2,822 research outputs found
Effective dynamics of the hybrid quantization of the Gowdy T^3 universe
The quantum dynamics of the linearly polarized Gowdy T^3 model (compact
inhomogeneous universes admitting linearly polarized gravitational waves) is
analyzed within Loop Quantum Cosmology by means of an effective dynamics. The
analysis, performed via analytical and numerical methods, proves that the
behavior found in the evolution of vacuum (homogeneous) Bianchi I universes is
preserved qualitatively also in the presence of inhomogeneities. More
precisely, the initial singularity is replaced by a big bounce which joins
deterministically two large classical universes. In addition, we show that the
size of the universe at the bounce is at least of the same order of magnitude
(roughly speaking) as the size of the corresponding homogeneous universe
obtained in the absence of gravitational waves. In particular, a precise lower
bound for the ratio of these two sizes is found. Finally, the comparison of the
amplitudes of the gravitational wave modes in the distant future and past shows
that, statistically (i.e., for large samples of universes), the difference in
amplitude is enhanced for nearly homogeneous universes, whereas this difference
vanishes in inhomogeneity dominated cases. The presented analysis constitutes
the first systematic effective study of an inhomogeneous system within Loop
Quantum Cosmology, and it proves the robustness of the results obtained for
homogeneous cosmologies in this context.Comment: 21 pages, 11 figures, RevTex4-1 + BibTe
Physical evolution in Loop Quantum Cosmology: The example of vacuum Bianchi I
We use the vacuum Bianchi I model as an example to investigate the concept of
physical evolution in Loop Quantum Cosmology (LQC) in the absence of the
massless scalar field which has been used so far in the literature as an
internal time. In order to retrieve the system dynamics when no such a suitable
clock field is present, we explore different constructions of families of
unitarily related partial observables. These observables are parameterized,
respectively, by: (i) one of the components of the densitized triad, and (ii)
its conjugate momentum; each of them playing the role of an evolution
parameter. Exploiting the properties of the considered example, we investigate
in detail the domains of applicability of each construction. In both cases the
observables possess a neat physical interpretation only in an approximate
sense. However, whereas in case (i) such interpretation is reasonably accurate
only for a portion of the evolution of the universe, in case (ii) it remains so
during all the evolution (at least in the physically interesting cases). The
constructed families of observables are next used to describe the evolution of
the Bianchi I universe. The performed analysis confirms the robustness of the
bounces, also in absence of matter fields, as well as the preservation of the
semiclassicality through them. The concept of evolution studied here and the
presented construction of observables are applicable to a wide class of models
in LQC, including quantizations of the Bianchi I model obtained with other
prescriptions for the improved dynamics.Comment: RevTex4, 22 pages, 4 figure
Anti-deSitter universe dynamics in LQC
A model for a flat isotropic universe with a negative cosmological constant
and a massless scalar field as sole matter content is studied within
the framework of Loop Quantum Cosmology. By application of the methods
introduced for the model with , the physical Hilbert space and the
set of Dirac observables are constructed. As in that case, the scalar field
plays here the role of an emergent time. The properties of the system are found
to be similar to those of the FRW model: for small energy densities, the
quantum dynamics reproduces the classical one, whereas, due to modifications at
near-Planckian densities, the big bang and big crunch singularities are
replaced by a quantum bounce connecting deterministically the large
semiclassical epochs. Thus in Loop Quantum Cosmology the evolution is
qualitatively cyclic.Comment: Revtex4, 29 pages, 20 figures, typos correcte
Extremal Isolated Horizons: A Local Uniqueness Theorem
We derive all the axi-symmetric, vacuum and electrovac extremal isolated
horizons. It turns out that for every horizon in this class, the induced metric
tensor, the rotation 1-form potential and the pullback of the electromagnetic
field necessarily coincide with those induced by the monopolar, extremal
Kerr-Newman solution on the event horizon. We also discuss the general case of
a symmetric, extremal isolated horizon. In particular, we analyze the case of a
two-dimensional symmetry group generated by two null vector fields. Its
relevance to the classification of all the symmetric isolated horizons,
including the non-extremal once, is explained.Comment: 22 pages, page size changed, typos and equations (142), (143a)
corrected, PACS number adde
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