Macroscopically-Discrete Quantum Cosmology

نویسنده

  • Geoffrey F. Chew
چکیده

Milne’s Lorentz-group-based cosmological spacetime and Gelfand-Naimark unitary Lorentz-group representation through transformation of Hilbert-space vectors combine to define a Fock space of ‘cosmological preons’—quantum-theoretic universe constituents. Lorentz invariance of ‘age’–global time– accompanies Milne’s ‘cosmological principle’ that attributes to each spatial location a Lorentz frame. We divide Milne spacetime—the interior of a forward lightcone– into ‘slices’ of fixed macroscopic width in age, with ‘cosmological rays’ defined on (hyperbolic) slice boundaries. The Fock space of our macroscopically-discrete quantum cosmology (DQC) is defined only at these exceptional universe ages. Self-adjoint-operator expectations over the ray at any spacetime-slice boundary prescribe throughout the following slice a non-fluctuating continuous ‘classical reality’ represented by Dalembertians, of classical electromagnetic (vector) and gravitational (tensor) potentials, that are current densities of locally-conserved electric charge and energy-momentum. The ray at the upper boundary of a slice is determined from the lower-boundary ray by branched slice-traversing stepped Feynman paths that carry potential-depending action. Path step is at Planck-scale; branching points represent preon creation-annihilation. Each single-preon wave function depends on the coordinates of a 6-dimensional manifold, one of whose ‘extra’ dimensions associates in Dirac sense to a self-adjoint operator that represents the preon’s reversible local time. Within a path, local-time intervals equal corresponding intervals of monotonically-increasing global time even though, within a (fixed-age) ray, the local time of a preon is variable. The operator canonically conjugate to a preon’s local time represents its (total) energy in its (Milne) ‘local frame’. A macroscopically-stable positive-energy single-preon wave function identifies either with a Standard-Model elementary particle or with a graviton. Within intermediate-density sub-Hubble-scale universe regions such as the solar system, where ‘reproducible measurement’ is meaningful, physical special relativity—‘Poincaré invariance’—approximates DQC for spacetime scales far above that of Planck. c © Electronic Journal of Theoretical Physics. All rights reserved.

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Loop Quantum Cosmology IV: Discrete Time Evolution

Using general features of recent quantizations of the Hamiltonian constraint in loop quantum gravity and loop quantum cosmology, a dynamical interpretation of the constraint equation as evolution equation is presented. This involves a transformation from the connection to a dreibein representation and the selection of an internal time variable. Due to the discrete nature of geometrical quantiti...

متن کامل

Stability of additive functional equation on discrete quantum semigroups

We construct  a noncommutative analog of additive functional equations on discrete quantum semigroups and show that this noncommutative functional equation has Hyers-Ulam stability on amenable discrete quantum semigroups. The discrete quantum semigroups that we consider in this paper are in the sense of van Daele, and the amenability is in the sense of Bèdos-Murphy-Tuset. Our main result genera...

متن کامل

Covariant Effective Action for Loop Quantum Cosmology

In loop quantum cosmology, non-perturbative quantum gravity effects lead to the resolution of the big bang singularity by a quantum bounce without introducing any new degrees of freedom. Though fundamentally discrete, the theory admits a continuum description in terms of an effective Hamiltonian. Here we provide an algorithm to obtain the corresponding effective action, establishing in this way...

متن کامل

Semiclassical states, effective dynamics, and classical emergence in loop quantum cosmology

1550-7998=20 We construct physical semiclassical states annihilated by the Hamiltonian constraint operator in the framework of loop quantum cosmology as a method of systematically determining the regime and validity of the semiclassical limit of the quantum theory. Our results indicate that the evolution can be effectively described using continuous classical equations of motion with nonperturb...

متن کامل

Dynamical initial conditions in quantum cosmology.

Loop quantum cosmology is shown to provide both the dynamical law and initial conditions for the wave function of a universe by one discrete evolution equation. Accompanied by the condition that semiclassical behavior is obtained at large volume, a unique wave function is predicted.

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2009