1,516 research outputs found
On waveform multigrid method
Waveform multigrid method is an efficient method for solving certain classes of time dependent PDEs. This paper studies the relationship between this method and the analogous multigrid method for steady-state problems. Using a Fourier-Laplace analysis, practical convergence rate estimates of the waveform multigrid iterations are obtained. Experimental results show that the analysis yields accurate performance prediction
Parallelization and visual analysis of multidimensional fields: Application to ozone production, destruction, and transport in three dimensions
Atmospheric modeling is a grand challenge problem for several reasons, including its inordinate computational requirements and its generation of large amounts of data concurrent with its use of very large data sets derived from measurement instruments like satellites. In addition, atmospheric models are typically run several times, on new data sets or to reprocess existing data sets, to investigate or reinvestigate specific chemical or physical processes occurring in the earth's atmosphere, to understand model fidelity with respect to observational data, or simply to experiment with specific model parameters or components
Quantum Monte Carlo Study of Strongly Correlated Electrons: Cellular Dynamical Mean-Field Theory
We study the Hubbard model using the Cellular Dynamical Mean-Field Theory
(CDMFT) with quantum Monte Carlo (QMC) simulations. We present the algorithmic
details of CDMFT with the Hirsch-Fye QMC method for the solution of the
self-consistently embedded quantum cluster problem. We use the one- and
two-dimensional half-filled Hubbard model to gauge the performance of CDMFT+QMC
particularly for small clusters by comparing with the exact results and also
with other quantum cluster methods. We calculate single-particle Green's
functions and self-energies on small clusters to study their size dependence in
one- and two-dimensions.Comment: 14 pages, 18 figure
Human brain distinctiveness based on EEG spectral coherence connectivity
The use of EEG biometrics, for the purpose of automatic people recognition,
has received increasing attention in the recent years. Most of current analysis
rely on the extraction of features characterizing the activity of single brain
regions, like power-spectrum estimates, thus neglecting possible temporal
dependencies between the generated EEG signals. However, important
physiological information can be extracted from the way different brain regions
are functionally coupled. In this study, we propose a novel approach that fuses
spectral coherencebased connectivity between different brain regions as a
possibly viable biometric feature. The proposed approach is tested on a large
dataset of subjects (N=108) during eyes-closed (EC) and eyes-open (EO) resting
state conditions. The obtained recognition performances show that using brain
connectivity leads to higher distinctiveness with respect to power-spectrum
measurements, in both the experimental conditions. Notably, a 100% recognition
accuracy is obtained in EC and EO when integrating functional connectivity
between regions in the frontal lobe, while a lower 97.41% is obtained in EC
(96.26% in EO) when fusing power spectrum information from centro-parietal
regions. Taken together, these results suggest that functional connectivity
patterns represent effective features for improving EEG-based biometric
systems.Comment: Key words: EEG, Resting state, Biometrics, Spectral coherence, Match
score fusio
Parallelized Inference for Gravitational-Wave Astronomy
Bayesian inference is the workhorse of gravitational-wave astronomy, for
example, determining the mass and spins of merging black holes, revealing the
neutron star equation of state, and unveiling the population properties of
compact binaries. The science enabled by these inferences comes with a
computational cost that can limit the questions we are able to answer. This
cost is expected to grow. As detectors improve, the detection rate will go up,
allowing less time to analyze each event. Improvement in low-frequency
sensitivity will yield longer signals, increasing the number of computations
per event. The growing number of entries in the transient catalog will drive up
the cost of population studies. While Bayesian inference calculations are not
entirely parallelizable, key components are embarrassingly parallel:
calculating the gravitational waveform and evaluating the likelihood function.
Graphical processor units (GPUs) are adept at such parallel calculations. We
report on progress porting gravitational-wave inference calculations to GPUs.
Using a single code - which takes advantage of GPU architecture if it is
available - we compare computation times using modern GPUs (NVIDIA P100) and
CPUs (Intel Gold 6140). We demonstrate speed-ups of for
compact binary coalescence gravitational waveform generation and likelihood
evaluation and more than for population inference within the
lifetime of current detectors. Further improvement is likely with continued
development. Our python-based code is publicly available and can be used
without familiarity with the parallel computing platform, CUDA.Comment: 5 pages, 4 figures, submitted to PRD, code can be found at
https://github.com/ColmTalbot/gwpopulation
https://github.com/ColmTalbot/GPUCBC
https://github.com/ADACS-Australia/ADACS-SS18A-RSmith Add demonstration of
improvement in BNS spi
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