1,190 research outputs found
Ab initio linear scaling response theory: Electric polarizability by perturbed projection
A linear scaling method for calculation of the static {\em ab inito} response
within self-consistent field theory is developed and applied to calculation of
the static electric polarizability. The method is based on density matrix
perturbation theory [Niklasson and Challacombe, cond-mat/0311591], obtaining
response functions directly via a perturbative approach to spectral projection.
The accuracy and efficiency of the linear scaling method is demonstrated for a
series of three-dimensional water clusters at the RHF/6-31G** level of theory.
Locality of the response under a global electric field perturbation is
numerically demonstrated by approximate exponential decay of derivative density
matrix elements.Comment: 4.25 pages in PRL format, 2 figure
Recommended from our members
New polymorphous computing fabric.
This paper introduces a new polymorphous computing Fabric well suited to DSP and Image Processing and describes its implementation on a Configurable System on a Chip (CSOC). The architecture is highly parameterized and enables customization of the synthesized Fabric to achieve high performance for a specific class of application. For this reason it can be considered to be a generic model for hardware accelerator synthesis from a high level specification. Another important innovation is the Fabric uses a global memory concept, which gives the host processor random access to all the variables and instructions on the Fabric. The Fabric supports different computing models including MIMD, SPMD and systolic flow and permits dynamic reconfiguration. We present a specific implementation of a bank of FIR filters on a Fabric composed of 52 cells on the Altera Excalibur ARM running at 33 MHz. The theoretical performance of this Fabric is 1.8 GMACh. For the FIR application we obtain 1.6 GMAC/s real performance. Some automatic tools have been developed like the tool to provide a host access utility and assembler
Recommended from our members
Fabric-based systems: model, tools, applications.
A Fabric Based System is a parameterized cellular architecture in which an array of computing cells communicates with an embedded processor through a global memory . This architecture is customizable to different classes of applications by funtional unit, interconnect, and memory parameters, and can be instantiated efficiently on platform FPGAs . In previous work, we have demonstrated the advantage of reconfigurable fabrics for image and signal processing applications . Recently, we have build a Fabric Generator, a Java-based toolset that greatly accelerates construction of the fabrics presented in. A module-generation library is used to define, instantiate, and interconnect cells' datapaths . FG generates customized sequencers for individual cells or collections of cells . We describe the Fabric-Based System model, the FG toolset, and concrete realizations offabric architectures generated by FG on the Altera Excalibur ARM that can deliver 4.5 GigaMACs/s (8/16 bit data, Multiply-Accumulate)
Polarimetric variations of binary stars. V. Pre-main-sequence spectroscopic binaries located in Ophiuchus and Scorpius
We present polarimetric observations of 7 pre-main-sequence (PMS)
spectroscopic binaries located in the rho Oph and Upper Sco star forming
regions (SFRs). The average observed polarizations at 7660A are between 0.5%
and 3.5%. After estimates of the interstellar polarization are removed, all
binaries have an intrinsic polarization above 0.4%. Two binaries,
NTTS162814-2427 and NTTS162819-2423S, present high levels of intrinsic
polarization between 1.5% and 2.1%. All 7 PMS binaries have a statistically
variable or possibly variable polarization. Combining these results with our
previous sample of binaries located in the Tau, Aur and Ori SFRs, 68% of the
binaries have an intrinsic polarization above 0.5%, and 90% of the binaries are
polarimetrically variable or possibly variable. NTTS160814-1857,
NTTS162814-2427, and NTTS162819-2423S are clearly polarimetrically variable.
The first two also exhibit phase-locked variations over ~10 and ~40 orbits
respectively. NTTS160905-1859 shows periodic variations that are not
phased-locked and only present for short intervals of time. The amplitudes of
the variations reach a few tenths of a percent. The high-eccentricity system
NTTS162814-2427 shows single-periodic variations, in agreement with our
previous numerical simulations. Non-periodic events introduce stochastic noise
that partially masks the periodic variations and prevents the Brown, McLean, &
Emslie (1978) formalism from finding a reasonable estimate of the inclination.Comment: 63 pages, including 21 figures and 18 tables, accepted by A
Polarimetric variations of binary stars. IV. Pre-main-sequence spectroscopic binaries located in Taurus, Auriga, and Orion
We present polarimetric observations of 14 pre-main-sequence (PMS) binaries
located in the Taurus, Auriga, and Orion star forming regions. The majority of
the average observed polarizations are below 0.5%, and none are above 0.9%.
After removal of estimates of the interstellar polarization, about half the
binaries have an intrinsic polarization above 0.5%, even though most of them do
not present other evidences for the presence of circumstellar dust. Various
tests reveal that 77% of the PMS binaries have or possibly have a variable
polarization. LkCa3, Par1540, and Par2494 present detectable periodic and
phase-locked variations. The periodic polarimetric variations are noisier and
of a lesser amplitude (~0.1%) than for other types of binaries, such as hot
stars. This could be due to stochastic events that produce deviations in the
average polarization, a non-favorable geometry (circumbinary envelope), or the
nature of the scatterers (dust grains are less efficient polarizers than
electrons). Par1540 is a Weak-line TTauri Star, but nonetheless has enough dust
in its environment to produce detectable levels of polarization and variations.
A fourth interesting case is W134, which displays rapid changes in polarization
that could be due to eclipses. We compare the observations with some of our
numerical simulations, and also show that an analysis of the periodic
polarimetric variations with the Brown, McLean, & Emslie (BME) formalism to
find the orbital inclination is for the moment premature: non-periodic events
introduce stochastic noise that partially masks the periodic low-amplitude
variations and prevents the BME formalism from finding a reasonable estimate of
the orbital inclination.Comment: 70 pages, 20 figures, to be published in the Astronomical Journa
Recommended from our members
Implementation of the shower max electron trigger at CDF
The authors have built and installed new electronics which brings the central shower max detector into the CDF Level-2 trigger. By matching a stiff track from the central fast track processor to an associated shower max cluster, this trigger improvement reduces the electron Level-2 cross section by approximately 50% while retaining greater than 85% of real electrons and allows the authors to lower their electron trigger threshold
The Effect of Multiple Scattering on the Polarization from Binary Star Envelopes. I. Self- and Externally Illuminated Disks
We present the results of a Monte Carlo radiative transfer code that
calculates the polarization produced by multiple Thomson scattering and
variable absorptive opacity in a circumstellar disk around one component of a
close detached binary system. We consider in detail the polarization variations
over the binary cycle that result from the disk's illumination by the external
star and by its own volume emission. We identify key features of these
polarization phase curves and investigate their behavior as functions of
optical depth, albedo, and inclination for geometrically thin and thick disks.
The polarization due to disk self-illumination is sensitive to the internal
optical characteristics of the disk, while the polarization arising from
external illumination is mainly sensitive to the disk's geometrical thickness.
With appropriate flux weighting, these results, combined with those for an
internally illuminated disk, allow simulation of the polarization signature
from an arbitrary binary-disk system.Comment: 34 pages, 17 figures. Submitted to ApJ, revised in response to
referee comments. Color figures available from
http://www.ruf.rice.edu/~jhoffman/monte/colorfigs.htm
Search for the Supersymmetric Partner of the Top-Quark in Collisions at
We report on a search for the supersymmetric partner of the top quark (stop)
produced in events using of
collisions at recorded with the Collider Detector at
Fermilab. In the case of a light stop squark, the decay of the top quark into
stop plus the lightest supersymmetric particle (LSP) could have a significant
branching ratio. The observed events are consistent with Standard Model production and decay. Hence, we set limits on the branching ratio of
the top quark decaying into stop plus LSP, excluding branching ratios above 45%
for a LSP mass up to 40 {\rm GeV/c}.Comment: 11 pages, 4 figure
Measurement of Rapidity Distribution for High Mass Drell-Yan ee Pairs at CDF
We report on the first measurement of the rapidity distribution dsigma/dy
over nearly the entire kinematic region of rapidity for e^+e^- pairs in the
Z-boson region of 66116 GeV/c^2.
The data sample consists of 108 pb^{-1} of ppbar collisions at \sqrt{s}=1.8 TeV
taken by the Collider Detector at Fermilab during 1992--1995. The total cross
section in the -boson region is measured to be 252 +- 11 pb. The measured
total cross section and d\sigma/dy are compared with quantum chromodynamics
calculations in leading and higher orders.Comment: 7 pages, 3 figures. Submitted to Physical Review Letter
Search for Narrow Diphoton Resonances and for gamma-gamma+W/Z Signatures in p\bar p Collisions at sqrt(s)=1.8 TeV
We present results of searches for diphoton resonances produced both
inclusively and also in association with a vector boson (W or Z) using 100
pb^{-1} of p\bar p collisions using the CDF detector. We set upper limits on
the product of cross section times branching ratio for both p\bar
p\to\gamma\gamma + X and p\bar p\to\gamma\gamma + W/Z. Comparing the inclusive
production to the expectations from heavy sgoldstinos we derive limits on the
supersymmetry-breaking scale sqrt{F} in the TeV range, depending on the
sgoldstino mass and the choice of other parameters. Also, using a NLO
prediction for the associated production of a Higgs boson with a W or Z boson,
we set an upper limit on the branching ratio for H\to\gamma\gamma. Finally, we
set a lower limit on the mass of a `bosophilic' Higgs boson (e.g. one which
couples only to \gamma, W, and Z$ bosons with standard model couplings) of 82
GeV/c^2 at 95% confidence level.Comment: 30 pages, 11 figure
- …