Submitted:
03 May 2025
Posted:
06 May 2025
You are already at the latest version
Abstract
We introduce an information-geometric framework in which spacetime, gravity, and gauge kinematics naturally emerge from quantum correlations. Central to this approach is the "footballhedron," a convex geometric structure encoding the global state's correlation patterns. Observers perceive spacetime as lower-dimensional projections of this object, resulting in an emergent information-theoretic metric consistent with classical geometry. Rotations of the footballhedron correspond to Lorentz transformations, while extremizing Fisher information yields Einstein's equations and an emergent correlation-defined stress-energy tensor. A finite Coxeter tessellation of the footballhedron provides an intrinsic ultraviolet cutoff at the Planck scale and naturally generates internal gauge symmetries through its automorphisms. We propose experimental tests using spin entanglement and optomechanical setups. Explicit holographic examples, including cosmological scenarios and tensor-network models, illustrate how this unified approach coherently integrates quantum correlations, gravitational dynamics, and gauge structure in an observer-dependent geometry.
Keywords:
1. Introduction
- A minimal set of axioms explicitly linking correlation data to observer projections, grounding spacetime structure rigorously in quantum-information geometry.
- A novel ultraviolet completion via finite Coxeter tessellation of the footballhedron, providing an intrinsic regulator and yielding gauge algebra kinematics through facet-label automorphisms [8].
2. Framework
Notation and Conventions
Geometric notation
- Hilbert space of the global quantum system.
- Pure quantum-state vector in , .
- Density operator on , with and .
- Observer-defined Hermitian operators on .
- Connected two-point correlator, .
- P
- Maximum correlator order (interaction-cutoff) in the direct sum
- C
- Full correlator space, .
- Modified two-point function with cutoff profile g (see Definition 1).
- Correlationhedron of the global state :
- Uniform volume measure on , used to define push-forward densities.
- Observer-projection map , selecting the correlators accessible to .
- Jacobian (derivative) of the projection , mapping tangent spaces .
- Emergent manifold (image of under ).
- Radius and angular frequency of the hyperspherical embedding of , which together give as the invariant correlation speed.
- c
- Invariant correlation speed, .
- For a tessellation of into N patches, is the UV momentum cutoff.
- Planck length (UV scale) used in estimates like .
Information-theoretic notation
- Index conventions: Greek indices run from 1 to ; repeated indices are summed (Einstein convention).
- : Push-forward scalar density on , defined by .
- : Local information density (pointwise Fisher kernel),
- : Fisher information matrix,
- : Emergent spacetime metric,
- : Inverse emergent spacetime metric,
2.1. Foundational Axioms
- No-signaling constraints hold;
- Tsirelson-type bounds hold.
- UV regulator. Replacing the continuum by N finite cells enforces a highest momentum scaleas shown in Corollary 8, taming all short-distance divergences without any ad hoc smoothing.
- Discrete symmetry (CSCH). The facet reflections of the tessellation give precisely the Coxeter-group relations needed to derive the Cartan-Schwarz-Cartan identities and hence the emergent gauge algebra (see Section 2.8).
2.2. Geometric Foundations
2.3. Time Factorization and Entanglement–Time Duality
2.4. Emergent Lorentzian Structure
2.5. Emergent Gravitational Dynamics
- The emergence of spacetime geometry from quantum correlations follows a minimal informational principle.
- Observers’ projections constrain the correlation structure, requiring the informational measure to reflect observer-dependence explicitly.
- Compatibility with known holographic and entropic gravity scenarios to ensure physical consistency.
2.6. Horizons and Causal Boundaries
2.7. Ultraviolet Completion and Discreteness
UV Cutoff from Finite Tessellation
2.8. Gauge Symmetry from Tessellation
- Begin with the full symmetry described by the Coxeter group , the symmetry group of the 120-cell polychoron. Selecting subsets of facets invariant under the subgroup , corresponding precisely to the Weyl group of the Lie algebra , explicitly realizes the embedding:
- A further geometric refinement corresponds precisely to the Georgi-Glashow symmetry breaking:explicitly labeling or “coloring” subsets of facets according to their subgroup invariances. This yields exactly the gauge symmetry structure of the Standard Model.
2.9. Cosmological Implications
2.10. Holography and Tensor-Network Examples
3. Testable Predictions and Experimental Proposals
3.1. Spin-Entanglement Curvature Witness
- Magnetic field control: Homogeneity to suppress Zeeman broadening.
- Shot-noise limit: Phase uncertainty rad for shots.
- State fidelity: Preparation and readout fidelity to keep systematic bias below .
- Temperature stability:mK to mitigate thermal decoherence.
3.2. Optomechanical Curvature Detection
- Mechanical quality factor: to limit thermal decoherence rates to .
- Displacement sensitivity:m for phase resolution rad.
- Laser stability: Linewidth Hz to suppress phase noise above rad.
- Repetition count: cycles for statistical averaging.
Further directions
4. Conclusion
Limitations
- Gauge symmetry realization. While the Coxeter tessellation identifies the Lie algebra of emergent gauge groups, it remains to be shown how local gauge fields and their charges (gauge bosons) arise dynamically.
- Dark matter phenomenology. The interpretation of hidden correlation modes as an effective pressureless dust requires quantitative study: e.g., how do these modes influence structure formation or gravitational lensing compared to particle dark matter?
- Dark energy mechanism. A constant monopole term in the correlation density yields an effective , but its value is currently a free parameter. A microscopic mechanism to fix this offset (perhaps via global correlation constraints or boundary conditions on the footballhedron) should be developed.
- Quantum fluctuations of geometry. Our framework so far yields a classical emergent metric. To approach full quantum gravity, one must examine fluctuations in the correlator density and their impact on , potentially giving rise to graviton-like excitations.
- Domain of validity. We have restricted to finite correlator order P and assumed a smooth, structure. Near critical points or in highly quantum or nonlinear regimes, higher-order correlators may be essential and smoothness may fail.
Future Work
- Emergent gauge dynamics. Develop a concrete model for gauge boson emergence by introducing dynamics for facet variables or by constructing an effective action for correlation-constraint fluctuations.
- Cosmological and astrophysical tests. Perform N-body and lensing simulations using hidden-mode dark matter to derive observable signatures distinct from WIMP or axion models.
- Correlation-offset determination. Seek principles (e.g., symmetry, extremal entropy) that fix the constant correlation mode, thereby predicting the effective cosmological constant rather than treating it as arbitrary.
- Quantum correlator perturbations. Study small fluctuations of around classical solutions to extract a spectrum of metric perturbations and compare with graviton propagation in linearized gravity.
- Refined experimental signatures. Identify observables in spin-entanglement and optomechanical setups that distinguish this information-geometric framework from standard semiclassical gravity, for instance a nontrivial dependence of the curvature witness on the entanglement angle.
- Standard Model gauge embedding. Provide a concrete tessellation ( Coxeter cell) that yields SU(3)×SU(2)×U(1), or else clearly mark this construction as highly conjectural.
- Beyond finite P. Relax the finite-order correlator cutoff and explore emergent geometry when including higher correlators or nonperturbative correlator spectra.
- Tensor-network realizations. Pursue tensor-network simulations as a direct computational method to quantitatively validate emergent geometry predictions, particularly in critical and nonlinear correlation regimes [4].
- Numerical and simulation studies. Perform large-scale numerical simulations of hidden-mode cosmological effects to rigorously test and differentiate predictions from established dark matter and dark energy models [6].
Appendix E
Appendix E.1. Geometric Foundations
Appendix E.2. Time Factorization and Entanglement–Time Duality
Appendix E.3. Emergent Lorentzian Structure
Appendix E.4. Emergent Gravitational Dynamics
Appendix E.5. Horizons and Causal Boundaries
Appendix E.6. Ultraviolet Completion and Discreteness
Appendix E.7. Gauge Symmetry from Tessellation
Appendix E.8. Cosmological Implications
Appendix E.9. Holography and Tensor-Network Examples
References
- Ted Jacobson. Thermodynamics of spacetime: The einstein equation of state. Phys. Rev. Lett., 75:1260–1263, 1995.
- Erik Verlinde. On the origin of gravity and the laws of newton. J. High Energy Phys., 2011(4):29, 2011.
- Shun’ichi Amari. Information Geometry and Its Applications. Springer, Tokyo, Japan, 2016.
- Brian Swingle. Entanglement renormalization and holography. Phys. Rev. D, 86(6):065007, 2012.
- Luca Bombelli, Joohan Lee, David Meyer, and Rafael Sorkin. Space-time as a causal set. Phys. Rev. Lett., 59(5):521–524, 1987.
- Agostino Russo. The correlationhedron: Spacetime as projections of quantum correlations. Preprint, 2025.
- J. D. Bekenstein. Universal upper bound on the entropy-to-energy ratio for bounded systems. Phys. Rev. D, 23:287–298, 1981.
- H. S. M. Coxeter. Regular Polytopes. Dover, New York, 1973.
- Mark Van Raamsdonk. Building up spacetime with quantum entanglement. Gen. Relativ. Gravit., 42:2323–2329, 2010.
- Don N. Page and William K. Wootters. Evolution without evolution: Dynamics described by stationary observables. Phys. Rev. D, 27(12):2885–2892, 1983.
- Itamar Pitowsky. Quantum Probability—Quantum Logic. Springer, Berlin, 1991.
- B. S. Tsirelson. Quantum generalizations of bell’s inequality. Lett. Math. Phys., 4:93–100, 1980.
- K. Osterwalder and R. Schrader. Axioms for euclidean green’s functions. Commun. Math. Phys., 31(2):83–112, 1973.
- Steven Weinberg. The Quantum Theory of Fields, Volume I: Foundations. Cambridge University Press, 1995.
- Carlo Rovelli. Relational quantum mechanics. Int. J. Theor. Phys., 35(8):1637–1678, 1996.
- Shun-ichi Amari. Differential-Geometrical Methods in Statistics. Springer, 1985.
- Thomas M. Cover and Joy A. Thomas. Elements of Information Theory. Wiley, 2006.
- Juan Maldacena. The large-n limit of superconformal field theories and supergravity. Adv. Theor. Math. Phys., 2:231–252, 1998.
- Shinsei Ryu and Tadashi Takayanagi. Holographic derivation of entanglement entropy from the anti-de sitter space/conformal field theory correspondence. Phys. Rev. Lett., 96(18):181602, 2006.
- Sougato Bose, Anupam Mazumdar, Gavin W. Morley, Hendrik Ulbricht, Marko Toro, Mauro Paternostro, Andrew A. Geraci, Peter F. Barker, M. S. Kim, and Gerard Milburn. Spin entanglement witness for quantum gravity. Phys. Rev. Lett., 119(24):240401, 2017.
- Chiara Marletto and Vlatko Vedral. Gravitationally induced entanglement between two massive particles is sufficient evidence of quantum effects in gravity. Phys. Rev. Lett., 119(24):240402, 2017.
- S. W. Hawking and W. Israel, editors. General Relativity: An Einstein Centenary Survey. Cambridge University Press, Cambridge, 1979.
- G. W. Gibbons and S. W. Hawking, editors. Euclidean Quantum Gravity. World Scientific, Singapore, 1993.
| 1 | More general relational-frame constructions can be obtained when exact factorization fails. |
| 2 | This Wick rotation formally invokes the Osterwalder–Schrader axioms (reflection positivity, Euclidean invariance, symmetry, cluster decomposition) to ensure a unique analytic continuation from Euclidean correlators to Lorentzian Green’s functions [13,14]. In physically relevant examples, e.g. ground states of gapped local Hamiltonians or KMS thermal states, the Hamiltonian’s spectral gap and thermal KMS condition guarantee holomorphy in a strip around the real axis and exponential decay at large imaginary-time separations, so that the transfer matrix converges and the Wick rotation is well-defined. |

Disclaimer/Publisher’s Note: The statements, opinions and data contained in all publications are solely those of the individual author(s) and contributor(s) and not of MDPI and/or the editor(s). MDPI and/or the editor(s) disclaim responsibility for any injury to people or property resulting from any ideas, methods, instructions or products referred to in the content. |
© 2025 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (http://creativecommons.org/licenses/by/4.0/).