5,654 research outputs found
A relation between moduli space of D-branes on orbifolds and Ising model
We study D-branes transverse to an abelian orbifold C^3/Z_n Z_n. The moduli
space of the gauge theory on the D-branes is analyzed by combinatorial
calculation based on toric geometry. It is shown that the calculation is
related to a problemto count the number of ground states of an
antiferromagnetic Ising model. The lattice on which the Ising model is defined
is a triangular one defined on the McKay quiver of the orbifold.Comment: 20 pages, 13 figure
Hope for the Best, Prepare for the Worst: Response of Tall Steel Buildings to the ShakeOut Scenario Earthquake
This work represents an effort to develop one plausible realization of the effects of the scenario event on tall steel moment-frame buildings. We have used the simulated ground motions with three-dimensional nonlinear finite element models of three buildings in the 20-story class to simulate structural responses at 784 analysis sites spaced at approximately 4 km throughout the San Fernando Valley, the San Gabriel Valley, and the Los Angeles Basin. Based on the simulation results and available information on the number and distribution of steel buildings, the recommended damage scenario for the ShakeOut drill was 5% of the estimated 150 steel moment-frame structures in the 10–30 story range collapsing, 10% red-tagged, 15% with damage serious enough to cause loss of life, and 20% with visible damage requiring building closure
Microfluidic droplet control by photothermal interfacial flow
This paper was presented at the 4th Micro and Nano Flows Conference (MNF2014), which was held at University College, London, UK. The conference was organised by Brunel University and supported by the Italian Union of Thermofluiddynamics, IPEM, the Process Intensification Network, the Institution of Mechanical Engineers, the Heat Transfer Society, HEXAG - the Heat Exchange Action Group, and the Energy Institute, ASME Press, LCN London Centre for Nanotechnology, UCL University College London, UCL Engineering, the International NanoScience Community, www.nanopaprika.eu.Droplet-based microfluidics is an emerging field that can perform a variety of discrete operation of
tiny amount of reagent or individual cell. Noncontact manipulation of droplets in a microfluidic platform can
be achieved by using the Marangoni convection due to a local temperature gradient given by the irradiation
of heating light. This method provides noncontact, selective and flexible manipulation for droplets flowing in
microfluidic network. Although the potential of this selective operation method of droplets was confirmed,
the driving force exerted on droplets has not been quantitatively obtained. In this study, we have developed a
measurement system of the temperature field around droplets during the manipulation by light irradiation
and evaluated the manipulation force. In O/W emulsion system with oleic acid and buffer solution, oleic acid
for droplet and buffer solution for continuous phase, the temperature distribution around the droplets was
measured by laser-induced fluorescence. From the balance of drag force and photo-induced Marangoni force,
the driving force was determined. From the results, we confirmed the applicability of the noncontact droplet
manipulation using the photothermal Marangoni effect
Bayesian Updating and Model Class Selection of Deteriorating Hysteretic Structural Models using Seismic Response Data
Identification of structural models from measured earthquake response can play a
key role in structural health monitoring, structural control and improving performance-based
design. System identification using data from strong seismic shaking is complicated by the
nonlinear hysteretic response of structures where the restoring forces depend on the previous
time history of the structural response rather than on an instantaneous finite-dimensional
state. Furthermore, this inverse problem is ill-conditioned because even if some components
in the structure show substantial yielding, others will exhibit nearly elastic response, producing
no information about their yielding behavior. Classical least-squares or maximum likelihood
estimation will not work with a realistic class of hysteretic models because it will be
unidentifiable based on the data. On the other hand, Bayesian updating and model class selection
provide a powerful and rigorous approach to tackle this problem when implemented
using Markov Chain Monte Carlo simulation methods such as the Metropolis-Hastings, Gibbs
Sampler and Hybrid Monte Carlo algorithms. The emergence of these stochastic simulation
methods in recent years has led to a renaissance in Bayesian methods across all disciplines in
science and engineering because the high-dimensional integrations that are involved can now
be readily evaluated. The power of these methods to handle ill-conditioned or unidentifiable
system identification problems is demonstrated by using a recently-developed stochastic simulation
algorithm, Transitional Markov Chain Monte Carlo, to perform Bayesian updating and
model class selection on a class of Masing hysteretic structural models that are relatively
simple yet can give realistic responses to seismic loading. Examples will be given using deteriorating
hysteretic building models with simulated seismic response data
Simulation of an 1857-like Mw 7.9 San Andreas Fault Earthquake and the Response of Tall Steel Moment Frame Buildings in Southern California – A Prototype Study
In 1857, an earthquake of magnitude 7.9 occurred on the San Andreas fault, starting at Parkfield and rupturing
in a southeasterly direction for more than 360 km. Such a unilateral rupture produces significant directivity
toward the San Fernando and Los Angeles basins. The strong shaking in the basins due to this earthquake
would have had significant long-period content (2-8 s), and the objective of this study is to quantify the impact
of such an earthquake on two 18-story steel moment frame building models, hypothetically located at 636 sites
on a 3.5 km grid in southern California. End-to-end simulations include modeling the source and rupture of a
fault at one end, numerically propagating the seismic waves through the earth structure, simulating the damage
to engineered structures and estimating the economic impact at the other end using high-performance computing.
In this prototype study, we use an inferred finite source model of the magnitude 7.9, 2002 Denali fault
earthquake in Alaska, and map it onto the San Andreas fault with the rupture originating at Parkfield and
propagating southward over a distance of 290 km. Using the spectral element seismic wave propagation code,
SPECFEM3D, we simulate an 1857-like earthquake on the San Andreas fault and compute ground motions at
the 636 analysis sites. Using the nonlinear structural analysis program, FRAME3D, we subsequently analyze
3-D structural models of an existing tall steel building designed using the 1982 Uniform Building Code (UBC),
as well as one designed according to the 1997 UBC, subjected to the computed ground motion at each of these
sites. We summarize the performance of these structural models on contour maps of peak interstory drift.
We then perform an economic loss analysis for the two buildings at each site, using the Matlab Damage and
Loss Analysis (MDLA) toolbox developed to implement the PEER loss-estimation methodology. The toolbox
includes damage prediction and repair cost estimation for structural and non-structural components and allows
for the computation of the mean and variance of building repair costs conditional on engineering demand
parameters (i.e. inter-story drift ratios and peak floor accelerations). Here, we modify it to treat steel-frame
high-rises, including aspects such as mechanical, electrical and plumbing systems, traction elevators, and the
possibility of irreparable structural damage. We then generate contour plots of conditional mean losses for the
San Fernando and the Los Angeles basins for the pre-Northridge and modern code-designed buildings, allowing
for comparison of the economic effects of the updated code for the scenario event. In principle, by simulating
multiple seismic events, consistent with the probabilistic seismic hazard for a building site, the same basic
approach could be used to quantify the uncertain losses from future earthquakes
A cooperative game of information trading: The core, the nucleolus and the kernel
A certain trade of the information about a technological innovation between the initial owner of the information andn identical producers is studied by means of a cooperative game theoretic approach. The information trading situation is modelled as a cooperative (n+1)-person game with side payments. The symmetrical strong ɛ-cores (including the core), the nucleolus and the kernel of the cooperative game model are determined. Interpretations of these game theoretic solutions and their implications for the information trading problem are given
Response of tall steel buildings in southern California to the magnitude 7.8 shakeout scenario earthquake
Currently, there is a significant campaign being undertaken in southern California to increase public awareness
and readiness for the next large earthquake along the San Andreas Fault, culminating in a large-scale
earthquake response exercise. The USGS ShakeOut scenario is a key element to understanding the likely
effects of such an event. A source model for a M7.8 scenario earthquake has been created (Hudnet et al.
2007), and used in conjunction with a velocity model for southern California to generate simulated ground
motions for the event throughout the region (Graves et al. 2008). We were charged by the USGS to provide
one plausible realization of the effects of the scenario event on tall steel moment-frame buildings. We have
used the simulated ground motions with three-dimensional non-linear finite element models of three buildings
(in two orthogonal orientations and two different connection fragility conditions, for a total of twelve
cases) in the 20-story class to simulate structural responses at 784 analysis sites spaced at approximately
4 km throughout the San Fernando Valley, the San Gabriel Valley and the Los Angeles Basin. Based on
the simulation results and available information on the number and distribution of steel buildings, we have
recommended that the ShakeOut drill be planned with a damage scenario comprising of 5% of the estimated
150 steel moment frame structures in the 10-30 story range collapsing (8 collapses), 10% of the structures
red-tagged (16 red-tagged buildings), 15% of the structures with damage serious enough to cause loss of life
(24 buildings with fatalities), and 20% of the structures with visible damage requiring building closure (32
buildings with visible damage and possible injuries). This paper details the analytical study underlying these
recommendations
Shell Model Study of the Double Beta Decays of Ge, Se and Xe
The lifetimes for the double beta decays of Ge, Se and
Xe are calculated using very large shell model spaces. The two neutrino
matrix elements obtained are in good agreement with the present experimental
data. For eV we predict the following upper bounds to the
half-lives for the neutrinoless mode: , and . These results are the first from a new generation of Shell
Model calculations reaching O(10) dimensions
Neutrino Opacities in Neutron Stars with Kaon Condensates
The neutrino mean free paths in hot neutron-star matter are obtained in the
presence of kaon condensates. The kaon-induced neutrino absorption process,
which is allowed only in the presence of kaon condensates, is considered for
both nondegenerate and degenerate neutrinos. The neutrino mean free path due to
this process is compared with that for the neutrino-nucleon scattering. While
the mean free path for the kaon-induced neutrino absorption process is shown to
be shorter than the ordinary two-nucleon absorption process by several orders
of magnitude when temperature is not very high, the neutrino-nucleon scattering
process has still a dominant contribution to the neutrino opacity. Thus, the
kaon-induced neutrino absorption process has a minor effect on the thermal and
dynamical evolution of protoneutron stars.Comment: 35 pages, 4 figure
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