188 research outputs found
Knowledge based improvement : simulation and artificial intelligence for understanding and improving decision making in an operations system
The thesis investigates the possibility of using simulation for understanding and
improving the design of decision making in a real context. The approach is based on the
problem of representing decision making behaviour in Discrete Event Simulation.
An investigation of existing techniques led to the design of a methodology known as
Knowledge Based Improvement (KBI). The KBI covers the key stages of the process of
using simulation for understanding and improving the design of decision making. Using a
research strategy that involves a case study in Ford, the research tests each stage of KBI.
The thesis explains how simulation can be used for understanding real decision making
problems and for collecting the data required for modelling individual decision making
strategies. The thesis demonstrates the possibility of a simulation based knowledge
elicitation in a real context and it investigates the practical difficulties involved in this
process.
The research tests the process of understanding decision making policies by modelling
specific decision makers using Artificial Intelligence. It tests the use of simulation for
assessing the decision making strategies and it shows that simulation can be used for
identifying efficient strategies and for improving the design of decision making practices.
The thesis reports the degree of success of the approach in relation to the data that were
collected and it describes the validation checks that were undertaken. In addition, it
reports the lessons learned from the application of the KBI methodology, the overall
success of the approach and the main limitations that were identified during the
implementation
Particle motion and gravitational lensing in the metric of a dilaton black hole in a de Sitter universe
We consider the metric exterior to a charged dilaton black hole in a de
Sitter universe. We study the motion of a test particle in this metric.
Conserved quantities are identified and the Hamilton-Jacobi method is employed
for the solutions of the equations of motion. At large distances from the black
hole the Hubble expansion of the universe modifies the effective potential such
that bound orbits could exist up to an upper limit of the angular momentum per
mass for the orbiting test particle. We then study the phenomenon of strong
field gravitational lensing by these black holes by extending the standard
formalism of strong lensing to the non-asymptotically flat dilaton-de Sitter
metric. Expressions for the various lensing quantities are obtained in terms of
the metric coefficients.Comment: 8 pages, RevTex, 1 eps figures; discussion improved; typos corrected;
references adde
Evolution of a Primordial Black Hole Population
We reconsider in this work the effects of an energy absorption term in the
evolution of primordial black holes (hereafter PBHs) in the several epochs of
the Universe. A critical mass is introduced as a boundary between the accreting
and evaporating regimes of the PBHs. We show that the growth of PBHs is
negligible in the Radiation-dominated Era due to scarcity of energy density
supply from the expanding background, in agreement with a previous analysis by
Carr and Hawking, but that nevertheless the absorption term is large enough for
black holes above the critical mass to preclude their evaporation until the
universe has cooled sufficiently. The effects of PBH motion are also discussed:
the Doppler effect may give rise to energy accretion in black-holes with large
peculiar motions relative to background. We discuss how cosmological
constraints are modified by the introduction of the critical mass since that
PBHs above it do not disturb the CMBR. We show that there is a large range of
admissible masses for PBHs above the critical mass but well below the
cosmological horizon. Finally we outline a minimal kinetic formalism, solved in
some limiting cases, to deal with more complicated cases of PBH populationsComment: RevTex file, 8 pp., 3 .ps figures available upon request from
[email protected]
Quantum Corrections for a Braneworld Black Hole
By using the quantum tunneling approach over semiclassical approximations, we
study the quantum corrections to the Hawking temperature, entropy and
Bekenstein-Hawking entropy-area relation for a black hole lying on a brane.Comment: 8 pages, accepted for publication in IJTP, references adde
Kang-Redner Anomaly in Cluster-Cluster Aggregation
The large time, small mass, asymptotic behavior of the average mass
distribution \pb is studied in a -dimensional system of diffusing
aggregating particles for . By means of both a renormalization
group computation as well as a direct re-summation of leading terms in the
small reaction-rate expansion of the average mass distribution, it is shown
that \pb \sim \frac{1}{t^d} (\frac{m^{1/d}}{\sqrt{t}})^{e_{KR}} for , where and . In two
dimensions, it is shown that \pb \sim \frac{\ln(m) \ln(t)}{t^2} for . Numerical simulations in two dimensions supporting the analytical
results are also presented.Comment: 11 pages, 6 figures, Revtex
Information transfer using a single particle path-spin hybrid entangled state
The path-spin entangled state of a single spin-1/2 particle is considered
which is generated by using a beam-spitter and a spin-flipper. Using this
hybrid entanglement at the level of a single particle as a resource, we
formulate a protocol for transferring of the state of an unknown qubit to a
distant location. Our scheme is implemented by a sequence of unitary operations
along with suitable spin-measurements, as well as by using classical
communication between the two spatially separated parties. This protocol, thus,
demonstrates the possibility of using intraparticle entanglement as a physical
resource for performing information theoretic tasks
Astrophysical constraints on primordial black holes in Brans-Dicke theory
We consider cosmological evolution in Brans-Dicke theory with a population of
primordial black holes. Hawking radiation from the primordial black holes
impacts various astrophysical processes during the evolution of the Universe.
The accretion of radiation by the black holes in the radiation dominated era
may be effective in imparting them a longer lifetime. We present a detailed
study of how this affects various standard astrophysical constraints coming
from the evaporation of primordial black holes. We analyze constraints from the
present density of the Universe, the present photon spectrum, the distortion of
the cosmic microwave background spectrum and also from processes affecting
light element abundances after nucleosynthesis. We find that the constraints on
the initial primordial black hole mass fractions are tightened with increased
accretion efficiency.Comment: 15 page
Brane Decay of a (4+n)-Dimensional Rotating Black Hole. II: spin-1 particles
The present works complements and expands a previous one, focused on the
emission of scalar fields by a (4+n)-dimensional rotating black hole on the
brane, by studying the emission of gauge fields on the brane from a similar
black hole. A comprehensive analysis of the particle, energy and angular
momentum emission rates is undertaken, for arbitrary angular momentum of the
black hole and dimensionality of spacetime. Our analysis reveals the existence
of a number of distinct features associated with the emission of spin-1 fields
from a rotating black hole on the brane, such as the behaviour and magnitude of
the different emission rates, the angular distribution of particles and energy,
the relative enhancement compared to the scalar fields, and the magnitude of
the superradiance effect. Apart from their theoretical interest, these features
can comprise clear signatures of the emission of Hawking radiation from a
brane-world black hole during its spin-down phase upon successful detection of
this effect during an experiment.Comment: 35 pages, 19 figures, Latex fil
Dark energy from quantum wave function collapse of dark matter
Dynamical wave function collapse models entail the continuous liberation of a
specified rate of energy arising from the interaction of a fluctuating scalar
field with the matter wave function. We consider the wave function collapse
process for the constituents of dark matter in our universe. Beginning from a
particular early era of the universe chosen from physical considerations, the
rate of the associated energy liberation is integrated to yield the requisite
magnitude of dark energy around the era of galaxy formation. Further, the
equation of state for the liberated energy approaches
asymptotically, providing a mechanism to generate the present acceleration of
the universe.Comment: 5 pages in Elsevier style to match with version published in Phys.
Lett.
Epidemic processes with immunization
We study a model of directed percolation (DP) with immunization, i.e. with
different probabilities for the first infection and subsequent infections. The
immunization effect leads to an additional non-Markovian term in the
corresponding field theoretical action. We consider immunization as a small
perturbation around the DP fixed point in d<6, where the non-Markovian term is
relevant. The immunization causes the system to be driven away from the
neighbourhood of the DP critical point. In order to investigate the dynamical
critical behaviour of the model, we consider the limits of low and high first
infection rate, while the second infection rate remains constant at the DP
critical value. Scaling arguments are applied to obtain an expression for the
survival probability in both limits. The corresponding exponents are written in
terms of the critical exponents for ordinary DP and DP with a wall. We find
that the survival probability does not obey a power law behaviour, decaying
instead as a stretched exponential in the low first infection probability limit
and to a constant in the high first infection probability limit. The
theoretical predictions are confirmed by optimized numerical simulations in 1+1
dimensions.Comment: 12 pages, 11 figures. v.2: minor correction
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