Feynman-Weinberg Quantum Gravity and the Extended Standard Model as a Theory of Everything

Abstract

I argue that the (extended) Standard Model (SM) of particle physics and the renormalizable Feynman-Weinberg theory of quantum gravity comprise a theory of everything. I show that imposing the appropriate cosmological boundary conditions make the theory finite. The infinities that are normally renormalized away and the series divergence infinities are both eliminated by the same mechanism. Furthermore, this theory can resolve the horizon, flatness, and isotropy problems of cosmology. Joint mathematical consistency naturally yields a scale-free, Gaussian, adiabatic perturbation spectrum, and more matter than antimatter. I show that mathematical consistency of the theory requires the universe to begin at an initial singularity with a pure $SU(2{)}_L$ gauge field. I show that quantum mechanics requires this field to have a Planckian spectrum whatever its temperature. If this field has managed to survive thermalization to the present day, then it would be the CMBR. If so, then we would have a natural explanation for the dark matter and the dark energy. I show that isotropic ultrahigh energy (UHE) cosmic rays are explained if the CMBR is a pure $SU(2{)}_L$ gauge field. The $SU(2{)}_L$ nature of the CMBR may have been seen in the Sunyaev-Zel'dovich effect. I propose several simple experiments to test the hypothesis.

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Cited by in corpus (13)

• The Mathematical Universe
• The Quantum State Of The Universe From Deformation Quantization and Classical-Quantum Correlation
• Theoretical and Observational Implications of Planck's Constant as a Running Fine Structure Constant
• The Fully Covariant Energy Momentum Stress Tensor For Gravity and the Einstein Equation in General Relativity
• General Relativity As an Aether Theory
• An observer principle for general relativity
• Many-Worlds Quantum Mechanics is Neither Mathematically Nor Experimentally Equivalent to Standard Quantum Mechanics
• The Day the Universes Interacted: Quantum Cosmology without a Wave function
• Hamilton-Jacobi Many-Worlds Theory and the Heisenberg Uncertainty Principle
• Northern Hemisphere UHECR data further supports CMBR photons with weak U(1) component
• Identifying the Unidentified Auger UHE Cosmic Rays with the Help of the Standard Model of Particle Physics
• The Jacobi Curvature Operator in Semi Riemannian Geometry and the Energy Momentum Stress Tensor of the Gravitational Field
• Taking Cognition Seriously: A generalised physics of cognition