Gravitation and Spacetime: Emergent from Spinor Interactions -- How?
Martin Rainer

TL;DR
This paper explores the idea that spacetime and gravity emerge from fundamental spinor interactions, comparing classical and quantum approaches, and proposing a unified view of causal structure and geometry.
Contribution
It introduces a framework where spacetime geometry and causal structure emerge from spinor interactions within a causal double cone region.
Findings
Spacetime properties are linked to underlying spinor interactions.
Emergent causal structure and spin networks arise from particle spinors.
Comparison of classical and quantum approaches highlights common foundational elements.
Abstract
Newtonian gravity arises as the nonrelativistic, static, weak-field limit of some Lorentzian spacetime geometry solving the generally covariant Einstein equations for a given matter field configuration. Spacetime geometry has a local description in the spinor basis of Penrose. The breakdown of relativistic quantum (field) theory at small distances suggests that, the Lorentzian geometry is to be modified below some regularization length. The thermodynamic correspondence, e.g. for black holes or other horizons, indicates that, Lorentzian spacetime is an emergent geometric description of an ensemble of more fundamental constituents. The independent derivations of the area law of the Bekenstein-Hawking entropy by string theory and loop quantum gravity show that, (some) properties of spacetime do not depend on the nature of its fundamental constituents (in leading order). Whether, on a…
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Taxonomy
TopicsNoncommutative and Quantum Gravity Theories · Quantum Electrodynamics and Casimir Effect · Cosmology and Gravitation Theories
