light speed measurement of dλdt=rcdλ0dt0=rc(ν)dλ0dt0\frac{d\lambda}{dt}=r_{c}\frac{d\lambda_{0}}{dt_{0}}=r_{c}(\nu)\frac{d\lambda_{0}}{dt_{0}} from scale transformation of τ=rl=rcrt\tau=r_{l}=r_{c}\cdot r_{t}. ν=ν(s)\nu=\nu(s) is defined as speed scale and a function of ss. Thus we can get

rc2\displaystyle r_{c}^{2} =gαβLαLβrt2\displaystyle=g_{\alpha\beta}\frac{L^{\alpha}L^{\beta}}{r_{t}^{2}} (21)

with Einstein notation.

Define proper speed measurements from rvα=rlαrt=Lαrt=Uα(Vα(s))r_{v^{\alpha}}=\frac{r_{l^{\alpha}}}{r_{t}}=\frac{L^{\alpha}}{r_{t}}=U^{\alpha}(V^{\alpha}(s)). For space components, rvi=Ui(Vi(s))=rlirt=rlircrTrcrTrt=vircrcrTrt=vircrl0rt=vircrv0r_{v^{i}}=U^{i}(V^{i}(s))=\frac{r_{l^{i}}}{r_{t}}=\frac{r_{l^{i}}}{r_{c}r_{T}}\frac{r_{c}r_{T}}{r_{t}}=\frac{v^{i}}{r_{c}}\frac{r_{c}r_{T}}{r_{t}}=\frac{v^{i}}{r_{c}}\frac{r_{l^{0}}}{r_{t}}=\frac{v^{i}}{r_{c}}r_{v^{0}}, where rcrT=rl0=rv0rtr_{c}r_{T}=r_{l^{0}}=r_{v^{0}}r_{t} and then the coordinate speed measurement vi=rlirTv^{i}=\frac{r_{l^{i}}}{r_{T}} with rTr_{T} being the measurement of the coordinate time micro interval. Using Eq. (21), Thus we have

rc2\displaystyle r_{c}^{2} =rc2(ν(s))=gαβUα(Vα(s))Uβ(Vβ(s))\displaystyle=r_{c}^{2}(\nu(s))=g_{\alpha\beta}U^{\alpha}(V^{\alpha}(s))U^{\beta}(V^{\beta}(s)) (22)

with Einstein notation.

Performing differentiation on both sides of Eq. (20) with respect to ss, we aim to find how the metric tensor and scaling components evolve as time scale ss changes. Thus, we obtain

0\displaystyle 0 =dτds(dgαβ/dτgαβ2τ+dLα/dτLα+dLβ/dτLβ)gαβLαLβ\displaystyle=\frac{d\tau}{ds}(\frac{dg_{\alpha\beta}/d\tau}{g_{\alpha\beta}}-\frac{2}{\tau}+\frac{dL^{\alpha}/d\tau}{L^{\alpha}}+\frac{dL^{\beta}/d\tau}{L^{\beta}})g_{\alpha\beta}L^{\alpha}L^{\beta} (23)

with Einstein notation. This equation governs how the metric tensor evolves under scaling transformations, showing the intricate dependencies between derivatives of scale variables and the metric. The terms represent a balance between metric changes and scaling influences, indicating that the metric must adjust to maintain consistency in spacetime geometry under scaling.

Under conditions of Lα0L^{\alpha}\neq 0, Lβ0L^{\beta}\neq 0, and dτ/ds0d\tau/ds\neq 0, we get equations for cases of gαβ0g_{\alpha\beta}\neq 0

dgαβ/dτgαβ\displaystyle\frac{dg_{\alpha\beta}/d\tau}{g_{\alpha\beta}} =2τdLα(τ)/dτLα(τ)dLβ(τ)/dτLβ(τ).\displaystyle=\frac{2}{\tau}-\frac{dL^{\alpha}(\tau)/d\tau}{L^{\alpha}(\tau)}-\frac{dL^{\beta}(\tau)/d\tau}{L^{\beta}(\tau)}. (24)

The conditions Lα0L^{\alpha}\neq 0 and Lβ0L^{\beta}\neq 0 ensure that the microelements being measured are non-zero on the chosen scale. Such constraints help prevent ultraviolet (UV) divergence, ensuring the physical validity of the model bibitem1 ; bibitem2 . dτ/ds0d\tau/ds\neq 0 ensures that τ(s)\tau(s) varies with ss in a non-trivial way. This condition ensures that τ(s)\tau(s) is not a constant function but varies with the parameter ss. Physically, this means that the system is evolving or changing over time or space, representing a fluctuating mode in space or time scales. If dτ/ds=0d\tau/ds=0, τ(s)\tau(s) would be constant, implying no change or evolution, which would trivialize the analysis. These conditions ensure that the metric tensor and scaling behavior described by Eq. (24) are physically meaningful. They allow the equation to capture the dynamic, non-trivial structure of spacetime at microscopic scales, where quantum effects and scaling laws significantly influence spacetime geometry. After integral Eq. (24), we get

gαβ\displaystyle g_{\alpha\beta} =καβτ2LαLβ,\displaystyle=\kappa_{\alpha\beta}\frac{\tau^{2}}{L^{\alpha}L^{\beta}}, (25)

where gαβ=gβαg_{\alpha\beta}=g_{\beta\alpha}, and καβ\kappa_{\alpha\beta} are integral constant and satisfy the relation of

Σα,βκαβ=1.\displaystyle\Sigma_{\alpha,\beta}\kappa_{\alpha\beta}=1. (26)

IV The Lorentz factor at the micro-scale

According to the equivalence principle of general relativity bibitem8 ; bibitem9 ; bibitem10 , the influence of a gravitational field is locally indistinguishable from an inertial frame, meaning the laws of physics reduce to those of special relativity in a sufficiently small local region. This principle allows the use of a local inertial frame where gravitational effects can be approximately neglected. Consequently, in such a locally inertial frame, the metric tensor gαβg_{\alpha\beta} can be approximated by the flat spacetime metric ηαβ\eta_{\alpha\beta}. Therefore, in a local inertial frame or even in a flat spacetime, καβ\kappa_{\alpha\beta} in a D-dimensional flat spacetime with metric gαβ=ηαβg_{\alpha\beta}=\eta_{\alpha\beta} can be determined. Here, ηαβ=(±,1,,1)\eta_{\alpha\beta}=(\pm,\mp 1,...,\mp 1) is the D-dimensional Minkowski spacetime metric for time-like and space-like interval bibitem11 .

In the realm of physics, special relativity bibitem12 ; bibitem13 provides a framework for understanding how time and space are perceived differently by observers in relative motion. The Lorentz factor is a key component of this theory, quantifying the degree of time dilation and length contraction experienced by objects moving at significant fractions of the speed of light. However, at the microscopic scale, where quantum effects play a crucial role, the influence of spacetime fluctuations on these relativistic effects becomes a fascinating subject of study Lieu1 ; Jacobson ; Abdo ; Zimdahl ; Maziashvili ; Lieu2 . This exploration seeks to extend the understanding of the Lorentz factor by incorporating the impact of quantum fluctuations, offering a nuanced view of how intrinsic measurements of space and time behave at the quantum level. By examining a scenario involving microscopic length measurements along a given spatial axis, we delve into the interplay between relativity and quantum mechanics, introducing scale parameters to capture the essence of intrinsic measurements in a D-dimensional space.

In special relativity, the Lorentz factor describes the relativistic effects on time and length measurements due to an object’s velocity. At the micro-scale, where quantum effects become significant, we explore how spacetime fluctuations influence this factor. We consider a scenario where a microscopic length is measured at a velocity v1v^{1} along a given spatial axis ii-axis (i=1, 2, 3, …, D-1, chose i=1i=1). We introduce the scale parameter ςi=σi/τ\varsigma^{i}=\sigma^{i}/\tau with σi\sigma^{i} representing the micro space length measurement along the i-axis in the rest frame, i.e., representing the intrinsic measurements. Let τ\tau denote the micro proper length measurement. Thus, the micro intrinsic measurements in a D-dimensional space can be defined as:

σα=(τ,σi)=(τ,ςiτ).\displaystyle\sigma^{\alpha}=(\tau,\sigma^{i})=(\tau,\varsigma^{i}\tau). (27)

in an instantaneous rest frame. For the relativistic length contraction effect, we have:

rl1\displaystyle r_{l^{1}} =ς1τ1[v1]2[v0]2\displaystyle=\varsigma^{1}\tau\sqrt{1-\frac{[v^{1}]^{2}}{[v^{0}]^{2}}} (28)

with v1=rl1rT=rv1rcrv0=ς1rc/γLtz2v^{1}=\frac{r_{l^{1}}}{r_{T}}=\frac{r_{v^{1}}\cdot r_{c}}{r_{v^{0}}}=\varsigma^{1}r_{c}/\gamma_{Ltz}^{2} and v0=rcv^{0}=r_{c}. For the relativistic time dilation effect, we have:

rl0rc=rt/1[v1]2[v0]2\displaystyle\frac{r_{l^{0}}}{r_{c}}=r_{t}/\sqrt{1-\frac{[v^{1}]^{2}}{[v^{0}]^{2}}} (29)

Here, the Lorentz factor γLtz=1/1[v1]2[v0]2\gamma_{Ltz}=1/\sqrt{1-\frac{[v^{1}]^{2}}{[v^{0}]^{2}}}. Thus we derive equations

{ϑ0=11ϑ1ϑ0;ϑ1=[ς1]2(1ϑ1ϑ0),\begin{cases}\vartheta^{0}=\frac{1}{1-\frac{\vartheta^{1}}{\vartheta^{0}}};\\ \vartheta^{1}=[\varsigma^{1}]^{2}(1-\frac{\vartheta^{1}}{\vartheta^{0}}),\end{cases} (30)

where ϑ1=[rl1τ]2=[rv1rc]2\vartheta^{1}=[\frac{r_{l^{1}}}{\tau}]^{2}=[\frac{r_{v^{1}}}{r_{c}}]^{2} and ϑ0=[rl0τ]2=[rv0rc]2\vartheta^{0}=[\frac{r_{l^{0}}}{\tau}]^{2}=[\frac{r_{v^{0}}}{r_{c}}]^{2}. The solutions are:

{(ϑ11,ϑ10)=(11+4[ς1]22,11+4[ς1]22);(ϑ21,ϑ20)=(1+1+4[ς1]22,1+1+4[ς1]22).\begin{cases}(\vartheta^{1}_{1},\vartheta^{0}_{1})=(\frac{-1-\sqrt{1+4[\varsigma^{1}]^{2}}}{2},\frac{1-\sqrt{1+4[\varsigma^{1}]^{2}}}{2});\\ (\vartheta^{1}_{2},\vartheta^{0}_{2})=(\frac{-1+\sqrt{1+4[\varsigma^{1}]^{2}}}{2},\frac{1+\sqrt{1+4[\varsigma^{1}]^{2}}}{2}).\end{cases} (31)

From (ϑ21,ϑ20)(\vartheta^{1}_{2},\vartheta^{0}_{2}) with considering positive solutions, The Lorentz factor is then given by:

γLtz2=11ϑ21ϑ20=12(1+1+4[ς1]2).\displaystyle\gamma_{Ltz}^{2}=\frac{1}{1-\frac{\vartheta^{1}_{2}}{\vartheta^{0}_{2}}}=\frac{1}{2}(1+\sqrt{1+4[\varsigma^{1}]^{2}}). (32)

The form and structure of Eq. (30) render it particularly suitable to be interpreted as an iterative equation, as it demonstrates how a system can approximate a state through recursive calculations under specific conditions. The value of ϑ0\vartheta_{0} depends on the preceding value of ϑ1\vartheta_{1}, and conversely, the value of ϑ1\vartheta_{1} depends on the preceding value of ϑ0\vartheta_{0}. This interdependence creates a recursive or cyclic relationship. Through repeated iterations, one can observe whether ϑ0\vartheta_{0} and ϑ1\vartheta_{1} converge towards a stable value, known as a fixed point. The two solutions in Eq. (31) represent fixed points, with the positive one being a stable point, as determined by analyzing the Jacobian matrix. It provides a framework for modeling the evolution of a system over time through successive calculations. This iterative process helps in approaching a system’s state under specific conditions, emphasizing the recursive relationships in spacetime dynamics and highlighting the mutual dependency between ϑ0\vartheta_{0} and ϑ1\vartheta_{1}, which are scaling variables associated with spacetime measurements. This interdependency might illustrate the stability of these variables through iterative methods, offering potential insights into how spacetime could stabilize or reach fixed points when subjected to quantum fluctuations or scaling transformations.

The Lorentz factor can be obtained from a basic perspective. γ¯Ltz\bar{\gamma}_{Ltz} is introduced to act as the Lorentz factor. Therefore, the micro space length measurement contracted by scale γ¯Ltz\bar{\gamma}_{Ltz} gives rl1=σ1/γ¯Ltz=ς1τ/γ¯Ltzr_{l^{1}}=\sigma^{1}/\bar{\gamma}_{Ltz}=\varsigma^{1}\tau/\bar{\gamma}_{Ltz}, while the micro time inflated by γ¯Ltz\bar{\gamma}_{Ltz} gives rT=rl0/rc=rtγ¯Ltzr_{T}=r_{l^{0}}/r_{c}=r_{t}\bar{\gamma}_{Ltz} (i.e. rl0=rcrT=rcrtγ¯Ltz=τγ¯Ltzr_{l^{0}}=r_{c}r_{T}=r_{c}r_{t}\bar{\gamma}_{Ltz}=\tau\bar{\gamma}_{Ltz}). v1=ς1rc/γ¯Ltz2v^{1}=\varsigma^{1}r_{c}/\bar{\gamma}_{Ltz}^{2}. Since there is no contraction effect of the micro length along axis i>1i>1, rli>1=σi>1=ςi>1τr_{l}^{i>1}=\sigma^{i>1}=\varsigma^{i>1}\tau. Using the D-dimension local flat spacetime matric ηαβ\eta_{\alpha\beta}, we can get

καβ=±(γ¯Ltz20000[ς1]2/γ¯Ltz20000[ς2]20000[ςD1]2).\kappa_{\alpha\beta}=\pm\begin{pmatrix}\bar{\gamma}^{2}_{Ltz}&0&0&\cdots&0\\ 0&-[\varsigma^{1}]^{2}/\bar{\gamma}^{2}_{Ltz}&0&\cdots&0\\ 0&0&-[\varsigma^{2}]^{2}&\cdots&0\\ \vdots&\vdots&\vdots&\ddots&\vdots\\ 0&0&0&\cdots&-[\varsigma^{D-1}]^{2}\end{pmatrix}. (33)

From the constraint of Σα,βκαβ=1\Sigma_{\alpha,\beta}\kappa_{\alpha\beta}=1, we get the constrained relation connecting the dimension and components of spacetime,

1\displaystyle 1 =±{γ¯Ltz2[ς1]2/γ¯Ltz2k=2D1[ςk]2}.\displaystyle=\pm\{\bar{\gamma}^{2}_{Ltz}-[\varsigma^{1}]^{2}/\bar{\gamma}^{2}_{Ltz}-\sum_{k=2}^{D-1}[\varsigma^{k}]^{2}\}. (34)

We call καβ\kappa_{\alpha\beta} the spacetime structure coefficients. Eq. (34) can be deemed as an equation of γ¯Ltz2\bar{\gamma}^{2}_{Ltz} and its solutions are

γ¯Ltz2\displaystyle\bar{\gamma}^{2}_{Ltz} =12{(k=2D1[ςk]2±1)±4[ς1]2+(k=2D1[ςk]2±1)2}.\displaystyle=\frac{1}{2}\{(\sum_{k=2}^{D-1}[\varsigma^{k}]^{2}\pm 1)\pm\sqrt{4[\varsigma^{1}]^{2}+(\sum_{k=2}^{D-1}[\varsigma^{k}]^{2}\pm 1)^{2}}\}. (35)

The limit of light speed needs γ¯Ltz2>0\bar{\gamma}^{2}_{Ltz}>0 in Minkowski spacetime. The physical significance of this equation lies in its role in understanding how spacetime fluctuations at microscopic scales can be related to the relativistic effects of time dilation and length contraction. The Lorentz factor is a key component in the theory of relativity, used to describe how measurements of time and space differ for observers in different inertial frames. This equation demonstrates that the Lorentz factor depends on the scaling parameters ςk\varsigma^{k} which represent the fluctuations in spacetime geometry across different dimensions. The positive value of γ¯Ltz2\bar{\gamma}^{2}_{Ltz} is necessary to ensure the consistency of the model with the principles of relativity, particularly in preserving the limit on the speed of light. This relationship highlights how quantum fluctuations at the Planck scale can impact classical relativistic concepts, providing fundamental insight into the nature of spacetime.

Considering two limit situations for v1=0v^{1}=0 and rcr_{c}. If v1=0v^{1}=0, it corresponds to that ς1=0\varsigma^{1}=0 and γ¯Ltz2=k=2D1[ςk]2±1\bar{\gamma}_{Ltz}^{2}=\sum_{k=2}^{D-1}[\varsigma^{k}]^{2}\pm 1 or γ¯Ltz2=0\bar{\gamma}_{Ltz}^{2}=0. Consequently, σ1=0\sigma^{1}=0, signifying there is no spatial component in this direction. Additionally, we have k=2D1[σk]2=(γ¯Ltz21)τ2\sum_{k=2}^{D-1}[\sigma^{k}]^{2}=(\bar{\gamma}_{Ltz}^{2}\mp 1)\tau^{2} for the positive solution. If v1=rcv^{1}=r_{c}, needing ς1=γ¯Ltz2\varsigma^{1}=\bar{\gamma}_{Ltz}^{2} and following with σ1=γ¯Ltz2τ2\sigma^{1}=\bar{\gamma}_{Ltz}^{2}\tau^{2}, then k=2D1[ςk]2=1\sum_{k=2}^{D-1}[\varsigma^{k}]^{2}=\mp 1 and k=2D1[σk]2=τ2\sum_{k=2}^{D-1}[\sigma^{k}]^{2}=\mp\tau^{2}.

There is a generalization of Eq. (30). Based on Eq. (35), the generalized Lorentz inflation/contraction transformation becomes

{ϑ0=k=2D1[ςk]2±11ϑ1ϑ0;ϑ1=[ς1]2k=2D1[ςk]2±1(1ϑ1ϑ0),\begin{cases}&\vartheta^{0}=\frac{\sum_{k=2}^{D-1}[\varsigma^{k}]^{2}\pm 1}{1-\frac{\vartheta^{1}}{\vartheta^{0}}};\\ &\vartheta^{1}=\frac{[\varsigma^{1}]^{2}}{\sum_{k=2}^{D-1}[\varsigma^{k}]^{2}\pm 1}(1-\frac{\vartheta^{1}}{\vartheta^{0}}),\end{cases} (36)

where ϑ0ϑ1=[ς1]2\vartheta^{0}\vartheta^{1}=[\varsigma^{1}]^{2}.

Comparing Eq. (35) to Eq. (32), when k=2D1[ςk]2\sum_{k=2}^{D-1}[\varsigma^{k}]^{2} equals 0 for time-like metric while 2 for space-like metric, we get positive γ¯Ltz=γLtz\bar{\gamma}_{Ltz}=\gamma_{Ltz}. And then we have expressions

[ς1]2=rc2[v1]2(rc2[v1]2)2=[ϑ0]2[ϑ1]2([ϑ0]2[ϑ1]2)2;\displaystyle[\varsigma^{1}]^{2}=\frac{r_{c}^{2}[v^{1}]^{2}}{(r_{c}^{2}-[v^{1}]^{2})^{2}}=\frac{[\vartheta^{0}]^{2}[\vartheta^{1}]^{2}}{([\vartheta^{0}]^{2}-[\vartheta^{1}]^{2})^{2}}; (37)
γLtz2[ς1]2γLtz2=1;\displaystyle\gamma_{Ltz}^{2}-[\varsigma^{1}]^{2}\gamma_{Ltz}^{-2}=1; (38)
v1=rl1rT=ς1γLtz2rc=rv1γLtz=ς1rc12(1+1+4[ς1]2);\displaystyle v^{1}=\frac{r_{l^{1}}}{r_{T}}=\frac{\varsigma^{1}}{\gamma_{Ltz}^{2}}r_{c}=\frac{r_{v^{1}}}{\gamma_{Ltz}}=\frac{\varsigma^{1}r_{c}}{\frac{1}{2}(1+\sqrt{1+4[\varsigma^{1}]^{2}})}; (39)
vi>1=rli>1rT=ςi>1γLtzrc=rvi>1γLtz;\displaystyle v^{i>1}=\frac{r_{l}^{i>1}}{r_{T}}=\frac{\varsigma^{i>1}}{\gamma_{Ltz}}r_{c}=\frac{r_{v^{i>1}}}{\gamma_{Ltz}}; (40)
v0=rl0rT=rc.\displaystyle v^{0}=\frac{r_{l^{0}}}{r_{T}}=r_{c}. (41)

The speed vi>2v^{i>2} can be defined as the speed of fluctuation in micro-length measurements (σi>2\sigma^{i>2}) associated with the fluctuation on i=1i=1 axis with a speed of v1v^{1} (0v1rc0\leq v^{1}\leq r_{c}, TABLE 1 illustrates the relationships in the limiting situation for v1=0v^{1}=0 and rcr_{c}). This association is expressed via vαv^{\alpha} being constrained by the relationship of

rc2γLtz2=±([v0]2k=1D1[vk]2),\displaystyle\frac{r_{c}^{2}}{\gamma_{Ltz}^{2}}=\pm([v^{0}]^{2}-\sum_{k=1}^{D-1}[v^{k}]^{2}), (42)

where k=2D1[vk]2=2rc2γLtz2=2(rc2[v1]2)\sum_{k=2}^{D-1}[v^{k}]^{2}=\frac{2r_{c}^{2}}{\gamma_{Ltz}^{2}}=2(r_{c}^{2}-[v^{1}]^{2}) for space-like metric and 0 for time-like metric.

Table 1: The relationships in the limit-situation
v1=0v^{1}=0 γLtz2=1\gamma_{Ltz}^{2}=1 ϑ1=0\vartheta^{1}=0 ς1=0\varsigma^{1}=0 ϑ0=1\vartheta^{0}=1
v1=rcv^{1}=r_{c} γLtz2=\gamma_{Ltz}^{2}=\infty ϑ1=ϑ0\vartheta^{1}=\vartheta^{0} ς1=\varsigma^{1}=\infty ϑ0=\vartheta^{0}=\infty

V Micro measurement in spacetime with Schwarzschild Metric

The Schwarzschild metric describes the spacetime around a non-rotating, spherically symmetric black hole. If considering the black hole with Schwarzschild Metric bibitem14 , the space-like line element has the form of

dλ2=(1rsr)c2dt2+(1rsr)1dr2+r2dΩ2\displaystyle d\lambda^{2}=-(1-\frac{r_{s}}{r})c^{2}dt^{2}+(1-\frac{r_{s}}{r})^{-1}dr^{2}+r^{2}d\Omega^{2} (43)

in Schwarzschild coordinates, where dΩ2=dθ2+sin2(θ)dϕ2d\Omega^{2}=d\theta^{2}+sin^{2}(\theta)d\phi^{2}. And rs=2GMc2r_{s}=\frac{2GM}{c^{2}} is the Schwarzschild radius at where the event horizon is. GG is the gravitational constant, MM is the object mass, and cc is the speed of light. In the presence of gravitational fields, measurements of space and time are affected differently compared to special relativity. Specifically, gravitational fields can cause contraction effects in spatial measurements and dilation effects in time measurements. These effects arise due to the curvature of spacetime in general relativity. In regions with strong gravity, time appears to slow down (gravitational time dilation), while space can be warped, affecting perceived distances. These phenomena differ from the effects predicted by special relativity, which deals with time dilation and length contraction due to relative motion. However, in the absence of gravitational fields or in regions with weak gravity, the predictions of general relativity converge to those of special relativity. In such scenarios, spacetime is essentially flat, and the familiar Lorentz transformations apply, with the Lorentz factor γ¯Ltz\bar{\gamma}_{Ltz} describing time dilation and length contraction.

Define a new factor γg\gamma_{g} to replace γ¯Ltz\bar{\gamma}_{Ltz} to act as the Lorentz factor in the spacetime of Schwarzschild Metric to measure the micro length contraction and micro time inflation effect. It can be seen as a correction factor with respect to γ¯Ltz\bar{\gamma}_{Ltz} when measuring in a gravitational field. Using the constraint of Σα,βκαβ=1\Sigma_{\alpha,\beta}\kappa_{\alpha\beta}=1, we get

γg2=(1rsr)1γ¯Ltz2.\displaystyle\gamma_{g}^{2}=(1-\frac{r_{s}}{r})^{-1}\bar{\gamma}^{2}_{Ltz}. (44)

When M=0M=0 or rr\rightarrow\infty, γg2=γ¯Ltz2\gamma^{2}_{g}=\bar{\gamma}^{2}_{Ltz}. When r=rsr=r_{s}, γg2=\gamma^{2}_{g}=\infty. When r=0r=0, γg2=0\gamma^{2}_{g}=0. γg2\gamma^{2}_{g} is remaining positive when γ¯Ltz2<0\bar{\gamma}^{2}_{Ltz}<0 at r<rsr<r_{s} and γ¯Ltz2>0\bar{\gamma}^{2}_{Ltz}>0 at r>rsr>r_{s}. It can be seen that γg\gamma_{g} describes a dual effect of gravitational field in the general relativity frame and local motion in the special relativity frame. From this generalized Lorentz factor γg\gamma_{g} in Schwarzschild Metric, we can still keep Eq. (34) remaining. Consequently, the physical laws satisfy the Lorentz transformation when the physical variables are defined to be scaled by γg\gamma_{g}.

There is also a generalization of Lorentz inflation/contraction transformation in Schwarzschild Metric. Namely,

{ϑ0=(1rsr)1k=2D1[ςk]2±11ϑ1ϑ0;ϑ1=(1rsr)1[ς1]2k=2D1[ςk]2±1(1ϑ1ϑ0),\begin{cases}&\vartheta^{0}=(1-\frac{r_{s}}{r})^{-1}\frac{\sum_{k=2}^{D-1}[\varsigma^{k}]^{2}\pm 1}{1-\frac{\vartheta^{1}}{\vartheta^{0}}};\\ &\vartheta^{1}=(1-\frac{r_{s}}{r})^{-1}\frac{[\varsigma^{1}]^{2}}{\sum_{k=2}^{D-1}[\varsigma^{k}]^{2}\pm 1}(1-\frac{\vartheta^{1}}{\vartheta^{0}}),\end{cases} (45)

where ϑ0ϑ1=[ς1]2(1rsr)2\vartheta^{0}\vartheta^{1}=[\varsigma^{1}]^{2}(1-\frac{r_{s}}{r})^{-2}.

The mass of a particle moving along rr scaled by γg\gamma_{g} is expressed by

mg2=γg2m02=(1rsr)1γ¯Ltz2m02=γ¯Ltz2mg02,\displaystyle m^{2}_{g}=\gamma_{g}^{2}m^{2}_{0}=(1-\frac{r_{s}}{r})^{-1}\bar{\gamma}^{2}_{Ltz}m^{2}_{0}=\bar{\gamma}^{2}_{Ltz}m^{2}_{g0}, (46)

where mg02=(1rsr)1m02m^{2}_{g0}=(1-\frac{r_{s}}{r})^{-1}m^{2}_{0} is introduced as the measured mass of the particle at instantaneous rest in a gravitational field with Schwarzschild metric and m0m_{0} is the mass of the particle at rest in a flat metric. When rr\rightarrow\infty or M=0M=0, mg02=m02m^{2}_{g0}=m^{2}_{0}. When r0r\rightarrow 0, mg02=0m^{2}_{g0}=0. Therefore, the energy-momentum relationship measured locally in the gravitational field with the Schwarzschild Metric becomes

Eg2=pg2c2+mg02c4,\displaystyle E^{2}_{g}=p^{2}_{g}c^{2}+m^{2}_{g0}c^{4}, (47)

where Eg2=γ¯Ltz2(1rsr)1m02c4=γ¯Ltz2mg02c4E^{2}_{g}=\bar{\gamma}^{2}_{Ltz}(1-\frac{r_{s}}{r})^{-1}m^{2}_{0}c^{4}=\bar{\gamma}^{2}_{Ltz}m^{2}_{g0}c^{4}. And pg,12=γ¯Ltz2(1rsr)1m02vg12=γ¯Ltz2mg02vg,12p^{2}_{g,1}=\bar{\gamma}^{2}_{Ltz}(1-\frac{r_{s}}{r})^{-1}m^{2}_{0}v^{2}_{g1}=\bar{\gamma}^{2}_{Ltz}m^{2}_{g0}v^{2}_{g,1} with vg,1=ς1rcγg2v_{g,1}=\frac{\varsigma^{1}r_{c}}{\gamma_{g}^{2}} and pg,k>12=γ¯Ltz2mg02vg,k>12p^{2}_{g,k>1}=\bar{\gamma}^{2}_{Ltz}m^{2}_{g0}v^{2}_{g,k>1} with vg,k>1=ςk>1rcγgv_{g,k>1}=\frac{\varsigma^{k>1}r_{c}}{\gamma_{g}}. Thus, pg2=k=1D1pg,k2p^{2}_{g}=\sum_{k=1}^{D-1}p^{2}_{g,k}. This energy-momentum relationship scaled by (1rsr)(1-\frac{r_{s}}{r}) on both sides can be back to the one in Minkowski spacetime. When rr\rightarrow\infty or M=0M=0, the former is also back to the latter. When r>>rsr>>r_{s}, we get

Eg2=pg2c2+m02c4[1+rsr+(rsr)2+O(3)],\displaystyle E^{2}_{g}=p^{2}_{g}c^{2}+m^{2}_{0}c^{4}[1+\frac{r_{s}}{r}+(\frac{r_{s}}{r})^{2}+O(3)], (48)

VI Scaling Geodesic Equations and Einstein Field Equations

Geodesic equations bibitem8 ; bibitem9 ; bibitem10 ; Tsamparlis ; Hackmann are fundamental in the study of general relativity and differential geometry. They describe the path that an object follows under the influence of gravity alone, without any other forces acting on it. They are crucial for understanding the motion of objects in a gravitational field, serving as the foundation for analyzing how gravity shapes the trajectories of particles and light. They provide insights into both macroscopic phenomena, like the orbits of planets, and microscopic effects, such as the influence of gravity on quantum particles. As such, geodesics are integral to bridging the gap between classical and quantum descriptions of gravity.

The geodesic equations can be written in scaling form on a micro-scale via operators’ transformations. Firstly, by using Eq. (8), the Christoffel symbols can be represented in the form of

𝚪βγα\displaystyle\mathbf{\Gamma}^{\alpha}_{\beta\gamma} =12gαμ1dx0(a^βgγμXβ+a^γgβμXγ+a^μgβγXμ)\displaystyle=\frac{1}{2}g^{\alpha\mu}\frac{1}{dx_{0}}(\hat{a}_{\beta}\frac{\partial g_{\gamma\mu}}{\partial X^{\beta}}+\hat{a}_{\gamma}\frac{\partial g_{\beta\mu}}{\partial X^{\gamma}}+\hat{a}_{\mu}\frac{\partial g_{\beta\gamma}}{\partial X^{\mu}}) (49)
=1dx0Γβγα\displaystyle=\frac{1}{dx_{0}}\Gamma^{\alpha}_{\beta\gamma}

with Einstein notation, where Γβγα\Gamma^{\alpha}_{\beta\gamma} are defined as dimensionless scaling Christoffel symbols. Combining the Eq. (3) and Eq. (4), the scaling geodesic equations are obtained by

(L¯αLα)+ΓβγαLαLβ=0\displaystyle(\bar{L}^{\alpha}-L^{\alpha})+\Gamma^{\alpha}_{\beta\gamma}L^{\alpha}L^{\beta}=0 (50)

with Einstein notation. The equation demonstrates how local geodesic paths (which describe the shortest path between points in spacetime) evolve with scaling functions, offering insights into the complex structure of spacetime at microscopic scales.

In the framework of general relativity, gravity is conceptualized not as a force but as an outcome of the curvature of spacetime, with the stress-energy tensor serving as the source of this curvature. Within the geometric interpretation of gravity, geodesics are indicative of the curved geometry inherent in spacetime. All length-minimizing curves are geodesics, and all geodesics are length-minimizing, at least locally bibitem15 . The local geodesic equations can be viewed as a constraint on microscopic spacetime measurements at a local level. When representing the measurement of spacetime microelements through scaling functions, the geodesic equations represented by scales elucidate the restrictions on nontrivial fluctuations of scales.

The scaled Einstein Field Equations represented by scales XαX^{\alpha} can be obtained in the same way. Which characterizes how the scales of micro geometric spacetime measurements are influenced by stress-energy tensor.

By considering a transformation of a linear mapping between coordinate xαx^{\alpha} and scale X¯α\bar{X}^{\alpha}. The latter are new scales obtained by rescaling ζα\zeta^{\alpha} on XαX^{\alpha}. ζα\zeta^{\alpha} are the rescaling factors on differential operators, establishing a connection between coordinate xαx^{\alpha} and scale X¯α\bar{X}^{\alpha} and making the micro measurements being carried out in a linear way, i.e.,

dxα=dX¯αdx0α.\displaystyle dx^{\alpha}=d\bar{X}^{\alpha}dx^{\alpha}_{0}. (51)

where X¯α\bar{X}^{\alpha} denotes a scaled version of coordinate xαx^{\alpha} in fact of our conventional understanding of the definition of measurement based on the unit system. We call these mapping conditions on rescaling factors ζα\zeta^{\alpha}. This will bring the spacetime structure measured by nonlinear kernel Lα(Xα)L^{\alpha}(X^{\alpha}) back to the linear kernel X¯α\bar{X}^{\alpha}. The spacetime fluctuation determined by the latter can equivalently represent the erratic point (xαx^{\alpha}) in spacetime. This greatly simplifies the complexity of handling the problems at the micro-scale and facilitates the extraction of intrinsic properties of the dynamic systems involved.

It is essential to emphasize that xαx^{\alpha} represents the position of a point in the coordinate frame on spacetime. However, X¯α\bar{X}^{\alpha} and XαX^{\alpha} denote the measuring scales of the micro-interval of the fluctuating spacetime near a point along the α\alpha-axis direction. Through a linear mapping between xαx^{\alpha} and X¯α\bar{X}^{\alpha}, the latter characterizes linear scaling measurements in the spacetime defined by the former. On the other hand, XαX^{\alpha} describes a spacetime with a structure of nonlinear measurement.

Comparing Eq. (8) and Eq. (13), the mapping conditions

xα=1dx0αX¯α\displaystyle\frac{\partial}{\partial x^{\alpha}}=\frac{1}{dx_{0}^{\alpha}}\frac{\partial}{\partial\bar{X}^{\alpha}} (52)

could be satisfied, resulting in a transformation making the microelement measurements from a nonlinear mode into a linear one. These linear conditions can be equivalently expressed as 1ζα=a^α\frac{1}{\zeta^{\alpha}}=\hat{a}_{\alpha} and then we get equations of

dLαdXα=ζα(L¯αLα1).\displaystyle\frac{dL^{\alpha}}{dX^{\alpha}}=\zeta^{\alpha}(\frac{\bar{L}^{\alpha}}{L^{\alpha}}-1). (53)

When dLαdXα=0\frac{dL^{\alpha}}{dX^{\alpha}}=0, then corresponds to ζα=1\zeta^{\alpha}=1, the spacetime nature is back to the classical non-fluctuation (stable) structure.

These equations can be regarded as nonlinear feedback equations, where the differences in the state of LαL^{\alpha} at different scaling scales drive the dynamic evolution of the system, leading to complex behaviors such as fluctuations, chaos, or bifurcations, depending on the system parameters. Rescaling factor ζα\zeta^{\alpha} modulates the system’s sensitivity, affecting how the output L¯α\bar{L}^{\alpha} responds to inputs at the original scale XαX^{\alpha}, affecting the stability and dynamic behavior of the system. Similar structures of Eq. (53) can be found in delay differential equations Richard , chaotic systemsLathrop , and proportional feedback modelsAstrom . These types of equations are commonly used to describe adaptive systems, nonlinear control systems, and dynamic systems with complex feedback structures. The form of the nonlinear feedback equations suggests the existence of adaptive and dynamic behaviors in spacetime geometry, prompting us to explore how more complex feedback structures manifest the evolution of spacetime at a micro-scale.

When Lα=[Xα]qαL^{\alpha}=[X^{\alpha}]^{q^{\alpha}} with qαq^{\alpha} being exponents that characterize a self-similarity and scaling behavior of spacetime fluctuations along the α\alpha-axis. In this situation, Eq. (53) becomes

[ζα]qα+1ζαqα[Xα]qα1=0.\displaystyle[\zeta^{\alpha}]^{q^{\alpha}+1}-\zeta^{\alpha}-q^{\alpha}[X^{\alpha}]^{q^{\alpha}-1}=0. (54)

When qα=1q^{\alpha}=1, we get ζα=φ=1±521.618034(0.618034)\zeta^{\alpha}=\varphi=\frac{1\pm\sqrt{5}}{2}\approx 1.618034(-0.618034), it is the golden ratio. The nonlinear form of this equation highlights the complexity of scaling effects, emphasizing the intricate relationship between scaling factors and exponents.

The subsequent instances are the scaled geodesic equations and scaled Einstein field equations within the linear measurement spacetime, as well as the constraint equations derived from their linear mapping conditions.

With the linear mapping conditions of

{xα=1dx0αX¯α,dxαdλ=dX¯αdX¯,d2xαdλ2=d2X¯αdX¯21dλ0,\begin{cases}&\frac{\partial}{\partial x^{\alpha}}=\frac{1}{dx_{0}^{\alpha}}\frac{\partial}{\partial\bar{X}^{\alpha}},\\ &\frac{dx^{\alpha}}{d\lambda}=\frac{d\bar{X}^{\alpha}}{d\bar{X}},\\ &\frac{d^{2}x^{\alpha}}{d\lambda^{2}}=\frac{d^{2}\bar{X}^{\alpha}}{d\bar{X}^{2}}\frac{1}{d\lambda_{0}},\end{cases} (55)

the geodesic equations can be derived in the equivalent scaling form, e.i.

d2X¯αdX¯2+Γ¯βγαdX¯βdX¯dX¯γdX¯=0\displaystyle\frac{d^{2}\bar{X}^{\alpha}}{d\bar{X}^{2}}+\bar{\Gamma}^{\alpha}_{\beta\gamma}\frac{d\bar{X}^{\beta}}{d\bar{X}}\frac{d\bar{X}^{\gamma}}{d\bar{X}}=0 (56)

with Einstein notation, where scaling Christoffel symbols are

Γ¯βγα=12g¯αμ(g¯γμX¯β+g¯βμX¯γ+g¯βγX¯μ)\displaystyle\bar{\Gamma}^{\alpha}_{\beta\gamma}=\frac{1}{2}\bar{g}^{\alpha\mu}(\frac{\partial\bar{g}_{\gamma\mu}}{\partial\bar{X}^{\beta}}+\frac{\partial\bar{g}_{\beta\mu}}{\partial\bar{X}^{\gamma}}+\frac{\partial\bar{g}_{\beta\gamma}}{\partial\bar{X}^{\mu}}) (57)

with

g¯αβ(X¯μ)=gαβ(xμX¯μ).\displaystyle\bar{g}_{\alpha\beta}(\bar{X}^{\mu})=g_{\alpha\beta}(x^{\mu}\rightarrow\bar{X}^{\mu}). (58)

In Eq. (55), dX¯αdX¯=dX¯αdXαdXαdXdXdX¯=(ζα+XαdζαdXα)dXαdX1χ\frac{d\bar{X}^{\alpha}}{d\bar{X}}=\frac{d\bar{X}^{\alpha}}{dX^{\alpha}}\frac{dX^{\alpha}}{dX}\frac{dX}{d\bar{X}}=(\zeta^{\alpha}+X^{\alpha}\frac{d\zeta^{\alpha}}{dX^{\alpha}})\frac{dX^{\alpha}}{dX}\frac{1}{\chi}. Utilizing the definitions of rlαr_{l}^{\alpha} and rlr_{l} and the expression of drlαdrl\frac{dr_{l^{\alpha}}}{dr_{l}}, we get dXαdX=L¯αLατ¯τdτ/dXdLα/dXα\frac{dX^{\alpha}}{dX}=\frac{\bar{L}^{\alpha}-L^{\alpha}}{\bar{\tau}-\tau}\frac{d\tau/dX}{dL^{\alpha}/dX^{\alpha}}. Thus, the linearized requirements of dxαdλ=dX¯αdX¯\frac{dx^{\alpha}}{d\lambda}=\frac{d\bar{X}^{\alpha}}{d\bar{X}} and 1ζα=a^α\frac{1}{\zeta^{\alpha}}=\hat{a}_{\alpha} result in

1+XαζαdζαdXα=χa^,\displaystyle 1+\frac{X^{\alpha}}{\zeta^{\alpha}}\frac{d\zeta^{\alpha}}{dX^{\alpha}}=\chi\hat{a}, (59)

The requirement of d2xαdλ2=d2X¯αdX¯21dλ0=1dλ0ddX(dX¯αdX¯)dXdX¯\frac{d^{2}x^{\alpha}}{d\lambda^{2}}=\frac{d^{2}\bar{X}^{\alpha}}{d\bar{X}^{2}}\frac{1}{d\lambda_{0}}=\frac{1}{d\lambda_{0}}\frac{d}{dX}(\frac{d\bar{X}^{\alpha}}{d\bar{X}})\frac{dX}{d\bar{X}} further leads to

dτdX=(1a^χ)(L¯αLα1),\displaystyle\frac{d\tau}{dX}=(\frac{1}{\hat{a}}-\chi)(\frac{\bar{L}^{\alpha}}{L^{\alpha}}-1), (60)

If linear mapping condition is used for proper measurement, a^=1χ\hat{a}=\frac{1}{\chi}, resulting ζα\zeta^{\alpha} and τ\tau are constants. In addition, from 1ζα=a^α\frac{1}{\zeta^{\alpha}}=\hat{a}_{\alpha}, we can obtain Eq. (53), with ζα\zeta^{\alpha} independent on XαX^{\alpha} once a^=1χ\hat{a}=\frac{1}{\chi}.

The geodesic equations formulated in terms of coordinates xαx^{\alpha} describe a continuous and stable spacetime. In contrast, the scaling geodesic equations Eq. (50) based on scales XαX^{\alpha} characterize a fluctuating spacetime at the microscopic level. Furthermore, the scaling geodesic equations Eq. (56) defined with scales X¯α\bar{X}^{\alpha} illustrate a fluctuating spacetime at the micro-scale with the linear mapping conditions.

With the linear mapping conditions of

{xα=1dx0αX¯α,2xαxβ=1dx0αdx0β2X¯αX¯β,\begin{cases}&\frac{\partial}{\partial x^{\alpha}}=\frac{1}{dx_{0}^{\alpha}}\frac{\partial}{\partial\bar{X}^{\alpha}},\\ &\frac{\partial^{2}}{\partial x^{\alpha}\partial x^{\beta}}=\frac{1}{dx_{0}^{\alpha}dx_{0}^{\beta}}\frac{\partial^{2}}{\partial\bar{X}^{\alpha}\partial\bar{X}^{\beta}},\end{cases} (61)

using 1ζβ=a^β\frac{1}{\zeta^{\beta}}=\hat{a}_{\beta} and 1[ζα]2dζαdXα=b^α\frac{1}{[\zeta^{\alpha}]^{2}}\frac{d\zeta^{\alpha}}{dX^{\alpha}}=\hat{b}_{\alpha}, under the transformation of ζα\zeta^{\alpha} for differential operators between xαx^{\alpha} and X¯α\bar{X}^{\alpha}, we can similarly get the scaling Einstein field equations in the absence of any matter,

G¯μν=R¯μν12g¯μνR¯=0,\displaystyle\bar{G}_{\mu\nu}=\bar{R}_{\mu\nu}-\frac{1}{2}\bar{g}_{\mu\nu}\bar{R}=0, (62)

and the scaling vacuum Einstein equations in the presence of a cosmological constant Λ¯\bar{\Lambda},

G¯μν=R¯μν12g¯μνR¯+Λ¯g¯μν=0,\displaystyle\bar{G}_{\mu\nu}=\bar{R}_{\mu\nu}-\frac{1}{2}\bar{g}_{\mu\nu}\bar{R}+\bar{\Lambda}\bar{g}_{\mu\nu}=0, (63)

where scaling Riemann curvature tensor

R¯σμνρ=X¯μΓ¯νσρX¯νΓ¯μσρ+Γ¯μλρΓ¯νσλ+Γ¯νλρΓ¯μσλ\displaystyle\bar{R}^{\rho}_{\sigma\mu\nu}=\frac{\partial}{\partial\bar{X}^{\mu}}\bar{\Gamma}^{\rho}_{\nu\sigma}-\frac{\partial}{\partial\bar{X}^{\nu}}\bar{\Gamma}^{\rho}_{\mu\sigma}+\bar{\Gamma}^{\rho}_{\mu\lambda}\bar{\Gamma}^{\lambda}_{\nu\sigma}+\bar{\Gamma}^{\rho}_{\nu\lambda}\bar{\Gamma}^{\lambda}_{\mu\sigma} (64)

and R¯=g¯μνR¯μν\bar{R}=\bar{g}^{\mu\nu}\bar{R}_{\mu\nu}, with Einstein notation. Therefore, we conclude that the scaling Einstein field equations in the absence of any matter and in the presence of a cosmological constant Λ¯\bar{\Lambda} require ζα\zeta^{\alpha} to satisfy

{dLαdXα=ζα(L¯αLα1);dζαdXα=[ζα]2b^α.\begin{cases}&\frac{dL^{\alpha}}{dX^{\alpha}}=\zeta^{\alpha}(\frac{\bar{L}^{\alpha}}{L^{\alpha}}-1);\\ &\frac{d\zeta^{\alpha}}{dX^{\alpha}}=[\zeta^{\alpha}]^{2}\hat{b}_{\alpha}.\end{cases} (65)

For the Einstein field equations with some specific stress-energy tensor, more conditions embedded in the stress-energy tensor need to be considered in the linear mapping conditions.

VII The golden ratio at the micro-scale

The micro distance measurement with Lα=XαL^{\alpha}=X^{\alpha} corresponds to a linear mode, expressed as dxα=Xαdx0αdx^{\alpha}=X^{\alpha}dx^{\alpha}_{0}. By adding the linear mapping dxα=dX¯αdx0αdx^{\alpha}=d\bar{X}^{\alpha}dx^{\alpha}_{0}, we obtain the following equations:

{xα=Xαdx0α+x0α;xα=X¯αdx0α+x¯0α,\begin{cases}&x^{\alpha}=X^{\alpha}dx^{\alpha}_{0}+x^{\alpha}_{0};\\ &x^{\alpha}=\bar{X}^{\alpha}dx^{\alpha}_{0}+\bar{x}^{\alpha}_{0},\end{cases} (66)

where dxα=xαx0αdx^{\alpha}=x^{\alpha}-x^{\alpha}_{0} and xαx^{\alpha} are the position coordinates relative to reference position coordinates x0αx^{\alpha}_{0} or x¯0α\bar{x}^{\alpha}_{0}, By letting dx0α=x0αx¯0αdx^{\alpha}_{0}=x^{\alpha}_{0}-\bar{x}^{\alpha}_{0}, we get

[(X¯αXα)1]dx0α=[(φ1)Xα1]dx0α=0,\displaystyle[(\bar{X}^{\alpha}-X^{\alpha})-1]dx^{\alpha}_{0}=[(\varphi-1)X^{\alpha}-1]dx^{\alpha}_{0}=0, (67)

resulting in dxαdx0α=Xα=1φ1=φ\frac{dx^{\alpha}}{dx^{\alpha}_{0}}=X^{\alpha}=\frac{1}{\varphi-1}=\varphi. Thus X¯α=ζαXα=φXα=φ2\bar{X}^{\alpha}=\zeta^{\alpha}X^{\alpha}=\varphi X^{\alpha}=\varphi^{2}. Introduce dx¯α=xαx¯0αd\bar{x}^{\alpha}=x^{\alpha}-\bar{x}^{\alpha}_{0}, we get dx¯αdxα=X¯αXα=φ\frac{d\bar{x}^{\alpha}}{dx^{\alpha}}=\frac{\bar{X}^{\alpha}}{X^{\alpha}}=\varphi. This is illustrated in FIG. 1, where φ\varphi is the golden ratio, indicating that within the spacetime of linear scale measurement, the golden ratio naturally arises at the microscopic scale.

To illustrate the linear measurement of micro distance, consider selecting two points x¯0\bar{x}_{0} and x0x_{0} that are sufficiently close in the coordinate space, the interval dx0=x0x¯0dx_{0}=x_{0}-\bar{x}_{0} between these two points is defined as the reference length. When a third point is selected, two microscopic intervals, dx¯d\bar{x} and dxdx can be defined. The ratio of these intervals is the golden ratio. We propose that micro-distance measurements in a defined 1-dimensional coordinate system can occur in two distinct scenarios: one where the third point is selected outside the reference interval and another where it is chosen within the interval. These scenarios correspond to the positive φR=1+52\varphi_{R}=\frac{1+\sqrt{5}}{2} and negative φL=152\varphi_{L}=\frac{1-\sqrt{5}}{2} solutions of the equation Eq. (53) with Lα=XαL^{\alpha}=X^{\alpha}, as shown in FIG. 1 (a) and (b) respectively. Here, the subscript ”R” indicates that xx is to the right of the reference point x0x_{0}, while ”L” is to the left.

Refer to caption
Figure 1: Golden section at the microscopic scale in the spacetime of linear scale measurement.

In this framework, for external measurements, dx0αdx^{\alpha}_{0} functions as the minimum reference length, limiting the measurement of micro-lengths smaller than dx0αdx^{\alpha}_{0}. Conversely, for internal measurements, dx0αdx^{\alpha}_{0} functions as the maximum reference length, constraining the measurement of micro-lengths larger than dx0αdx^{\alpha}_{0}. This insight provides a clue for understanding the existence of the Planck length, which manifests as a lower limit for external measurements and an upper limit for internal measurements in the depiction of microscopic phenomena.

In general, arbitrary Lα=Lα(Xα)L^{\alpha}=L^{\alpha}(X^{\alpha}) satisfying the linear mapping conditions are appropriate to the above analysis, making

X¯α=ζαXα=1+Lα.\displaystyle\bar{X}^{\alpha}=\zeta^{\alpha}X^{\alpha}=1+L^{\alpha}. (68)

If Lα>0L^{\alpha}>0 for the right measuring, while Lα<0L^{\alpha}<0 for the left measuring. Therefore, the metric tensor (Eq. 58) becomes g¯αβ(X¯σ)=gαβ[xσx0σ+(X¯σ1)dx0σ]\bar{g}_{\alpha\beta}(\bar{X}^{\sigma})=g_{\alpha\beta}[x^{\sigma}\rightarrow x^{\sigma}_{0}+(\bar{X}^{\sigma}-1)dx^{\sigma}_{0}]. The case of X¯α>1\bar{X}^{\alpha}>1 (external measurements) indicates that the UV problem is avoidable for the evolution of the equations (Eq. 56, 62, 63) in spacetime described by X¯σ\bar{X}^{\sigma}.

Once Eq. (53) is multiplied by XαX^{\alpha}, we get renormalization group equations Stueckelberg for micro measurements of the micro spacetime fluctuations, namely

XαdLαdXα=β(Lα)=(1+Lα)(L¯αLα1),\displaystyle X^{\alpha}\frac{dL^{\alpha}}{dX^{\alpha}}=\beta(L^{\alpha})=(1+L^{\alpha})(\frac{\bar{L}^{\alpha}}{L^{\alpha}}-1), (69)

where β(Lα)\beta(L^{\alpha}) is the beta function and β(Lα)=0\beta(L^{\alpha})=0 defines the fixed points of the measurements. At the fixed points L¯α=Lα\bar{L}^{\alpha}=L^{\alpha}, the beta function β(Lα)\beta(L^{\alpha}) vanishes, indicating that the fluctuations have reached equilibrium and a symmetric state, scale invariance. Deviations from this point drive the scaling behavior of the fluctuations, causing it to adjust towards the fixed point. The case Lα=1L^{\alpha}=-1 represents a potential unique solution. Based on stability analysis, Lα=1L^{\alpha}=-1 are saddle points (dβdLα\frac{d\beta}{dL^{\alpha}}=0) while L¯α=Lα\bar{L}^{\alpha}=L^{\alpha} are stable points (dβdLα<0\frac{d\beta}{dL^{\alpha}}<0) if Lα0L^{\alpha}\geq 0 or <1<-1. If 1<Lα<0-1<L^{\alpha}<0, L¯α=Lα\bar{L}^{\alpha}=L^{\alpha} are unstable points. Consequently, the measurements are unstable within the region between x¯0α\bar{x}^{\alpha}_{0} and x0αx^{\alpha}_{0} but stable outside. Here, L¯α=Lα(ζαXα)=Lα(Xα)\bar{L}^{\alpha}=L^{\alpha}(\zeta^{\alpha}X^{\alpha})=L^{\alpha}(X^{\alpha}) means scale invariant.

When Lσ=1L^{\sigma}=1, it follows X¯σ=2\bar{X}^{\sigma}=2, resulting in xσ=x0σ+dx0σx^{\sigma}=x^{\sigma}_{0}+dx^{\sigma}_{0}. When Lσ=1L^{\sigma}=-1, X¯σ=0\bar{X}^{\sigma}=0, resulting in xσ=x0σdx0σ=x¯0σx^{\sigma}=x^{\sigma}_{0}-dx^{\sigma}_{0}=\bar{x}^{\sigma}_{0}. In this case, spacetime measurements are performed in uniform and equidistant micro-intervals without fluctuations, and the physics is defined on equidistantly discrete points.

When considering a not-allowed situation in the current framework where Lα0L^{\alpha}\rightarrow 0, we have xσ=x0σx^{\sigma}=x^{\sigma}_{0}, which leads to gαβg_{\alpha\beta}\rightarrow\infty if Eq. (25) consistently used, indicating divergence, this represents a scenario of a singularity without fluctuation. Consequently, classical continuous spacetime allows for the definition of arbitrarily small intervals (i.e., dxα=0dx^{\alpha}=0), indicating that the definition of continuous spacetime results in singularities of spacetime measurements appearing everywhere when making arbitrarily infinitesimal measurements.

The emergence of the golden ratio in linear micro measurements suggests that spacetime possesses an intrinsic order characterized by mapping constraints. Physics is defined at two fixed points, φR\varphi_{R} and φL\varphi_{L}, with bilateral asymmetry around x0σx^{\sigma}_{0}. Generally, the mapping constraints can influence spacetime patterns or structures, making physics defined on discrete points (might be multiple) once the forms of Lα(Xα)L^{\alpha}(X^{\alpha}) measurements are given, since there are equations for solving XαX^{\alpha} based on Eq. 53 and Eq. 68. There is a condition to determine the forms of Lα(Xα)=ζαXα1L^{\alpha}(X^{\alpha})=\zeta^{\alpha}X^{\alpha}-1: ζα\zeta^{\alpha} are constants via analyzing Eq. (59) if considering the linear mapping constraint of a^=1χ\hat{a}=\frac{1}{\chi} for proper length measurement, resulting in Xα=12ζα[ζα]2X^{\alpha}=\frac{1}{2\zeta^{\alpha}-[\zeta^{\alpha}]^{2}}. When solving the forms of Lα(Xα)L^{\alpha}(X^{\alpha}), coupling with ζα(Xα)\zeta^{\alpha}(X^{\alpha}), using equations Eq. (53) and Eq. (68) without considering the constraint χa^=1\chi\hat{a}=1, it leads to the conclusion that micro measurements are performed through fluctuating functions Lα(Xα)L^{\alpha}(X^{\alpha}), indicating that physics is defined on a fluctuating spacetime.

What can be argued is that dx0αdx^{\alpha}_{0} as a critical reference length for both external and internal measurements plays a key role in addressing the problem of UV divergence bibitem1 ; bibitem2 ; Green1987 ; Schwartz ; Weinberg ; RovelliQG . For external measurements, dx0αdx^{\alpha}_{0} acts as the minimum reference length, preventing the measurement of micro-lengths smaller than this threshold. This limitation imposes a natural cutoff on the smallest measurable scales, thus setting a lower bound for the length scale of the system. Since UV divergences in quantum field theory arise from summing over arbitrarily small distances (or high energy scales), imposing a minimum length scale like dx0αdx^{\alpha}_{0} effectively circumvents such divergences. Specifically, the Planck length, lp=Gc31.616×1035l_{p}=\sqrt{\frac{\hbar G}{c^{3}}}\approx 1.616\times 10^{-35} meters, serves as this fundamental minimum length, providing a physical cutoff at the Planck scale and thereby avoiding UV divergences. Conversely, for internal measurements, dx0αdx^{\alpha}_{0} functions as the maximum reference length, constraining the measurement of micro-lengths larger than this limit. This creates an upper bound for internal measurements. By setting dx0αdx^{\alpha}_{0} as the lower bound for external measurements, the framework naturally introduces a constraint on measurable length scales. This constraint inherently avoids UV divergence by preventing the system from probing arbitrarily small lengths or high energy scales, which are typically responsible for such divergences in field theories. This mechanism is akin to the non-perturbative quantum gravity frameworks like LQG, where spacetime is quantized, thereby preventing classical singularities and divergences. Moreover, it parallels string theory, wherein the finite size of strings acts as a natural cutoff for high-energy interactions, effectively avoiding UV divergence. In summary, by incorporating dx0αdx^{\alpha}_{0} as a critical scale, this framework provides a natural means of avoiding UV divergence through physical limits on the smallest measurable lengths, resonating with the Planck scale as a fundamental boundary in quantum gravity and quantum field theories.

However, the physical significance of the mapping constraints and their connection to fundamental constants like the Planck length would require further investigation and validation within the broader framework of theoretical physics.

VIII Scaling Klein-Gordon Equation and Dirac Equation

The Klein-Gordon and Dirac equations are essential in quantum mechanics and quantum field theory, describing the behavior of particles and fields while incorporating quantum and relativistic effects Schwartz ; Weinberg . Investigating scaling within these equations may offer insights into how particle fields behave in spacetimes with complex geometries. At extremely small scales, such as the Planck length, the classical notion of continuous spacetime might become inadequate, potentially giving rise to a network of quantized geometries RovelliQG . If spacetime indeed has a fluctuation structure, this could lead to modifications in the behavior of fields and particles.

From the operator transformations introduced in the second section, the Klein-Gordon equation and Dirac equation respective to the scale variables at the local micro-scale can be deduced and their forms in linear measuring spacetime can be obtained with mapping constraints. The Klein-Gordon equation bibitem16 ; bibitem17

{[mc]2}ϕ=0\displaystyle\{\Box-[\frac{mc}{\hbar}]^{2}\}\phi=0 (70)

can be written in scaling form of

{ημνa^μa^ν(2XμXνb^νXνXμXν)\displaystyle\{\eta^{\mu\nu}\hat{a}_{\mu}\hat{a}_{\nu}(\frac{\partial^{2}}{\partial X^{\mu}\partial X^{\nu}}-\hat{b}_{\nu}\frac{\partial X^{\nu}}{\partial X^{\mu}}\frac{\partial}{\partial X^{\nu}}) (71)
[rmrcr]2[dx0]2[m0]2[[dx0]/[dt0]]2[0]2}ϕ=0.\displaystyle-[\frac{r_{m}r_{c}}{r_{\hbar}}]^{2}\frac{[dx_{0}]^{2}[m_{0}]^{2}[[dx_{0}]/[dt_{0}]]^{2}}{[\hbar_{0}]^{2}}\}\phi=0.

Where =ημν2xμxν\Box=\eta^{\mu\nu}\frac{\partial^{2}}{\partial x^{\mu}\partial x^{\nu}}, ϕ=ϕ(xα)\phi=\phi(x^{\alpha}), rm=mm0r_{m}=\frac{m}{m_{0}} being the scaling measurement for particle mass, and r=0r_{\hbar}=\frac{\hbar}{\hbar_{0}} being the scaling measurement for Planck constant. After dimensional analysis, we get

{ημνa^μa^ν(2XμXνb^νXνXμXν)[rmrcr]2}ϕ=0£¬\displaystyle\{\eta^{\mu\nu}\hat{a}_{\mu}\hat{a}_{\nu}(\frac{\partial^{2}}{\partial X^{\mu}\partial X^{\nu}}-\hat{b}_{\nu}\frac{\partial X^{\nu}}{\partial X^{\mu}}\frac{\partial}{\partial X^{\nu}})-[\frac{r_{m}r_{c}}{r_{\hbar}}]^{2}\}\phi=0\textsterling\textlnot (72)

Here, ϕ=ϕ(xσx0σ+Lσ(Xσ)dx0σ)\phi=\phi(x^{\sigma}\rightarrow x^{\sigma}_{0}+L^{\sigma}(X^{\sigma})dx^{\sigma}_{0}), representing the fluctuation of the ϕ\phi field near x0σx^{\sigma}_{0} as driven by LσL^{\sigma} nonlinear fluctuates.

With the linear mapping conditions of

{xα=1dx0αX¯α,2xαxβ=1dx0αdx0β2X¯αX¯β,\begin{cases}&\frac{\partial}{\partial x^{\alpha}}=\frac{1}{dx_{0}^{\alpha}}\frac{\partial}{\partial\bar{X}^{\alpha}},\\ &\frac{\partial^{2}}{\partial x^{\alpha}\partial x^{\beta}}=\frac{1}{dx_{0}^{\alpha}dx_{0}^{\beta}}\frac{\partial^{2}}{\partial\bar{X}^{\alpha}\partial\bar{X}^{\beta}},\end{cases} (73)

we can similarly get the scaling Klein-Gordon equation expressed as

{ημν2X¯μX¯ν[rmrcr]2}ψ¯KG=0,\displaystyle\{\eta^{\mu\nu}\frac{\partial^{2}}{\partial\bar{X}^{\mu}\partial\bar{X}^{\nu}}-[\frac{r_{m}r_{c}}{r_{\hbar}}]^{2}\}\bar{\psi}_{KG}=0, (74)

where ψ¯KG(X¯σ)=ϕ[xσx0σ+(X¯σ1)dx0σ]\bar{\psi}_{KG}(\bar{X}^{\sigma})=\phi[x^{\sigma}\rightarrow x^{\sigma}_{0}+(\bar{X}^{\sigma}-1)dx^{\sigma}_{0}], representing the fluctuation of the ϕ\phi field near x0σx^{\sigma}_{0} as driven by X¯σ\bar{X}^{\sigma} linear fluctuates. Thus the linear measurement conditions can be expressed as

{dLαdXα=ζα(L¯αLα1);dζαdXα=[ζα]2b^α.\begin{cases}&\frac{dL^{\alpha}}{dX^{\alpha}}=\zeta^{\alpha}(\frac{\bar{L}^{\alpha}}{L^{\alpha}}-1);\\ &\frac{d\zeta^{\alpha}}{dX^{\alpha}}=[\zeta^{\alpha}]^{2}\hat{b}_{\alpha}.\end{cases} (75)

These conditions are the same as the ones for scaling Einstein field equations in the absence of any matter and scaling vacuum Einstein equations in the presence of a cosmological constant.

Following the same procedure, the Dirac equation bibitem18 ; bibitem19

[iγ^μxμmc]ψ=0\displaystyle[i\hat{\gamma}^{\mu}\frac{\partial}{\partial x^{\mu}}-\frac{mc}{\hbar}]\psi=0 (76)

with γ^μ\hat{\gamma}^{\mu} being gamma matrices, can be written in scaling form of

[iγ^μa^μXμrmrcr[dx0][m0][[dx0]/[dt0]][0]]ψ=0.\displaystyle[i\hat{\gamma}^{\mu}\hat{a}_{\mu}\frac{\partial}{\partial X^{\mu}}-\frac{r_{m}r_{c}}{r_{\hbar}}\frac{[dx_{0}][m_{0}][[dx_{0}]/[dt_{0}]]}{[\hbar_{0}]}]\psi=0. (77)

After dimensional analysis, we get

[iγ^μa^μXμrmrcr]ψ=0.\displaystyle[i\hat{\gamma}^{\mu}\hat{a}_{\mu}\frac{\partial}{\partial X^{\mu}}-\frac{r_{m}r_{c}}{r_{\hbar}}]\psi=0. (78)

Here, ψ=ψ(xσx0σ+Lσ(Xσ)dx0σ)\psi=\psi(x^{\sigma}\rightarrow x^{\sigma}_{0}+L^{\sigma}(X^{\sigma})dx^{\sigma}_{0}).

With the linear mapping conditions of

xα=1dx0αX¯α\displaystyle\frac{\partial}{\partial x^{\alpha}}=\frac{1}{dx_{0}^{\alpha}}\frac{\partial}{\partial\bar{X}^{\alpha}} (79)

the scaling Dirac equation is

[iγ^μX¯μrmrcr]ψ¯Dirca=0,\displaystyle[i\hat{\gamma}^{\mu}\frac{\partial}{\partial\bar{X}^{\mu}}-\frac{r_{m}r_{c}}{r_{\hbar}}]\bar{\psi}_{Dirca}=0, (80)

where ψ¯Dirca(X¯σ)=ψ[xσx0σ+(X¯σ1)dx0σ]\bar{\psi}_{Dirca}(\bar{X}^{\sigma})=\psi[x^{\sigma}\rightarrow x^{\sigma}_{0}+(\bar{X}^{\sigma}-1)dx^{\sigma}_{0}]. Thus, we have

dLαdXα=ζα(L¯αLα1).\displaystyle\frac{dL^{\alpha}}{dX^{\alpha}}=\zeta^{\alpha}(\frac{\bar{L}^{\alpha}}{L^{\alpha}}-1). (81)

The UV problem is also avoidable for the evolution of the equations (Eq. 74, 80) in spacetime described by X¯α\bar{X}^{\alpha}, in the case of X¯α>1\bar{X}^{\alpha}>1 (external measurements). The discussions for spacetime structures should be consistent with the previous section.

The scaling transformations of the Klein-Gordon and Dirac equations illustrate how changes in measurement scales can influence their forms. By incorporating scaling factors, this approach offers a potential step toward integrating quantum mechanics with the fluctuating geometry of spacetime. The shift from nonlinear to linear measurements introduces scaling factors, which impact the field equations. These transformations suggest that spacetime may possess a scaling nature, which could affect particle dynamics, thereby providing a new perspective on the relationship between quantum fluctuations and spacetime geometry. This approach may offer fresh insights into fundamental constants and quantum field theory, suggesting a possible connection between measurement scales and fundamental physics. However, further exploration and empirical validation are required to fully understand these implications.

IX Summary

The Planck length represents the smallest resolution in physics, where the quantum fluctuations of spacetime become evident, as inferred by the uncertainty principle. This article introduces a novel concept of spacetime microelement measurements with scaling factors, establishing a framework to explore the scaling behavior of spacetime at the Planck scale. In this framework, the microstructure of spacetime fluctuations can be characterized by three types which are stable, linear fluctuation, and non-linear fluctuations incorporated with a scaling function.

A scaling-characterized metric tensor is derived from the Lorentz scalar line element, which is expressed through micro measurements in the form of scaling functions. By applying local Lorentz transformations to these micro measurements, the spacetime structure coefficients can be defined, constraining the dimensions and components of spacetime in the rest frame. Besides, the scaled Lorentz factor at the micro-scale can be obtained from the constraint of them.

Key physical differential equations such as geodesic, Einstein field, Klein-Gordon, and Dirac can be transformed into scaling form, reflecting the localized spacetime dynamics properties at the micro-scale. Under stable conditions, spacetime can revert to a classical non-fluctuating state, with a symmetry of scale invariance by analyzing the renormalization group equations for micro measurements, corresponding to the fields and functions defined in the classical spacetime being stable. These equations acquire new forms characterized by the linear scale measurements X¯α\bar{X}^{\alpha}, within the mapping conditions on the scale transformation factors ζα\zeta^{\alpha}. In classical spacetime, differential equations capture the local properties of fields or spacetime functions, providing well-defined values at every point without fluctuations. In classical field theory, fields have clear, fixed values throughout spacetime. However, when spacetime experiences fluctuations, these values can become variable, driven by the spacetime fluctuations themselves. Near a given point x0αx^{\alpha}_{0} in spacetime, these functions depend on the spacetime fluctuations of XαX^{\alpha}. Once the spacetime fluctuations are linearly mapped and with given forms of measurements, these fields or functions can be defined at discrete points in spacetime, resulting in well-defined values. This indicates that the linear mapping constraints with given forms of measurements can help stabilize the fluctuations while leading to discretizing spacetime. Physics might be defined by fluctuating spacetime for the forms solved by the linear mapping constraints without preset forms.

It can be summarized that the mapping conditions yield three distinct types of constraints: (1) zeroth-order constraints, as given by Equation (68); (2) first-order constraints, as delineated by Equation (53); and (3) second-order constraints, which are represented by the second set of equations in Equation (65). Here, the term ’order’ refers to the order of differentiation of scaling functions Lα(Xα)L^{\alpha}(X^{\alpha}) with respect to scaling factors XαX^{\alpha} and also corresponds to the mapping orders between xαx^{\alpha} and X¯α\bar{X}^{\alpha}. Equations (59) and (60) represent the mapping constraints for proper measurements, connecting the coordinate-based measurements.

It is interesting to note that the golden ratio naturally emerged in the microscopic scale of linear measurements (Lα=XαL^{\alpha}=X^{\alpha}) with the mapping constraints, suggesting a fundamental reference length that restricts micro-length measurements to specific ranges. This insight provides a potential explanation for the existence of the Planck length in addressing the problem of UV divergence. In general, for arbitrary Lα=Lα(Xα)>0L^{\alpha}=L^{\alpha}(X^{\alpha})>0, the UV problem is avoidable for all the equations with the linear mapping conditions in the measurements of direction towards the Plank scale.

This work presents a coherent framework for understanding spacetime scaling at the Planck scale. While this is just the first step of a long march and these ideas are theoretically intriguing, they need further exploration and validation to assess the physical accuracy and relevance to spacetime and quantum gravity. The avoidable UV problem is at least a positive starting point. Future work will focus on identifying potential approaches to quantizing the scaling gravitational field equations in fluctuating spacetime at the Planck scale. While theoretical advancements have been made, direct experimental validation remains a challenge. Further research will explore the connections between this framework and established theories like string theory and loop quantum gravity. Indirect evidence for scaling structures might be pursued through high-energy physics experiments or cosmological observations, offering promising pathways to test the theoretical predictions.

Acknowledgements

We thank Dr. Baiyang Zhang and Dr. Yang Zhou for the interesting discussions and the suggestions for text editing. This work is supported by the National Natural Science Foundation of China with Grants No. 12475138 and 12147101, the Strategic Priority Research Program of Chinese Academy of Sciences (No. XDB34000000) and the Science and Technology Commission of Shanghai Municipality (23590780100).

References