Up to now there is no definition or an example of a gauge-invariant quantum field theory in four-dimensional space-time, with mathematical rigor and in the absence of approximations. This is mainly due to three features of the theory: 1) the canonical quantization is not manifestly Lorentz invariant; 2) the Lagrangian is singular due to the gauge symmetry; and 3) the gaussian measure is not gauge invariant. At least one of these features becomes an obstacle to mathematical rigor in either the canonical or the path-integral quantization. Using the fact that there is a wave-function associated to any probability distribution, we study a class of statistical field theories in four-dimensional space-time where the (classical) canonical coo...
Abstract. Certain difficulties of quantum gravity can be avoided if we embed the spacetime V4 into a...
In curved spacetimes, the lack of criteria for the construction of a unique quantization is a fundam...
The paper is the second part of the work devoted to the problem of time in quantum cosmology. Here ...
Up to now there is no definition or an example of a gauge-invariant quantum field theory in four-dim...
Up to now there is no definition or an example of a gauge-invariant quantum field theory in four-dim...
Up to now there is no definition or an example of a gauge-invariant quantum field theory in four-dim...
Up to now there is no definition or an example of a gauge-invariant quantum field theory in four-dim...
Up to now there is no definition or an example of a gauge-invariant quantum field theory in four-dim...
Up to now there is no definition or an example of a Quantum Yang-Mills theory in four- dimensional s...
Quantum Yang-Mills theory, Classical Statistical Field Theory (for Hamiltonians which are non-polyno...
Quantum Yang-Mills theory, Classical Statistical Field Theory (for Hamiltonians which are non-polyno...
Quantum Yang-Mills theory, Classical Statistical Field Theory (for Hamiltonians which are non-polyno...
Quantum Yang-Mills theory, Classical Statistical Field Theory (for Hamiltonians which are non-polyno...
The conventional group of four-dimensional diffeomorphisms is not realizeable as a canonical transfo...
We prove that, under the standard conformal scaling, a free scalar field in de Sitter spacetime admi...
Abstract. Certain difficulties of quantum gravity can be avoided if we embed the spacetime V4 into a...
In curved spacetimes, the lack of criteria for the construction of a unique quantization is a fundam...
The paper is the second part of the work devoted to the problem of time in quantum cosmology. Here ...
Up to now there is no definition or an example of a gauge-invariant quantum field theory in four-dim...
Up to now there is no definition or an example of a gauge-invariant quantum field theory in four-dim...
Up to now there is no definition or an example of a gauge-invariant quantum field theory in four-dim...
Up to now there is no definition or an example of a gauge-invariant quantum field theory in four-dim...
Up to now there is no definition or an example of a gauge-invariant quantum field theory in four-dim...
Up to now there is no definition or an example of a Quantum Yang-Mills theory in four- dimensional s...
Quantum Yang-Mills theory, Classical Statistical Field Theory (for Hamiltonians which are non-polyno...
Quantum Yang-Mills theory, Classical Statistical Field Theory (for Hamiltonians which are non-polyno...
Quantum Yang-Mills theory, Classical Statistical Field Theory (for Hamiltonians which are non-polyno...
Quantum Yang-Mills theory, Classical Statistical Field Theory (for Hamiltonians which are non-polyno...
The conventional group of four-dimensional diffeomorphisms is not realizeable as a canonical transfo...
We prove that, under the standard conformal scaling, a free scalar field in de Sitter spacetime admi...
Abstract. Certain difficulties of quantum gravity can be avoided if we embed the spacetime V4 into a...
In curved spacetimes, the lack of criteria for the construction of a unique quantization is a fundam...
The paper is the second part of the work devoted to the problem of time in quantum cosmology. Here ...