58 research outputs found
Wireless multimedia sensor network for plant disease detections
International audienceTo minimize pesticide use it is necessary to detect at the early stage the present of plant disease and perform local treatment instead of global systematic treatment. To achieve this goal, one of the techniques may be used is image processing through the deployment of WMSN in the cultivated field. However, transmitting massive image data wirelessly will increase significantly network traffic and particularly energy consumption. In this paper, we propose a plant disease detection approach which is designed to run on the resource-constrained WMSN nodes. Through the analysis of plant images acquired by the node, this new approach is able to make a preliminary local decision on the health condition of the plant and determine the necessity of sending back images to the control centre for further inspection, thus improving the efficiency of the monitoring network. The complete method includes image segmentation based on both color and shape, and uses 2D histogram as the feature for classification. Experiments on the plant images with nutrient deficiency symptoms show the classification accuracy of the new method reaches 87.5%
Linking the trans-Planckian and the information loss problems in black hole physics
The trans-Planckian and information loss problems are usually discussed in
the literature as separate issues concerning the nature of Hawking radiation.
Here we instead argue that they are intimately linked, and can be understood as
"two sides of the same coin" once it is accepted that general relativity is an
effective field theory.Comment: 10 pages, 2 figures. Replaced with the version to be published in
General Relativity and Gravitatio
The Covariant Entropy Bound, Brane Cosmology, and the Null Energy Condition
In discussions of Bousso's Covariant Entropy Bound, the Null Energy Condition
is always assumed, as a sufficient {\em but not necessary} condition which
helps to ensure that the entropy on any lightsheet shall necessarily be finite.
The spectacular failure of the Strong Energy Condition in cosmology has,
however, led many astrophysicists and cosmologists to consider models of dark
energy which violate {\em all} of the energy conditions, and indeed the current
data do not completely rule out such models. The NEC also has a questionable
status in brane cosmology: it is probably necessary to violate the NEC in the
bulk in order to obtain a "self-tuning" theory of the cosmological constant. In
order to investigate these proposals, we modify the Karch-Randall model by
introducing NEC-violating matter into in such a way that the brane
cosmological constant relaxes to zero. The entropy on lightsheets remains
finite. However, we still find that the spacetime is fundamentally incompatible
with the Covariant Entropy Bound machinery, in the sense that it fails the
Bousso-Randall consistency condition. We argue that holography probably forbids
all {\em cosmological} violations of the NEC, and that holography is in fact
the fundamental physical principle underlying the cosmological version of the
NEC.Comment: 21 pages, 3 figures, version 2:corrected and greatly improved
discussion of the Bousso-Randall consistency check, references added;
version3: more references added, JHEP versio
Can we live on a D-brane? -- Effective theory on a self-gravitating D-brane --
We consider a D-brane coupled with gravity in type IIB supergravity on S^5
and derive the effective theory on the D-brane in two different ways, that is,
holographic and geometrical projection methods. We find that the effective
equations on the brane obtained by these methods coincide. The theory on the
D-brane described by the Born-Infeld action is not like Einstein-Maxwell theory
in the lower order of the gradient expansion, i.e., the Maxwell field does not
appear in the theory. Thus the careful analysis and statement for cosmology on
self-gravitating D-brane should be demanded in realistic models.Comment: 13 pages, accepted for publication in Physical Review
Holographic Cosmic Quintessence on Dilatonic Brane World
Recently quintessence is proposed to explain the observation data of
supernova indicating a time-varying cosmological constant and accelerating
universe. Inspired by this and its mysterious origin, we look for the
possibility of quintessence as the holographic dark matters dominated in the
late time in the brane world scenarios. We consider both the cases of static
and moving brane in a dilaton gravity background. For the static brane we use
the Hamilton-Jacobi method motivated by holographic renormalization group to
study the intrinsic FRW cosmology on the brane and find out the constraint on
the bulk potential for the quintessence. This constraint requires a negative
slowly varying bulk potential which implies an anti-de Sitter-like bulk
geometry and could be possibly realized from the higher dimensional
supergravities or string theory. We find the similar constraint for the moving
brane cases and that the quintessence on it has the effect as a mildly
time-varying Newton constant.Comment: 16pages, no figure, Latex; revised version, references added, typos
corrected, abstract and comments improved; final version, will appear in PR
Stable, Time-Dependent, Exact Solutions for Brane Models with a Bulk Scalar Field
We derive two classes of brane-world solutions arising in the presence of a
bulk scalar field. For static field configurations, we adopt a time-dependent,
factorizable metric ansatz that allows for radion stabilization. The solutions
are characterized by a non-trivial warping along the extra dimension, even in
the case of a vanishing bulk cosmological constant, and lead to a variety of
inflationary, time-dependent solutions of the 3D scale factor on the brane. We
also derive the constraints necessary for the stability of these solutions
under time-dependent perturbations of the radion field, and we demonstrate the
existence of phenomenologically interesting, stable solutions with a positive
cosmological constant on the brane.Comment: 24 pages, latex, 4 eps figur
The dS/CFT Correspondence and the Big Smash
Recent observations suggest that the cosmological equation-of-state parameter
w is close to -1. To say this is to imply that w could be slightly less than
-1, which leads to R.Caldwell's "Phantom cosmologies". These often have the
property that they end in a "Big Smash", a final singularity in which the
Universe is destroyed in a finite proper time by excessive *expansion*. We show
that, classically, this fate is not inevitable: there exist Smash-free Phantom
cosmologies, obtained by a suitable perturbation of the deSitter equation of
state, in which the spacetime is in fact asymptotically deSitter. [Contrary to
popular belief, such cosmologies, which violate the Dominant Energy Condition,
do not necessarily violate causality.] We also argue, however, that the
physical interpretation of these classically acceptable spacetimes is radically
altered by ``holography'', as manifested in the dS/CFT correspondence. It is
shown that, if the boundary CFTs have conventional properties, then recent
ideas on "time as an inverse renormalization group flow" can be used to rule
out these cosmologies. Very recently, however, it has been argued that the CFTs
in dS/CFT are of a radically unconventional form, and this opens up the
possibility that Smash-free Phantom spacetimes offer a simple model of a
"bouncing" cosmology in which the quantum-mechanical entanglement of the field
theories in the infinite past and future plays an essential role.Comment: 22 pages, clarification of triple analytic continuation, additional
Comments added in the light of hep-th/020724
BEC Collapse and Dynamical Squeezing of Vacuum Fluctuations
We analyze the phenomena of Bose Novae, as described by Donley et al [Nature
412, 295 (2001)], by focusing on the behavior of excitations or fluctuations
above the condensate, as driven by the dynamics of the condensate (rather than
the dynamics of the condensate alone or the kinetics of the atoms). The
dynamics of the condensate squeezes and amplifies the quantum excitations,
mixing the positive and negative frequency components of their wave functions
thereby creating particles which appear as bursts and jets. By analyzing the
changing amplitude and particle content of these excitations, our simple
physical picture (based on a test field approximation) explains well the
overall features of the Bose Novae phenomena and provide excellent quantitative
fits with experimental data on several aspects, such as the scaling behavior of
the collapse time and the amount of particles in the jet. The predictions of
the bursts at this level of approximation is less than satisfactory but may be
improved on by including the backreaction of the excitations on the condensate.
The mechanism behind the dominant effect -- parametric amplification of vacuum
fluctuations and freezing of modes outside of horizon -- is similar to that of
cosmological particle creation and structure formation in a rapid quench (which
is fundamentally different from Hawking radiation in black holes). This shows
that BEC dynamics is a promising venue for doing `laboratory cosmology'.Comment: Latex 36 pages, 6 figure
Brane cosmology with curvature corrections
We study the cosmology of the Randall-Sundrum brane-world where the
Einstein-Hilbert action is modified by curvature correction terms: a
four-dimensional scalar curvature from induced gravity on the brane, and a
five-dimensional Gauss-Bonnet curvature term. The combined effect of these
curvature corrections to the action removes the infinite-density big bang
singularity, although the curvature can still diverge for some parameter
values. A radiation brane undergoes accelerated expansion near the minimal
scale factor, for a range of parameters. This acceleration is driven by the
geometric effects, without an inflaton field or negative pressures. At late
times, conventional cosmology is recovered.Comment: RevTex4, 8 pages, no figures, minor change
Dilatonic quantum multi-brane-worlds
d5 dilatonic gravity action with surface counterterms motivated by AdS/CFT
correspondence and with contributions of brane quantum CFTs is considered
around AdS-like bulk. The effective equations of motion are constructed. They
admit two (outer and inner) or multi-brane solutions where brane CFTs may be
different. The role of quantum brane CFT is in inducing of complicated brane
dilatonic gravity. For exponential bulk potentials the number of AdS-like bulk
spaces is found in analytical form.The correspondent flat or curved (de Sitter
or hyperbolic) dilatonic two branes are created, as a rule, thanks to quantum
effects. The observable early Universe may correspond to inflationary brane.
The found dilatonic quantum two brane-worlds usually contain the naked
singularity but in couple explicit examples the curvature is finite and horizon
(corresponding to wormhole-like space) appears.Comment: LaTeX file, 25 pages, discussion is enlarge
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