Circular and Hyperbolic Symmetry Unified in Hyper-Spacetime

Abstract

A unified geometric framework for the full Lorentz group is introduced, based on a bounded angle parametrization of spacetime transformations within a hyper-spherical geometry. By mapping the unbounded hyperbolic angle $\phi$ to a bounded angle $\beta$ using the Gudermannian function, hyperbolic, causal, and Euclidean three-spheres are brought together into a single structure: hyper-spacetime. This structure unifies the Euclidean ${\mathbb{R}}^4$ and Minkowski ${\mathbb{R}}^{\mathrm{1,3}}$ domains, incorporates discrete symmetries in a continuous way, and removes discontinuities at the lightlike boundary. Each three-sphere carries a natural spinor set, encoding symmetry, and acting as eigen-spinors of corresponding observables. These reproduce the Dirac spectrum while confining singular behavior to a scalar factor. The bounded angle parametrization therefore provides a continuous, closed representation of the full Lorentz group and a transparent geometric basis for spacetime symmetry.

1. Introduction

The Lorentz group $O\left(\mathrm{1,3}\right)$ [1,2,3,4,5,6] underlies the symmetries of spacetime and forms the mathematical backbone of both classical and quantum relativistic physics. In its standard formulation, spatial rotations are described by compact angles on the circle, while boosts are parameterized by the unbounded rapidity $\phi \in (-\mathrm{\infty },+\mathrm{\infty })$. Although effective, this conventional parametrization exhibits several structural limitations:

• Rapidity diverges at the lightlike boundary $v\to \pm c$;
• Discrete transformations $\{P,T,PT\}$ remain algebraically disconnected from continuous Lorentz transformations;
• Euclidean and Minkowski spacetime structures are treated as fundamentally separate, linked only by analytic continuation or Wick rotation;
• Spinor solutions of the Dirac equation are usually derived analytically, rather than emerging directly from geometric structure.

• These issues motivate the need for a compact, continuous, and geometrically transparent representation of Lorentz symmetry, one that unifies continuous and discrete transformations while clarifying the relationship between Euclidean and Minkowski domains.

1.1. Motivation

The divergence of rapidity at the lightlike limit is not merely a coordinate inconvenience: it obscures geometric relations between boosts and rotations, interrupts continuity at $v=\pm c$, and masks the structural similarity between hyperbolic and circular symmetries. Moreover, discrete spacetime reflections remain isolated algebraic operations in the conventional Lorentz group, preventing smooth interpolation between parity P, time reversal T, and the identity component I. A compact parametrization that connects these sectors continuously would offer a coherent geometric understanding of the full Lorentz group.

At the same time, many modern formalisms, from path integrals to Euclidean field theory and particle classification, rely on controlled transitions between Minkowski and Euclidean metrics [7]. Standard Wick rotation introduces imaginary time as a technical device, but its geometric meaning remains conceptually opaque [8,9,10]. A structural framework that embeds both domains within a single real geometry would provide a transparent foundation for analytic continuation and symmetry-based reasoning.

These motivations converge in the search for a unified geometric representation capable of handling boosts, rotations, discrete symmetries, and Euclidean/Minkowski duality in a single continuous mathematical object.

1.2. Research Gap and Objectives

Despite extensive research on Lorentz geometry [11], no previous framework provides the following:

• A bounded and continuous parametrization covering the full Lorentz group.
• A real geometric structure unifying Euclidean and Minkowski domains.
• Spinor sets that simultaneously encode symmetry, discrete operations, and Dirac eigen-spinors.
• A compact angular coordinate that regularizes the lightlike boundary.

This paper aims to fill these gaps through the following objectives:

• Unify circular and hyperbolic symmetry via the bounded angle $\beta$.
• Construct a triplet of three-spheres forming hyper-spacetime.
• Develop spinor sets that derive Dirac eigen-spinors geometrically.
• Provide a continuous representation of the full Lorentz group, including discrete reflections.
• Bridge Euclidean and Minkowski metrics through a natural geometric duality.

1.3. Central Idea: A Bounded Angular Parametrization

The key innovation of this work is the introduction of a bounded angular variable $\beta$, obtained through the Gudermannian mapping $\phi ={\mathrm{t}\mathrm{a}\mathrm{n}\mathrm{h}}^{-1}\left(\mathrm{s}\mathrm{i}\mathrm{n}\left(\beta \right)\right)$ [12,13,14] (Appendix B). This mapping transforms the unbounded rapidity parameter into a bounded angular domain, effectively compactifying the boost parameter space. In doing so, it closes the hyperbola into a hyperbolic one-sphere ${\mathbb{S}}_H^1$ and provides a continuous, finite coordinate for Lorentz boosts [15,16]. Replacing rapidity $\phi$ with the bounded angle β produces several important consequences:

• The lightlike boundary becomes a regular point of the domain.
• Divergences in boosts are isolated in a scalar density, while spinors remain finite.
• Both branches of the hyperbola are traversed continuously.
• Temporal orientation changes correspond to smooth shifts in $\beta$, turning a discrete transformation into a continuous operation.

This compactification unifies hyperbolic and circular symmetries, creating a single angular structure that links rotations, boosts and reflections across the full Lorentz group.

1.4. Hyper-Spacetime: A Unified Three-Sphere Geometry

Building on the bounded parametrization, this work introduces hyper-spacetime, a unified geometric structure constructed from a triplet of three-spheres: $ℬ=\{{\mathbb{S}}_H^3, {\mathbb{S}}_C^3, {\mathbb{S}}^3\}$:

• ${\mathbb{S}}_H^3\subset {\mathbb{R}}^{\mathrm{1,3}}$ is a hyperbolic unit sphere representing normalized momentum.
• ${\mathbb{S}}_C^3\subset {\mathbb{R}}^{\mathrm{1,3}}$ is a causal sphere encoding spacetime intervals.
• ${\mathbb{S}}^3\subset {\mathbb{R}}^4$ is a Euclidean sphere preserving the same temporal and spatial orientation.

All three share a common temporal axis and a reciprocal temporal bivector plane, establishing a correspondence between spatial vectors in the Minkowski domain and temporal bivectors in the Euclidean domain, and vice versa. This duality creates a continuous geometric bridge linking the Minkowski and Euclidean representations.

1.5. Spinors, Observables, and the Dirac Spectrum

Within this unified geometry, spinor sets $\left\{U_j\right\}$ and $\left\{V_j\right\}$ arise directly from variations in the hyper-spherical coordinates $(\beta ,\theta ,\varphi )$. These spinor sets act simultaneously as:

• Symmetry generators preserving the three-spheres;
• Eigen-spinors of geometric observables $\{p,q,u_r\}$;
• Continuous representatives of the discrete operations $\{I,P,T,PT\}$;
• A geometric reconstruction of the four Dirac plane-wave solutions.

Crucially, the Dirac spectrum emerges without solving a differential equation: it arises geometrically from the structure of hyper-spacetime, demonstrating that relativistic spinors are intrinsic to the unified geometry.

1.6. Novelty and Contribution

• The resulting framework provides the following:

• A closed, continuous, and bounded representation of the full Lorentz group $O\left(\mathrm{1,3}\right)$;
• A unified spinor structure generating the Dirac spectrum directly;
• Continuity across discrete symmetries and the lightlike boundary;
• A new geometric interpretation of Wick rotation;
• A compactified Lorentz parameter suitable for quantization and field-theoretic formulations;
• A pedagogically transparent geometric picture of spacetime symmetry.

The remainder of this work develops this structure rigorously, derives the related spinors and observables, and discusses both physical implications and potential applications.

1.7. Layout of the Paper

The core of the paper (Section 2, Section 3, Section 4, Section 5 and Section 6) develops the geometric framework. Section 2 and Section 3 present the bounded angular parametrization of Lorentz boosts that unifies circular and hyperbolic symmetry and applies naturally to special relativity, yielding harmonic relativistic proportionality factors [17,18]. Section 4 extends to four dimensions, a triplet of three-spheres is introduced that defines hyper-spacetime and shows how the full Lorentz group, with both continuous and discrete symmetries, emerges within its hyper-spherical coordinates. In Section 5 and Section 6, spinor sets are then constructed and analyzed as eigen-spinors of geometric observables, reproducing the Dirac spectrum while confining singularities to scalar factors. The final part of the paper (Section 7 and Section 8) turns to interpretation and outlook, discussing the physical implications of hyper-spacetime, and concludes with a summary of its unifying features.

1.8. Mathematical Formalism

The mathematical formalism throughout is based on the geometric algebra (GA) of spacetime (STA), as developed by Hestenes [19,20] (Appendix A). Its foundations trace back to Grassmann [21] and Clifford [22], whose work established a unified algebra of vectors, bivectors, and higher-grade multivectors. In this algebra, Lorentz transformations are expressed naturally through rotors, which generalize rotations and boosts in a coordinate-free manner [23,24,25,26,27]. In STA [19], a spacetime inertial frame $\{t,x,y,z\}$ is represented by four orthogonal basis vectors ${\gamma }_{\mu }=\{{\gamma }_0,{\gamma }_1,{\gamma }_2,{\gamma }_3\},$ which satisfy the real Clifford-algebra [7,28] relation ${\gamma }_{\mu }{\gamma }_{\nu }+{\gamma }_{\nu }{\gamma }_{\mu }=2{\eta }_{\mu \nu },$ equivalent to the algebra of the Dirac gamma matrices [4]. This framework provides the natural setting for the bounded parametrization, the three-sphere geometry, and the spinor sets constructed later in the paper.

2. Hyperbolic Rotation

Lorentz boosts are conventionally expressed as hyperbolic rotations, parameterized by the unbounded angle $\phi \in \left(-\mathrm{\infty },+\mathrm{\infty }\right)$ (rapidity) (Figure 1a).

Figure 1. Comparison of hyperbolic rotation. (a) In the unbounded parametrization, the rotor $R_{\mathcal{z}}\left(\phi \right)$ covers only one branch ${\mathbb{H}}_{+}^1$, with a discontinuity at lightlike boundaries. (b) Using the bounded angle $\beta$, the rotor $L_{\mathcal{z}}\left(\beta \right)$ spans the full symmetry ${\mathbb{S}}_H^1={\mathbb{H}}_{+}^1⨁{\mathbb{H}}_{-}^1$. The Gudermannian mapping ensures smooth continuity through infinity, closing the hyperbola into a one-sphere ${\mathbb{S}}_H^1$.

• A boost along the ${\gamma }_3$-axis ($\mathcal{z}$-axis) is generated by the hyperbolic rotor $R_{\mathcal{z}}\left(\phi \right)$:

$$R_{\mathcal{z}}\left(\phi \right)=\mathrm{e}\mathrm{x}\mathrm{p}\left(\phi {\sigma }_3/2\right)=\mathrm{c}\mathrm{o}\mathrm{s}\mathrm{h}\left(\phi /2\right)+\mathrm{s}\mathrm{i}\mathrm{n}\mathrm{h}\left(\phi /2\right){\sigma }_3, \phi \in \left(-\mathrm{\infty },+\mathrm{\infty }\right), R_{\mathcal{z}}{\tilde{R}}_{\mathcal{z}}=1$$

(1)

where bivector ${\sigma }_3={\gamma }_3{\gamma }_0$ represents the temporal plane of rotation. Acting on the temporal basis vector ${\gamma }_0$, the rotor generates the boosted spacetime vector $w\left(\phi \right)$:

$$w\left(\phi \right)=R_{\mathcal{z}}{\gamma }_0{\tilde{R}}_{\mathcal{z}}=\cosh \left(\phi \right){\gamma }_0+\sinh \left(\phi \right){\gamma }_3, {‖w\left(\phi \right)‖}^2=1$$

(2)

However, rotor $R_{\mathcal{z}}\left(\phi \right)$ only covers the positive branch ${\mathbb{H}}_{+}^1$ of the hyperbola. The negative branch ${\mathbb{H}}_{-}^1$ of the hyperbola is not present (Figure 1a).

To cover the full hyperbolic symmetry in a single parameter domain, the unbounded angle $\phi \in \left(-\mathrm{\infty },+\mathrm{\infty }\right)$ is related to the bounded angle $\beta \in \left[0, 2\pi \right]$ by using the Gudermannian function $\phi ={\mathrm{t}\mathrm{a}\mathrm{n}\mathrm{h}}^{-1}\left(\mathrm{s}\mathrm{i}\mathrm{n}\left(\beta \right)\right)$ (Appendix B) [12,13]. Substituting this function into $R_{\mathcal{z}}\left(\phi \right)$ yields the rotor $L_z\left(\beta \right)$:

$$\begin{array}{cc}{L}_{\mathcal{z}}\left(\beta \right)=\mathrm{e}\mathrm{x}\mathrm{p}\left({\mathrm{t}\mathrm{a}\mathrm{n}\mathrm{h}}^{-1}\left(\mathrm{s}\mathrm{i}\mathrm{n}\left(\beta \right)\right){\sigma }_3/2\right)=\sqrt{\sec \left(\beta \right)}{L}_{u1}\left(\beta \right),\hfill & L_{\mathcal{z}}{\tilde{L}}_{\mathcal{z}}=1\hfill \\ L_{u1}\left(\beta \right)=\mathrm{c}\mathrm{o}\mathrm{s}\left(\beta /2\right)+\mathrm{s}\mathrm{i}\mathrm{n}\left(\beta /2\right){\sigma }_3,\hfill & L_{u1}{\tilde{L}}_{u1}=\cos \left(\beta \right)\hfill \end{array}$$

(3)

The scalar factor $\sqrt{\sec \left(\beta \right)}$ ensures normalization, while $L_{u1}\left(\beta \right)$ acts as a temporal spinor (Appendix C). Applying rotor $L_{\mathcal{z}}\left(\beta \right)$ to ${\gamma }_0$ generates the boosted spacetime vector $w\left(\beta \right)$:

$$w\left(\beta \right)=L_{\mathcal{z}}{\gamma }_0{\tilde{L}}_{\mathcal{z}}=\sec \left(\beta \right){\gamma }_0+\tan \left(\beta \right){\gamma }_3, \beta \in \left[0,2\pi \right], {‖w\left(\beta \right)‖}^2=1$$

(4)

where the full hyperbolic symmetry is covered continuously (Figure 1b).

In summary, the bounded angle parametrization provides several advantages. It removes singularities by isolating them in the scalar density factor $\sqrt{\sec \left(\beta \right)}$, while the associated spinor remains regular. At $\beta =\pm \pi /2$, the mapping passes smoothly through infinity, ensuring continuity across the lightlike boundary where crossing corresponds to a time reversal. The two disconnected hyperbolic branches ${\mathbb{H}}_{+}^1$ and ${\mathbb{H}}_{-}^1$ are thereby closed into a single hyperbolic one-sphere ${\mathbb{S}}_H^1$ (Figure 1b). In this way, hyperbolic symmetry is unified within a single angular cycle.

3. Harmonic Relativistic Proportionality Factors

In special relativity, the relative speed $v/c$ is conventionally mapped to the unbounded angle $\phi \in \left(-\mathrm{\infty },+\mathrm{\infty }\right)$ (rapidity). Using instead the bounded angle $\beta \in \left[0, 2\pi \right]$ introduced in Section 2, this mapping provides a harmonic set of relativistic proportionality factors:

$$\begin{array}{cc}\mathrm{s}\mathrm{i}\mathrm{n}\left(\beta \right)=\pm v/c,\hfill & \mathrm{c}\mathrm{o}\mathrm{s}\left(\beta \right)=\pm \sqrt{1-{\left(v/c\right)}^2}\hfill \\ \sec \left(\beta \right)={\displaystyle \frac{1}{\pm \sqrt{1-{\left(v/c\right)}^2}}},\hfill & \tan \left(\beta \right)={\displaystyle \frac{\pm v/c}{\pm \sqrt{1-{\left(v/c\right)}^2}}}\hfill \end{array}$$

(5)

These factors form a bridge between circular and hyperbolic symmetry:

$$\begin{gathered} {\mathrm{s}\mathrm{i}\mathrm{n}}^2\left(\beta \right)+{\mathrm{c}\mathrm{o}\mathrm{s}}^2\left(\beta \right)=1, {\mathrm{s}\mathrm{e}\mathrm{c}}^2\left(\beta \right)-{\mathrm{t}\mathrm{a}\mathrm{n}}^2\left(\beta \right)=1 \\ {{\mathbb{S}}^1\subset \mathbb{R}}^2 ⟷ {{\mathbb{S}}_H^1\subset \mathbb{R}}^{\mathrm{1,1}} \end{gathered}$$

(6)

Consequently, the bounded angle mapping unifies circular ${{\mathbb{S}}^1\subset \mathbb{R}}^2$ with hyperbolic ${{\mathbb{S}}_H^1\subset \mathbb{R}}^{\mathrm{1,1}}$ symmetry (Figure 1b). A complete cycle on one-sphere ${\mathbb{S}}^1{\subset \mathbb{R}}^2$ corresponds one-to-one with a complete cycle on hyperbolic one-sphere ${\mathbb{S}}_H^1{\subset \mathbb{R}}^{\mathrm{1,1}}$. This includes a smooth passage through infinity at the lightlike boundaries $\beta =\pm \pi /2$.

To incorporate all the symmetries of the full Lorentz group $O\left(1, 3\right)$, the framework must extend from the two-dimensional (2D) relation ${\mathbb{R}}^2 {⟷\mathbb{R}}^{\mathrm{1,1}}$ to a four-dimensional (4D) relation that unifies the Euclidean domain ${\mathbb{R}}^4$ with the Minkowski domain ${\mathbb{R}}^{\mathrm{1,3}}$.

4. One Unified Geometry Bridging ${\mathbb{R}}^4$ and ${\mathbb{R}}^{\mathrm{1,3}}$

The generalization from two to four dimensions is realized by the introduction of a triplet of three-spheres embedded in a Euclidean $\left\{{\gamma }_0,{\sigma }_k\right\}{\subset \mathbb{R}}^4$ and a Minkowski $\left\{{\gamma }_0,{\gamma }_k\right\}\subset {\mathbb{R}}^{\mathrm{1,3}}$ domain (Appendix A). Accordingly, three distinct but related three-spheres are defined as follows:

$$\begin{array}{cc}{\mathbb{S}}_H^3=\left\{p =a_0{\gamma }_0+a_k{\gamma }_k\in {\mathbb{R}}^{\mathrm{1,3}}|a_{\mu }\in \mathbb{R},{ ‖p‖}^2=1\right\},\hfill & \mathrm{m}\mathrm{e}\mathrm{t}\mathrm{r}\mathrm{i}\mathrm{c}:\left\{+1,-1,-1,-1\right\}\hfill \\ {\mathbb{S}}_C^3=\left\{q = {\gamma }_0+a_k{\gamma }_k\in {\mathbb{R}}^{\mathrm{1,3}}|{a_k\in \mathbb{R}, ‖q‖}^2={\cos }^2\left(\beta \right)\right\},\hfill & \mathrm{m}\mathrm{e}\mathrm{t}\mathrm{r}\mathrm{i}\mathrm{c}:\left\{+1,-1,-1,-1\right\}\hfill \\ {\mathbb{S}}^3=\left\{u_r=a_0{\gamma }_0+a_k{\sigma }_k\in {\mathbb{R}}^4|{a_{\mu }\in \mathbb{R},{\sigma }_k={\gamma }_k{\gamma }_0,‖u_r‖}^2=1\right\},\hfill & \mathrm{m}\mathrm{e}\mathrm{t}\mathrm{r}\mathrm{i}\mathrm{c}:\left\{+1,+1,+1,+1\right\}\hfill \end{array}$$

(7)

Here,

• The hyperbolic three-sphere ${\mathbb{S}}_H^3$ is preserved by spacetime rotor ${\Lambda }_1$ (Figure 2b).
• The causal three-sphere ${\mathbb{S}}_C^3$ is preserved by spacetime spinor $U_1$ (Figure 3a).
• The Euclidean three-sphere ${\mathbb{S}}^3$ is preserved by Euclidean spinor $V_1$ (Figure 3b).

Each of these three-spheres is preserved by a specific spinor structure (as defined in Section 4.1), which ensures that the geometry remains invariant under both Lorentzian and Euclidean transformations. In this way, every three-sphere is not only defined by its metric but also carries a natural spinor representation that encodes its symmetry.

Figure 2. (a) The spatial two-sphere ${\mathbb{S}}_{\mathrm{0,2}}^2 {\subset \mathbb{R}}^{0,3}$, spanned by vectors $e_3\left(\theta ,\varphi \right)$, is preserved by the spatial spinor $S_1$. (b) The hyperbolic three-sphere ${\mathbb{S}}_H^3\subset {\mathbb{R}}^{\mathrm{1,3}}$, spanned by vectors $p$, is preserved by the spacetime rotor ${\Lambda }_1$. The spatial vectors $e_3\in {\mathbb{S}}_{\mathrm{0,2}}^2$ are all orthogonal to the temporal axis ${\gamma }_0$.

Figure 3. (a) The causal three-sphere ${\mathbb{S}}_C^3\subset {\mathbb{R}}^{\mathrm{1,3}}$, spanned by vectors $q$, is preserved by the spacetime spinor $U_1$. (b) The Euclidean three-sphere ${\mathbb{S}}^3\subset {\mathbb{R}}^4$, spanned by vectors $u_r$, is preserved by the Euclidean spinor $V_1$. In this structure, each of the aligned vectors $e_3\in {\mathbb{S}}_{\mathrm{0,2}}^2$ and $u_3\in {\mathbb{S}}^2$ is orthogonal to the temporal axis ${\gamma }_0$ in its respective domain, thereby fixing a reciprocal temporal bivector plane.

All three-spheres share the following: a common temporal axis ${\gamma }_0$, a common origin (spacetime event), and a reciprocal temporal bivector plane. They differ in their metric and spatial subspaces $\left\{{\gamma }_k\right\}\subset {\mathbb{R}}^{\mathrm{1,3}}$ and $\left\{{\sigma }_k\right\}\subset {\mathbb{R}}^4$ (Equation (7)), which define two complementary two-spheres:

$$\begin{gathered} {\mathbb{S}}_{\mathrm{0,2}}^2=\left\{e_3=a_k{\gamma }_k\in {\mathbb{R}}^{\mathrm{0,3}} | a_k\in \mathbb{R},{\left(e_3\right)}^2=-1\right\} \\ {\mathbb{S}}^2=\left\{u_3=a_k{\sigma }_k\in {\mathbb{R}}^{\mathrm{3,0}} | a_k\in \mathbb{R},{\left(u_3\right)}^2=+1\right\} \end{gathered}$$

(8)

Both two-spheres are preserved by spatial spinor $S_1$ (Figure 2a):

$$S_1\left(\theta ,\varphi \right)=\mathrm{e}\mathrm{x}\mathrm{p}\left({-\mathbb{i}\sigma }_3\varphi /2\right)\mathrm{e}\mathrm{x}\mathrm{p}\left({-\mathbb{i}\sigma }_2\theta /2\right), S_1{\tilde{S}}_1=1, S_1{\gamma }_0{\tilde{S}}_1={\gamma }_0$$

(9)

Applying spinor $S_1$ to ${\gamma }_3$ and ${\sigma }_3$ generates the spatial unit vectors $e_3$ and $u_3$:

$$\begin{array}{ccc}{e}_3\left(\theta ,\varphi \right)=S_1{\gamma }_3{\tilde{S}}_1=\sin \left(\theta \right)\cos \left(\varphi \right){\gamma }_1+\sin \left(\theta \right)\sin \left(\varphi \right){\gamma }_2+\cos \left(\theta \right){\gamma }_3,\hfill & {\left(e_3\right)}^2=-1,\hfill & e_3=u_3{\gamma }_0\hfill \\ u_3\left(\theta ,\varphi \right)=S_1{\sigma }_3{\tilde{S}}_1=\sin \left(\theta \right)\cos \left(\varphi \right){\sigma }_1+\sin \left(\theta \right)\sin \left(\varphi \right){\sigma }_2+\cos \left(\theta \right){\sigma }_3,\hfill & {\left(u_3\right)}^2=+1,\hfill & u_3=e_3{\gamma }_0\hfill \end{array}$$

(10)

They are orthogonal to ${\gamma }_0$, aligned $\left(e_3\wedge u_3=0\right)$, and define spatial direction. Moreover, they span a reciprocal temporal bivector plane $\left(e_3=u_3{\gamma }_0\leftrightarrow u_3=e_3{\gamma }_0\right)$, which is a cornerstone of the unified geometry. The Minkowski vector $e_3\in {\mathbb{R}}^{\mathrm{1,3}}$ acts as a temporal bivector in the Euclidean domain, while the Euclidean vector $u_3{\in \mathbb{R}}^4$ act as a temporal bivector in the Minkowski domain. This geometrical duality specifies spatial direction while simultaneously encoding for temporal orientation in the opposite domain. Their associated dual spatial bivector planes $\mathbb{i}{u}_3$ belongs to the common three-dimensional even subalgebra (Appendix A), ensuring domain-independence of spatial orientation.

4.1. Definition of the Spinors $\left\{U_1,V_1\right\}$, Rotor ${\Lambda }_1=\rho U_1$, and Vectors $\left\{p,q,u_r\right\}$

The two spinors $\left\{U_1,V_1\right\}$, and associated rotor ${\Lambda }_1=\rho U_1$, form a spinor structure that preserves the triplet of three-spheres $\left\{{\mathbb{S}}_H^3,{\mathbb{S}}_C^3,{\mathbb{S}}^3\right\}$ (Figure 2 and Figure 3). Thus, every three-sphere carries a natural spinor representation that encodes its symmetry. The Euclidean spinor $V_1$ (preserving ${\mathbb{S}}^3$) and spacetime spinor $U_1$ (preserving ${\mathbb{S}}_C^3$ and ${\mathbb{S}}_H^3$) are defined as

$$\begin{array}{ccc}{V}_1\left(\beta ,\theta ,\varphi \right)=S_1\left(\theta ,\varphi \right)L_{\mathrm{v}1}\left(\beta \right),\hfill & L_{\mathrm{v}1}\left(\beta \right)=\mathrm{c}\mathrm{o}\mathrm{s}\left(\beta /2\right)+\mathrm{s}\mathrm{i}\mathrm{n}\left(\beta /2\right){\gamma }_3,\hfill & V_1{V}_1^{-1}=1\hfill \\ U_1\left(\beta ,\theta ,\varphi \right)=S_1\left(\theta ,\varphi \right)L_{u1}\left(\beta \right),\hfill & L_{u1}\left(\beta \right)=\mathrm{c}\mathrm{o}\mathrm{s}\left(\beta /2\right)+\mathrm{s}\mathrm{i}\mathrm{n}\left(\beta /2\right){\sigma }_3,\hfill & U_1{\tilde{U}}_1=\cos \left(\beta \right)\hfill \\ {\Lambda }_1\left(\beta ,\theta ,\varphi \right)=\sqrt{\sec \left(\beta \right)}{U}_1\left(\beta ,\theta ,\varphi \right),\hfill & & {\Lambda }_1{\tilde{\Lambda }}_1=1\hfill \end{array}$$

(11)

Here $S_1$ acts as a spatial spinor (Equation (9)), $L_{\mathrm{v}1}$ and $L_{u1}$ act as temporal spinors (Appendix C), and the scalar factor $\sqrt{\sec \left(\beta \right)}$ ensures the unitarity of rotor ${\Lambda }_1$, the normalized form of $U_1$. Applying the spinors $U_1$ and $V_1$ yields the vectors spanning the three-spheres:

$$\begin{array}{cc}p\in {\mathbb{S}}_H^3: p\left(\beta ,\theta ,\varphi \right)={\Lambda }_1{\gamma }_0{\tilde{\Lambda }}_1=\sec \left(\beta \right){\gamma }_0+\tan \left(\beta \right)e_3\left(\theta ,\varphi \right),\hfill & {‖p‖}^2=1\hfill \\ q\in {\mathbb{S}}_C^3: q\left(\beta ,\theta ,\varphi \right)=U_1{\gamma }_0{\tilde{U}}_1= {\gamma }_0+\sin \left(\beta \right)e_3\left(\theta ,\varphi \right),\hfill & {‖q‖}^2={\cos }^2\left(\beta \right)\hfill \\ u_r\in {\mathbb{S}}^3: u_r\left(\beta ,\theta ,\varphi \right)=V_1{\gamma }_0{V}_1^{-1}=\cos \left(\beta \right){\gamma }_0+\sin \left(\beta \right)u_3\left(\theta ,\varphi \right),\hfill & {‖u_r‖}^2=1\hfill \end{array}$$

(12)

Here, $p\in {\mathbb{S}}_H^3$ is a hyperbolic unit vector, $q\in {\mathbb{S}}_C^3$ is a causal vector with variable norm, and $u_r\in {\mathbb{S}}^3$ is a Euclidean unit vector. The causal three-sphere ${\mathbb{S}}_C^3$ covers the spacetime region bounded by the light cone of a past event (Figure 3a). Each causal vector $q\in {\mathbb{S}}_C^3$ is future pointing and its norm represents proper length, vanishing at the lightlike boundaries. In this way, ${\mathbb{S}}_C^3$ integrates a natural form of causality in the triplet of three-spheres.

4.2. Geometric Duality

A central feature of hyper-spacetime is the geometric duality between the Minkowski and Euclidean domains, expressed directly through the spacetime spinor $U_1$ and the Euclidean spinor $V_1$ (Equation (11)). This duality is governed by the temporal spinors $L_{u1}$ and $L_{v1}$, which are defined by the temporal bivectors

$$\left[ {\gamma }_3\in {\mathbb{R}}^{\mathrm{1,3}} \leftrightarrow {\gamma }_3={\sigma }_3{\gamma }_0\subset {\mathbb{R}}^4 \right] \leftrightarrow \left[ {\sigma }_3\in {\mathbb{R}}^4 \leftrightarrow {\sigma }_3={\gamma }_3{\gamma }_0\subset {\mathbb{R}}^{\mathrm{1,3}} \right].$$

This relation shows that the temporal bivector ${\sigma }_3{\gamma }_0\subset {\mathbb{R}}^4$ acts as the spatial basis vector ${\gamma }_3\in {\mathbb{R}}^{\mathrm{1,3}}$, while the temporal bivector ${\gamma }_3{\gamma }_0\subset {\mathbb{R}}^{\mathrm{1,3}}$ acts as the spatial basis vector ${\sigma }_3\in {\mathbb{R}}^4$. With this structure in place, the only difference between $U_1$ and $V_1$ is the domain to which the temporal bivector resides. Their spatial component $S_1$ (Equations (9) and (11)) is identical in both cases, since the spatial bivectors $\mathbb{i}{\sigma }_k$ belong to the shared three-dimensional even subalgebra common to both metrics (Appendix A).

This establishes the geometric duality transparently: a vector (spatial direction) in one domain corresponds to a bivector (orientation) in the other. The combined spinors $U_1=S_1{L}_{u1}$ and $V_1=S_1{L}_{v1}$, therefore, encode the same orientation data, expressed within two different metric signatures. Each spinor preserves its associated three-spheres: $U_1$ preserves ${\mathbb{S}}_H^3$ and ${\mathbb{S}}_C^3$, while $V_1$ preserves ${\mathbb{S}}^3$. Consequently, the same angular coordinates $(\beta ,\theta ,\varphi )$ generate parallel spinor structures in both domains. This illustrates how the unified hyper-spacetime geometry emerges from the vector ↔ bivector duality linking the Euclidean and Minkowski representations.

In summary, the three-spheres $\left\{{\mathbb{S}}_H^3,{\mathbb{S}}_C^3,{\mathbb{S}}^3\right\}$ (Equation (7)) exhibit the following features:

• A common temporal axis ${\gamma }_0$ with a shared origin (spacetime event).
• Unit vectors $e_3\in {\mathbb{R}}^{\mathrm{1,3}}$ and $u_3{\in \mathbb{R}}^4$ that encode spatial direction and temporal orientation through the reciprocal relation $\left\{e_3=u_3{\gamma }_0\leftrightarrow u_3=e_3{\gamma }_0\right\}$, expressing a geometric duality between domains.
• Domain-independent spatial bivector planes $\mathbb{i}{u}_3\subset {\mathbb{R}}^3$, common to both domains.

A complete cycle on the Euclidean three-sphere ${\mathbb{S}}^3$ corresponds one-to-one with a complete cycle on hyperbolic three-sphere ${\mathbb{S}}_H^3$, thereby unifying ${\mathbb{R}}^4$ and ${\mathbb{R}}^{1,3}$. The apparent boundary at infinity ($\beta =\pm \pi /2$) is absorbed smoothly, making the entire structure closed and traversable. The unified geometry constructed from the triplet of three-spheres $\left\{{\mathbb{S}}_H^3,{\mathbb{S}}_C^3,{\mathbb{S}}^3\right\}$ is referred to as hyper-spacetime $ℬ$:

$$ℬ=\left\{{\mathbb{S}}_H^3,{\mathbb{S}}_c^3,{\mathbb{S}}^3\right\}$$

(13)

Its coordinates are given by the hyper-spherical set $\left(\beta ,\theta ,\varphi \right)$, where the spatial angles $\left(\theta ,\varphi \right)$ encode direction, and the temporal angle $\beta$ encodes relative speed (Equation (5)). Hence, the familiar relativistic parameters of direction and speed are reformulated as angular variables in a closed domain, and continuity at the lightlike boundaries.

5. Full Lorentz Group

The full Lorentz group $O\left(\mathrm{1,3}\right)$ [29,30,31] contains the symmetries of spacetime that preserve the Minkowski metric. It includes the following: (1) continuous transformations as boosts and spatial rotations, and (2) spacetime event reflections $\left\{I,P,T,PT\right\}$: identity (I), parity (P), time-reversal (T), and spacetime-reversal (PT). Thus, the full Lorentz group is defined as

$$\mathrm{O}\left(\mathrm{1,3}\right)=\left\{I,P,T,PT\right\}.S{O}^{+}\left(\mathrm{1,3}\right)$$

(14)

where $S{O}^{+}\left(\mathrm{1,3}\right)$ is the proper orthochronous Lorentz subgroup connected to identity.

In the conventional formalism, boosts in $S{O}^{+}\left(\mathrm{1,3}\right)$ are parameterized by the unbounded angle $\phi \in \left(-\infty ,+\infty \right)$, leading to singularities at the lightlike boundaries. Moreover, the discrete reflections $\left\{P,T,PT\right\}$ remain disconnected from identity. The standard way to extend the full Lorentz group $O\left(\mathrm{1,3}\right)$ is through its double cover $\mathrm{P}\mathrm{i}\mathrm{n}\left(\mathrm{1,3}\right)$, as it includes both proper and improper transformations [31]. However, even within $\mathrm{P}\mathrm{i}\mathrm{n}\left(\mathrm{1,3}\right)$, the discrete transformations remain disconnected from identity, leaving a gap between reflections and continuous transformations. This gap is closed by hyper-spacetime, in which continuous and discrete symmetries arise naturally within a unified geometry.

5.1. A Unified Geometry

In the hyper-spherical coordinates $\left(\beta ,\theta ,\varphi \right)$ of hyper-spacetime (defined in Section 4), the spacetime event reflections $\left\{I,P,T,PT\right\}$ manifest naturally as smooth angular transformations:

$$\begin{array}{ccc}\mathrm{Identity}\hfill & I\hfill & :\left(\pm \beta ,\theta ,\varphi \right)\hfill \\ \mathrm{Parity}\hfill & P\hfill & :\left(\mp \beta ,\theta \pm \pi ,\varphi \right)\hfill \\ \mathrm{Time}-\mathrm{reversal}\hfill & T\hfill & :\left(\mp \beta \pm \pi , \theta ,\varphi \right)\hfill \\ \mathrm{Spacetime}-\mathrm{reversal}\hfill & PT\hfill & :\left(\pm \beta \pm \pi ,\theta \pm \pi ,\varphi \right)\hfill \end{array}$$

(15)

These transformations correspond to changes in temporal orientation ($\pm$ sign changes or $\pm \pi$ shifts in $\beta$) and spatial orientation ($\pm \pi$ shifts in $\theta$). Crucially, all four reflections are smoothly connected to identity, eliminating discontinuities.

5.2. Spinor Representations

The spinor structure of hyper-spacetime provides explicit representations of the $\left\{I,P,T,PT\right\}$ transformations. Starting from the spacetime spinor $U_1\left(\beta ,\theta ,\varphi \right)$, variations in the hyper-spherical coordinates $\left(\beta ,\theta ,\varphi \right)$ generate the full set of spacetime spinors $\left\{U_{\mathrm{j}}\right\}$, where each of the spinors represents one of the $\left\{I,P,T,PT\right\}$ transformations:

$$\begin{array}{cc}I:\hfill & U_1\left(\beta ,\theta ,\varphi \right)=U_1\left(+\beta ,\theta ,\varphi \right)=S_1\left(\theta ,\varphi \right)\left(+\mathrm{c}\mathrm{o}\mathrm{s}\left(\beta /2\right)+\mathrm{s}\mathrm{i}\mathrm{n}\left(\beta /2\right){\sigma }_3\right)\hfill \\ P:\hfill & U_2\left(\beta ,\theta ,\varphi \right)=U_1\left(-\beta , \theta +\pi ,\varphi \right)=S_2\left(\theta ,\varphi \right)\left(+\mathrm{c}\mathrm{o}\mathrm{s}\left(\beta /2\right)-\mathrm{s}\mathrm{i}\mathrm{n}\left(\beta /2\right){\sigma }_3\right)\hfill \\ T:\hfill & U_3\left(\beta ,\theta ,\varphi \right)=U_1\left(-\beta +\pi ,\theta ,\varphi \right)=S_1\left(\theta ,\varphi \right)\left(-\mathrm{s}\mathrm{i}\mathrm{n}\left(\beta /2\right)-\mathrm{c}\mathrm{o}\mathrm{s}\left(\beta /2\right){\sigma }_3\right)\hfill \\ PT:\hfill & U_4\left(\beta ,\theta ,\varphi \right)=U_1\left(+\beta +\pi ,\theta +\pi ,\varphi \right)=S_2\left(\theta ,\varphi \right)\left(-\mathrm{s}\mathrm{i}\mathrm{n}\left(\beta /2\right)+\mathrm{c}\mathrm{o}\mathrm{s}\left(\beta /2\right){\sigma }_3\right)\hfill \end{array}$$

(16)

With $U_{\mathrm{j}}{\tilde{U}}_{\mathrm{j}}=\cos \left(\beta \right)\left\{+1,+1,-1,-1\right\}$. Similarly, changes in $V_1\left(\beta ,\theta ,\varphi \right)$ generate the full set of Euclidean spinors $\left\{V_{\mathrm{j}}\right\}$:

$$\begin{array}{cc}I:\hfill & V_1\left(\beta ,\theta ,\varphi \right)=V_1\left(+\beta ,\theta ,\varphi \right)=S_1\left(\theta ,\varphi \right)\left(+\mathrm{c}\mathrm{o}\mathrm{s}\left(\beta /2\right)+\mathrm{s}\mathrm{i}\mathrm{n}\left(\beta /2\right){\gamma }_3\right)\hfill \\ P:\hfill & V_2\left(\beta ,\theta ,\varphi \right)=V_1\left(-\beta ,\theta +\pi ,\varphi \right)=S_2\left(\theta ,\varphi \right)\left(+\mathrm{c}\mathrm{o}\mathrm{s}\left(\beta /2\right)-\mathrm{s}\mathrm{i}\mathrm{n}\left(\beta /2\right){\gamma }_3\right)\hfill \\ T:\hfill & V_3\left(\beta ,\theta ,\varphi \right)=V_1\left(-\beta +\pi ,\theta ,\varphi \right)=S_1\left(\theta ,\varphi \right)\left(-\mathrm{s}\mathrm{i}\mathrm{n}\left(\beta /2\right)-\mathrm{c}\mathrm{o}\mathrm{s}\left(\beta /2\right){\gamma }_3\right)\hfill \\ PT:\hfill & V_4\left(\beta ,\theta ,\varphi \right)=V_1\left(+\beta +\pi ,\theta +\pi ,\varphi \right)=S_2\left(\theta ,\varphi \right)\left(-\mathrm{s}\mathrm{i}\mathrm{n}\left(\beta /2\right)+\mathrm{c}\mathrm{o}\mathrm{s}\left(\beta /2\right){\gamma }_3\right)\hfill \end{array}$$

(17)

With $V_{\mathrm{j}}{V}_j^{-1}=\left\{+1,+1,+1,+1\right\}$. Note the algebraic closure: each of the spinors $U_{\mathrm{j}}$ and $V_{\mathrm{j}}$ can be a basis to generate the full set of transformations. The spatial spinors $\left\{S_1,S_2\right\}$ in $U_{\mathrm{j}}$ and $V_{\mathrm{j}}$ are generated from spatial spinor $S_1$ (Figure 2a) via a parity transformation:

$$P: {S_1\left(\theta +\pi ,\varphi \right)=S}_2\left(\theta ,\varphi \right), S_k{\tilde{S}}_i={\delta }_{ki}$$

(18)

This orthonormal set $\left\{S_k\right\}$ corresponds to the spatial Pauli spinors [32].

Each set $\left\{U_{\mathrm{j}}\right\}$ and $\left\{V_{\mathrm{j}}\right\}$ forms an orthonormal basis within its respective metric, and the discrete transformations remain continuously connected to the identity. The components of both sets are identical, differing only in their temporal bivector plane: ${\sigma }_3={\gamma }_3{\gamma }_0$ in the Minkowski domain versus ${\gamma }_3={\sigma }_3{\gamma }_0$ in the Euclidean domain.

5.3. Example: Continuous Time-Reversal in Hyper-Spacetime

The importance of representing the full Lorentz group becomes evident when considering time-reversal $T$. In the conventional formulation, $T$ is an isolated discrete reflection that cannot be reached continuously from the identity transformation. In hyper-spacetime, however, time-reversal corresponds to a smooth angular shift in the bounded parameter $\beta$:

$$T: \left(\beta ,\theta ,\varphi \right) \mapsto \left(-\beta +\pi ,\theta ,\varphi \right).$$

As $\beta$ varies continuously, a boost can pass smoothly through the lightlike boundary and change temporal orientation without algebraic discontinuity. The boosted vector

$$p\left(\beta \right)=\sec \left(\beta \right){\gamma }_0+\tan \left(\beta \right)e_3,$$

thus evolves continuously into its time-reversed counterpart. This example illustrates why the full Lorentz group $O\left(\mathrm{1,3}\right)$, —including the discrete reflections $P$, $T$, and $PT$ —must be treated on equal geometric footing. These symmetries are essential in relativistic physics (e.g., CPT invariance [31,33,34]), and incorporating them continuously removes the traditional separation between boosts, rotations, and reflections. Hyper-spacetime provides this unified representation within a single angular domain.

• In summary, hyper-spacetime provides:

• A smooth, closed, continuous angular domain for the full Lorentz group $O\left(\mathrm{1,3}\right)$.
• Discrete reflections $\left\{P,T,PT\right\}$, continuously connected to identity.
• Spinor sets $\left\{U_{\mathrm{j}}, V_j\right\}$ forming orthonormal bases in their respective metrics, unifying the Euclidean domain ${\mathbb{R}}^4$ with the Minkowski domain ${\mathbb{R}}^{\mathrm{1,3}}$.
• A closed realization of the double cover $\mathrm{P}\mathrm{i}\mathrm{n}\left(\mathrm{1,3}\right)$ through the spinor sets $\left\{U_{\mathrm{j}}, V_j\right\}$.
• Isolation of infinities at the lightlike boundaries $\beta =\pm \pi /2$ into the scalar density factor $\sqrt{\sec \left(\beta \right)}$ (Equation (11)), while the spinors themselves remain regular.

This prepares the ground for Section 6, where the eigen-spinor and eigenvalue structure of physical observables in hyper-spacetime is developed.

6. Eigen-Spinors and Eigenvalues in the Geometry of Hyper-Spacetime

Analogous to how the observables of $\mathrm{O}\left(2\right)$ lie on the surface of one-sphere ${\mathbb{S}}^1$, the observables of hyper-spacetime reside on the surfaces of the three-spheres $\left\{{\mathbb{S}}_H^3,{\mathbb{S}}_C^3,{\mathbb{S}}^3\right\}$, each preserved by the spinor sets $\left\{U_{\mathrm{j}},V_{\mathrm{j}}\right\}$. These spinor sets act not only as symmetry generators, but also as eigen-spinors of the corresponding observables $\left\{p,q,u_r\right\}$ (Equation (12)). This follows directly from the geometric algebra eigen-spinor eigenvalue relation (Appendix D):

$$𝒪{\mathsf{\Omega }}_k={\lambda }_k{\mathsf{\Omega }}_k{e}_1 \mapsto 𝒪={\displaystyle \frac{{\lambda }_k}{{\mathsf{\Omega }}_k{\tilde{\mathsf{\Omega }}}_k}}{\mathsf{\Omega }}_k{e}_1{\tilde{\mathsf{\Omega }}}_k, {\displaystyle \frac{{\lambda }_k}{{\mathsf{\Omega }}_k{\tilde{\mathsf{\Omega }}}_k}}\in \mathbb{R}$$

(19)

Here, $𝒪$ is an observable, $e_1$ is a basis vector (reference observable, e.g., ${\gamma }_0,{\sigma }_3, \mathrm{o}\mathrm{r} {\gamma }_3$), ${\mathsf{\Omega }}_k$ are the eigen-spinors of $𝒪$, and ${\lambda }_k$ the corresponding eigenvalues. In hyper-spacetime, however, the spinor sets $\left\{U_{\mathrm{j}},V_{\mathrm{j}}\right\}$ are generated geometrically by variations in the hyper-spherical coordinates $\left(\beta ,\theta ,\varphi \right)$ (Equation (15)), rather than being obtained by solving an eigen-spinor eigenvalue equation explicitly (Appendix D).

6.1. Spatial Eigen-Spinors

The spatial spinor set $\left\{S_k\right\}$ (Equation (18)), generated from a parity transformation, act as eigen-spinors of the spatial unit vectors $\left\{e_3\in {\mathbb{S}}_{\mathrm{0,2}}^2\right\}\subset {\mathbb{R}}^{\mathrm{1,3}}$ (Figure 2a) and $\left\{u_3\in {\mathbb{S}}^2\right\}\subset {\mathbb{R}}^4$ (Equation (10)). They satisfy the GA eigen-spinor eigenvalue relations (Appendix D):

$$\begin{array}{cc}{e}_3\in {\mathbb{S}}_{\mathrm{0,2}}^2{ \mapsto e}_3{S}_k={\lambda }_k{S}_k{\gamma }_3,\hfill & {\lambda }_k\in \left\{\pm 1\right\}\hfill \\ {u_3\in {\mathbb{S}}^2 \mapsto u}_3{S}_k={\lambda }_k{S}_k{\sigma }_3,\hfill & {\lambda }_k\in \left\{\pm 1\right\}\hfill \end{array}$$

(20)

So, $e_3$ and $u_3$ are observables with eigen-spinors $S_k$ and eigenvalues ${\lambda }_k=\pm 1$. Physically, these correspond to spin-up or spin-down measurements along the spatial directions of $u_3\left(\theta ,\varphi \right)$ and $e_3\left(\theta ,\varphi \right)$.

6.2. Spacetime Eigen-Spinors

The spacetime spinor set $\left\{U_{\mathrm{j}}\right\}$ (Equation (16)) and Euclidean spinor set $\left\{V_j\right\}$ (Equation (17)) act as eigen-spinors of the hyper-spacetime observables $\left\{p,q,u_r\right\}$ (Equation (12)):

$$\begin{array}{cc}p\in {\mathbb{S}}_H^3 \mapsto p{U}_j={\eta }_j{U}_j{\gamma }_0,\hfill & {\eta }_j\in \left\{+1,+1,-1,-1\right\}\hfill \\ q\in {\mathbb{S}}_C^3 \mapsto q{U}_j={\kappa }_j{U}_j{\gamma }_0,\hfill & {\kappa }_j\in \cos \left(\beta \right)\left\{+1,+1,-1,-1\right\}\hfill \\ u_r\in {\mathbb{S}}^3 \mapsto u_r{V}_j={\eta }_j{V}_j{\gamma }_0,\hfill & {\eta }_j\in \left\{+1,+1,-1,-1\right\}\hfill \end{array}$$

(21)

Here, the eigenvalues ${\eta }_j$ encodes two constant spin states combined with positive/negative temporal orientation in ${\mathbb{S}}_H^3$ and ${\mathbb{S}}^3$, while the eigenvalues ${\kappa }_j$ encodes two variable $\left(\pm \cos \left(\beta \right)\right)$ spin states combined with positive/negative temporal orientation in ${\mathbb{S}}_c^3$. Unlike ${\eta }_j$, the values of ${\kappa }_j$ depend on relative speed via angle $\beta$ (Equation (5)). Hence, a spin state in ${\mathbb{S}}_C^3$ vanishes at the lightlike boundaries $\beta =\pm \pi /2$.

6.3. Null Spinors

At the lightlike boundaries $\beta =\pm \pi /2$ ($v=\pm c$), the spacetime spinors $U_{\mathrm{j}}$ reduce to null spinors:

$$U_{\mathrm{j}}\left(\beta ,\theta ,\varphi \right)=S_{\mathrm{k}}\left(\theta ,\varphi \right)L_{u\mathrm{j}}\left(\beta \right) \mapsto U_{\mathrm{j}}\left(\pm {\displaystyle \frac{\pi }{2}},\theta ,\varphi \right)={\displaystyle \frac{1}{\sqrt{2}}}{S}_{\mathrm{k}}\left(\theta ,\varphi \right)\left(\pm 1\pm {\sigma }_3\right), U_{\mathrm{j}}{\tilde{U}}_{\mathrm{j}}=0$$

(22)

These spinors have zero intensity but preserve direction, lying on the light cone of ${\mathbb{S}}_C^3$ and ${\mathbb{S}}_H^3$. For the Euclidean spinors $V_j$, the corresponding boundary form is

$$V_{\mathrm{j}}\left(\beta ,\theta ,\varphi \right)=S_{\mathrm{k}}\left(\theta ,\varphi \right)L_{\mathrm{v}\mathrm{j}}\left(\beta \right) \mapsto V_{\mathrm{j}}\left(\pm {\displaystyle \frac{\pi }{2}},\theta ,\varphi \right)={\displaystyle \frac{1}{\sqrt{2}}}{S}_{\mathrm{k}}\left(\theta ,\varphi \right)\left(\pm 1\pm {\gamma }_3\right), V_{\mathrm{j}}{V}_1^{-1}=1$$

(23)

Thus, the Euclidean spinors $V_{\mathrm{j}}$ keep their unit intensity, while the intensities of spacetime spinors $U_{\mathrm{j}}$ become zero. Each spinor set pass smoothly through the lightlike boundary.

6.4. Correspondence with the Dirac Equation

The eigen-spinors $U_{\mathrm{j}}$ (Equation (21)) and eigenvalues ${\eta }_j$ of the observable $p\in {\mathbb{S}}_H^3$ reproduce those of the Dirac equation [23] (two spin states combined with positive/negative temporal orientation, i.e., matter/antimatter) (Appendix E). This agreement is remarkable because in hyper-spacetime these eigen-spinors are generated geometrically (Equation (16)), rather than being obtained by solving an eigen-spinor eigenvalue equation (Appendix D). This establishes a direct geometric origin for the Dirac spectrum, demonstrating that the fundamental structure of spacetime eigen-spinors emerges naturally within the hyper-spacetime framework.

In summary, the eigen-spinor structure of hyper-spacetime reproduces the Dirac spectrum, isolates singularities into a scalar density, and reveals null spinors as natural lightlike states.

7. Discussion

The hyper-spacetime framework developed in this paper provides a compact, continuous, and geometrically transparent representation of Lorentz symmetry. By replacing the unbounded rapidity $\phi$ with the bounded angular coordinate $\beta$, the structure of Lorentz boosts is reformulated in a closed domain in which both branches of the hyperbola, as well as the lightlike boundary, appear as regular geometric features. This compact parametrization enables boosts, rotations, and reflections to be expressed within a unified angular system, thereby revealing structural parallels between hyperbolic and circular symmetries that are hidden in the conventional rapidity formalism.

A central outcome is the introduction of a triplet of three-spheres (Figure 2 and Figure 3)

$$ℬ=\left\{{\mathbb{S}}_H^3,{\mathbb{S}}_c^3,{\mathbb{S}}^3\right\},$$

which encode hyperbolic, causal, and Euclidean structure within a shared geometric framework. The three-spheres possess a common temporal axis and a reciprocal temporal bivector plane, providing a continuous geometric bridge between Minkowski and Euclidean domains (Equation (10)). This real-domain duality constitutes an alternative to analytic continuation and offers a natural geometric basis for Wick-type transformations [8,9], in which transitions between signatures correspond to smooth variations in the bounded angle $\beta$.

The unified geometry also clarifies the status of discrete symmetries. In the conventional Lorentz group, $\{P,T,PT\}$ appear as isolated, algebraically imposed reflections. Here, they arise instead as continuous angular operations within the compact domain of hyper-spherical coordinates $(\beta ,\theta ,\varphi )$: shifts of $\beta$ and $\theta$ encode changes in temporal or spatial orientation. This continuity removes the algebraic disconnection between discrete and continuous transformations and provides a closed and unified representation of the full Lorentz group $O\left(\mathrm{1,3}\right)$.

Spinor structure plays a central role in this unification. By treating spinors as geometric entities generated directly from variations in the hyper-spherical coordinates $(\beta ,\theta ,\varphi )$ (Equation (15)), the spinor sets $\left\{U_j\right\}$ and $\left\{V_j\right\}$ (Equations (16) and (17)) act both as symmetry generators and as eigen-spinors of geometric observables $\{p,q,u_r\}$. Remarkably, their eigenvalue structure reproduces the Dirac spectrum: two spin states combined with positive and negative temporal orientation, with null spinors emerging naturally at the lightlike boundary. In this formulation, Dirac spinors arise not from solving the Dirac differential equation but from the intrinsic geometry of hyper-spacetime.

A brief physical example illustrates this geometry in practice: the hyperbolic three-sphere ${\mathbb{S}}_H^3$ parametrizes normalized relativistic momentum in bounded form, while the causal sphere ${\mathbb{S}}_c^3$ simultaneously parametrizes normalized spacetime intervals (Appendix E). Their geometric product yields relativistic action, and the compact angular domain provides a clean representation of lightlike limits, where the action reduces to a null-spinor configuration. This highlights how the framework can be used to reformulate standard relativistic quantities in a bounded, continuous setting.

Finally, to place the work in its broader context [35,36], conventional treatments of Lorentz symmetry [37] are typically based on Lie-algebraic parametrizations [38], rapidity methods, or complex-analytic Wick rotations [8,10]. More recent studies examine compactifications or alternative parametrizations, but these typically apply only to restricted subgroups (e.g., $S{O}^{+}\left(\mathrm{1,3}\right)$) or require analytic continuation to imaginary time [39,40,41]. In contrast, hyper-spacetime combines compactification, spinor unification, and Euclidean–Minkowski duality within a single four-dimensional real geometric construction.

8. Conclusions

This paper introduces a unified geometric framework—hyper-spacetime—that provides a bounded, continuous representation of the full Lorentz group. By replacing rapidity with a bounded angular parameter $\beta$, the framework unifies circular and hyperbolic symmetry, eliminates divergences at the lightlike boundary, and reveals a continuous pathway through both branches of the Lorentz boost hyperbola. This compact domain enables discrete symmetries $\{P,T,PT\}$ to be expressed as smooth angular transformations, providing a closed geometric picture of $O\left(\mathrm{1,3}\right)$.

The construction of a triplet of three-spheres $\left\{{\mathbb{S}}_H^3,{\mathbb{S}}_c^3,{\mathbb{S}}^3\right\}$ forms the core of hyper-spacetime. These spheres share a temporal axis and a reciprocal temporal bivector plane, establishing a real geometric duality between Minkowski and Euclidean representations. This duality offers a natural geometric interpretation of Wick rotation and clarifies how Euclidean and Lorentzian structures can be embedded within a single continuous geometry.

The associated spinor sets $\left\{U_j\right\}$ and $\left\{V_j\right\}$ (Equations (16) and (17)) reproduce the eigen-spinor structure of the Dirac equation, including null spinors at the lightlike boundary. In this sense, hyper-spacetime provides a geometric origin for Dirac spinors, where eigen-spinor behavior emerges directly from the geometry rather than from analytic solutions of a differential equation. Singularities are isolated in scalar density factors, allowing the spinors themselves to remain regular throughout the full angular domain.

Overall, the hyper-spacetime framework yields a closed and unified representation of Lorentz geometry, clarifies the role of discrete symmetries, and provides a continuous real-domain connection between Euclidean and Minkowski structures. Beyond its conceptual clarity, the framework suggests potential applications to geometric quantization, path-integral formulations, and the study of null-spinor behavior at the lightlike boundary. Future work may explore these directions, as well as the possibility of embedding interactions or gauge structures within the same compact geometric setting.