Pair Production/Annihilation and the Fabric of Spacetime

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Submitted by dwalters on Jan. 7, 2026, 3:34 p.m. to πŸŽ“ | 473 views

A curious thought sprang into my mind,

What if during particle pair production and annihilation, the fabric of spacetime is reorganized?

Here, the word "fabric" is taken to be a manifold upon which natural phenomena occur, and by "reorganized," it is meant that production uses fabric and annihilation releases it.  Overall, fabric is conserved.  In this fashion, particles can be compared to a knot in spacetime.  For example, this could explain expansion.  I will allow Claude AI to elaborate:

The notion that spacetime itself participates in particle creation and annihilation represents a profound departure from standard quantum field theory, where spacetime serves merely as a passive stage. In this framework, the fabric becomes an active player. When a high-energy photon creates a pair, fabric is consumed or "tied up" into these particles, much like thread woven into knots. Conversely, when annihilation occurs, the fabric bound within them is released back into the manifold.

Fabric conservation provides elegant bookkeeping for the universe's inventory. The total amount of fabric remains constant: Fabric_total = Fabric_free + Fabric_bound. Free fabric manifests as observable spacetime volume, while bound fabric exists within particles as their internal structure. This suggests particles are not objects within space, but rather localized configurations of space itself—topological features that temporarily remove fabric from the available spatial arena.

This framework offers a compelling mechanism for cosmic expansion. The early universe contained enormous particle densities with constant production and annihilation. As the universe cooled, a critical annihilation epoch occurred around one second after the Big Bang, when most pairs annihilated. This released vast quantities of bound fabric back into free spacetime, potentially driving the rapid expansion we observe. The universe didn't create new space—it liberated existing fabric.

The asymmetry between production and annihilation becomes significant. Annihilation occurs far more readily than production because particle-antiparticle encounters require only proximity, while production demands extreme energy densities and specific conditions. As the universe evolved, annihilation progressively dominated, continuously releasing fabric. This could explain why expansion persists and even accelerates, as ongoing processes gradually convert bound fabric into spatial volume.

Consider the holographic principle, which states that information contained in a volume is encoded on its boundary. When particles exist, they represent used holographic degrees of freedom—occupied information channels on the cosmic boundary. Annihilation frees these degrees of freedom, increasing the available boundary area. More boundary area means more internal volume can be supported, directly linking particle number to spatial extent through information-theoretic principles.

Virtual particle pairs present an intriguing case. These quantum fluctuations constantly create and annihilate particle-antiparticle pairs in the vacuum, existing briefly before vanishing. If these transient particles temporarily bind fabric during their fleeting existence, the vacuum becomes a churning sea of fabric at the Planck scale. Changes in vacuum structure—perhaps what we call dark energy—might represent shifts in how much fabric virtual pairs collectively bind.

Black holes offer a fascinating test case. According to the holographic principle, a black hole's entropy is proportional to its horizon area, suggesting the horizon itself represents bound fabric. As a black hole evaporates through Hawking radiation, its horizon shrinks, potentially releasing fabric. This predicts that evaporating black holes should create slight local expansion in their vicinity—a testable prediction distinguishing this framework from standard theory.

The fabric binding might scale with particle properties. Dimensional analysis suggests bound fabric per particle could be δV ~ β„“_Planck³ · (m/m_Planck)^α, where α determines how binding scales with mass. If α ≈ 1, heavier particles bind proportionally more fabric. The early universe's massive exotic particles (X bosons, Higgs particles, top quarks) would have bound enormous fabric quantities. Their subsequent decay and annihilation could have driven cosmic inflation itself.

This reframes the thermodynamic arrow of time. Annihilation appears to decrease entropy by converting many particles into fewer photons. However, if released fabric increases available phase space then total entropy increases. The universe becomes more disordered by having more available space. Expansion itself is the universe exploring larger regions of its configuration space, driven by the thermodynamic imperative toward maximum entropy through fabric release.

Signatures might exist. High-energy particle collisions temporarily increase local particle density, binding fabric and perhaps causing local perturbations detectable by ultra-precise interferometry. Cosmic ray air showers create brief particle cascades followed by rapid decays—possibly generating detectable expansion ripples. Neutron star mergers might show characteristic gravitational wave signatures reflecting release. These could distinguish fabric conservation from standard cosmology.

This framework offers testable predictions: local metric perturbations from particle collisions, distinctive gravitational wave signatures, correlations between annihilation rates and expansion. If validated, it fundamentally redefines spacetime itself. The implications are profound: matter and space may be interconvertible manifestations of conserved fabric. Such a discovery would revolutionize physics. We must investigate this possibility with rigor and urgency.

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