310 research outputs found
Normal Modes and No Zero Mode Theorem of Scalar Fields in BTZ Black Hole Spacetime
Eigenfunctions for normal modes of scalar fields in BTZ black hole spacetime
are studied. Orthonormal relations among them are derived. Quantization for
scalar fields is done and particle number, energy and angular momentum are
expressed by the creation and annihilation operators. Allowed physical normal
mode region is studied on the basis of the no zero mode theorem. Its
implication to the statistical mechanics is also studied.Comment: 11 pages,v2 typos correcte
Canonical Theory of 2+1 Gravity
Recently 2+1 dimensional gravity theory, especially has been
studied extensively. It was shown to be equivalent to the 2+1 Chern-Simon
theory and has been investigated to understand the black hole thermodynamics,
i.e. Hawking temperature and others. The purpose of this report is to
investigate the canonical formalism of the original 2+1 Einstein gravity theory
instead of the Chern-Simon theory. For the spherically symmetric space-time,
local conserved quantities(local mass and angular momentum) are introduced and
using them canonical quantum theory is defined. Constraints are imposed on
state vectors and solved analytically. The strategy to obtain the solution is
followed by our previous work.Comment: 6 pages, talk given at LLWI-2000: From Particles to Universe,
Alberta, 20-26 February 200
de Broglie-Bohm Interpretatin for Analytic Solutions of The Wheeler-DeWitt Equation in Spherically Symmetric Space-time
We discuss the implications of a wave function for quantum gravity, which
involves nothing but 3-dimensional geometries as arguments and is invariant
under general coordinate transformations. We derive an analytic wave function
from the Wheeler-DeWitt equation for spherically symmetric space-time with the
coordinate system arbitrary. The de Broglie-Bohm interpretation of quantum
mechanics is applied to the wave function. In this interpretation,
deterministic dynamics can be yielded from a wave function in fully quantum
regions as well as in semiclassical ones. By introducing a coordinate system
additionally, we obtain a cosmological black hole picture in compensation for
the loss of general covariance. Our analysis shows that the de Broglie-Bohm
interpretation gives quantum gravity an appropriate prescription to introduce
coordinate systems naturally and extract information from a wave function as a
result of breaking general covariance.Comment: 14 pages, REVTeX; abstract and content revise
Rotation Curves of Spiral Galaxies and Large Scale Structure of Universe under Generalized Einstein Action
We consider an addition of the term which is a square of the scalar curvature
to the Einstein-Hilbert action. Under this generalized action, we attempt to
explain i) the flat rotation curves observed in spiral galaxies, which is
usually attributed to the existence of dark matter, and ii) the contradicting
observations of uniform cosmic microwave background and non-uniform galaxy
distributions against redshift. For the former, we attain the flatness of
velocities, although the magnitudes remain about half of the observations. For
the latter, we obtain a solution with oscillating Hubble parameter under
uniform mass distributions. This solution leads to several peaks of galaxy
number counts as a function of redshift with the first peak corresponding to
the Great Wall.Comment: 16 page
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