文档介绍：Feynman-Weinberg Quantum Gravity and the Extended
Standard Model as a Theory of Everything
F. J. Tipler
Department of Mathematics and Department of Physics,
Tulane University, New Orleans, LA 70118
(Dated: February 3, 2008)
Abstract
I argue that the (extended) Standard Model (SM) of particle physics and the renormalizable
Feynman-Weinberg theory of quantum prise a theory of everything. I show that im-
posing 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 per-
turbation 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.
arXiv: [hep-th] 24 Apr 2007
KEY WORDS: Axiom of Choice, Axiom of Constructibility, Power Set Axiom, Large Cardinal
Axioms, Continuum Hypothesis, Generalized Continuum Hypothesis, dark matter, dark energy,
cosmological constant, flatness problem, isotropy problem, horizon problem, Harrison-Zel’dovich
spectrum, quantum cosmology, UHE cosmic rays, varying constants, curvature singularities, singu-
larity h