472 research outputs found
DocuDrama
This paper presents an approach combining concepts of virtual storytelling with cooperative processes. We will describe why storytelling is relevant in cooperation support applications. We will outline how storytelling concepts provide a new quality for groupware applications. Different prototypes illustrate a combination of a groupware application with various storytelling components in a Theatre of Work
Spectrum from the warped compactifications with the de Sitter universe
We discuss the spectrum of the tensor metric perturbations and the stability
of warped compactifications with the de Sitter spacetime in the
higher-dimensional gravity. The spacetime structure is given in terms of the
warped product of the non-compact direction, the spherical internal dimensions
and the four-dimensional de Sitter spacetime. To realize a finite bulk volume,
we construct the brane world model, using the cut-copy-paste method. Then, we
compactify the spherical directions on the brane. In any case, we show the
existence of the massless zero mode and the mass gap of it with massive
Kaluza-Klein modes. Although the brane involves the spherical dimensions, no
light massive mode is excited. We also investigate the scalar perturbations,
and show that the model is unstable due to the existence of a tachyonic bound
state, which seems to have the universal negative mass square, irrespective of
the number of spacetime dimensions.Comment: Journal version (JHEP
Symbolic Activities in Virtual Spaces
This paper presents an approach to combine concepts ofsymbolic acting and virtual storytelling with the support ofcooperative processes. We will motivate why symboliclanguages are relevant in the social context of awarenessapplications. We will describe different symbolicpresentations and illustrate their application in three differentprototypes
High-energy effective theory for matter on close Randall Sundrum branes
Extending the analysis of hep-th/0504128, we obtain a formal expression for
the coupling between brane matter and the radion in a Randall-Sundrum
braneworld. This effective theory is correct to all orders in derivatives of
the radion in the limit of small brane separation, and, in particular, contains
no higher than second derivatives. In the case of cosmological symmetry the
theory can be obtained in closed form and reproduces the five-dimensional
behaviour. Perturbations in the tensor and scalar sectors are then studied.
When the branes are moving, the effective Newtonian constant on the brane is
shown to depend both on the distance between the branes and on their velocity.
In the small distance limit, we compute the exact dependence between the
four-dimensional and the five-dimensional Newtonian constants.Comment: Updated version as published in PR
Black String Perturbations in RS1 Model
We present a general formalism for black string perturbations in
Randall-Sundrum 1 model (RS1). First, we derive the master equation for the
electric part of the Weyl tensor . Solving the master equation
using the gradient expansion method, we give the effective Teukolsky equation
on the brane at low energy. It is useful to estimate gravitational waves
emitted by perturbed rotating black strings. We also argue the effect of the
Gregory-Laflamme instability on the brane using our formalism.Comment: 14 pages, Based on a talk presented at ACRGR4, the 4th Australasian
Conference on General Relativity and Gravitation, Monash University,
Melbourne, January 2004. To appear in the proceedings, in General Relativity
and Gravitatio
Gravity, Stability and Energy Conservation on the Randall-Sundrum Brane-World
We carefully investigate the gravitational perturbation of the
Randall-Sundrum (RS) single brane-world solution [hep-th/9906064], based on a
covariant curvature tensor formalism recently developed by us. Using this
curvature formalism, it is known that the `electric' part of the 5-dimensional
Weyl tensor, denoted by , gives the leading order correction to the
conventional Einstein equations on the brane. We consider the general solution
of the perturbation equations for the 5-dimensional Weyl tensor caused by the
matter fluctuations on the brane. By analyzing its asymptotic behaviour in the
direction of the 5th dimension, we find the curvature invariant diverges as we
approach the Cauchy horizon. However, in the limit of asymptotic future in the
vicinity of the Cauchy horizon, the curvature invariant falls off fast enough
to render the divergence harmless to the brane-world. We also obtain the
asymptotic behavior of on the brane at spatial infinity, assuming
the matter perturbation is localized. We find it falls off sufficiently fast
and will not affect the conserved quantities at spatial infinity. This
indicates strongly that the usual conservation law, such as the ADM energy
conservation, holds on the brane as far as asymptotically flat spacetimes are
concerned.Comment: 10 pages, references adde
Effective theory for close limit of two branes
We discuss the effective theory for the close limit of two branes in a
covariant way. To do so we solve the five dimensional Einstein equation along
the direction of the extra dimension. Using the Taylor expansion we solve the
bulk spacetimes and derive the effective theory describing the close limit. We
also discuss the radion dynamics and braneworld black holes for the close limit
in our formulation.Comment: 6 pages, a version to be published in Phy.Rev.
Scalar perturbations from brane-world inflation
We investigate the scalar metric perturbations about a de Sitter brane
universe in a 5-dimensional anti de Sitter bulk. We compare the master-variable
formalism, describing metric perturbations in a 5-dimensional longitudinal
gauge, with results in a Gaussian normal gauge. For a vacuum brane (with
constant brane tension) there is a continuum of normalizable Kaluza-Klein
modes, with m>3H/2, which remain in the vacuum state. A light radion mode, with
m=\sqrt{2}H, satisfies the boundary conditions for two branes but is not
normalizable in the single-brane case. When matter is introduced (as a test
field) on the brane, this mode, together with the zero-mode and an infinite
ladder of discrete tachyonic modes, become normalizable. However, the boundary
condition requires the self-consistent 4-dimensional evolution of scalar field
perturbations on the brane and the dangerous growing modes are not excited.
These normalizable discrete modes introduce corrections at first-order to the
scalar field perturbations computed in a slow-roll expansion. On super-Hubble
scales, the correction is smaller than slow-roll corrections to the de Sitter
background. However on small scales the corrections can become significant.Comment: 15 page
Ballistic and diffuse transport through a ferromagnetic domain wall
We study transport through ballistic and diffuse ferromagnetic domain walls
in a two-band Stoner model with a rotating magnetization direction. For a
ballistic domain wall, the change in the conductance due to the domain wall
scattering is obtained from an adiabatic approximation valid when the length of
the domain wall is much longer than the Fermi wavelength. In diffuse systems,
the change in the resistivity is calculated using a diagrammatic technique to
the lowest order in the domain wall scattering and taking into account
spin-dependent scattering lifetimes and screening of the domain wall potential.Comment: 9 pages, 3 figures, to appear in Phys. Rev.
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