7,181 research outputs found
The population and reproductive biology of Pseudochromis Queenslandica at One Tree Island, Great Barrier Reef
The China-Russia Axis: What does it want and how will it get it?
This paper examines the statements and actions by China and Russia and its leaders, ascertains what their economic and military objectives are and why, and describes how this powerful “Axis” intends to achieve them
On the Magnitude of Dark Energy Voids and Overdensities
We investigate the clustering of dark energy within matter overdensities and
voids. In particular, we derive an analytical expression for the dark energy
density perturbations, which is valid both in the linear, quasi-linear and
fully non-linear regime of structure formation. We also investigate the
possibility of detecting such dark energy clustering through the ISW effect. In
the case of uncoupled quintessence models, if the mass of the field is of order
the Hubble scale today or smaller, dark energy fluctuations are always small
compared to the matter density contrast. Even when the matter perturbations
enter the non-linear regime, the dark energy perturbations remain linear. We
find that virialised clusters and voids correspond to local overdensities in
dark energy, with \delta_{\phi}/(1+w) \sim \Oo(10^{-5}) for voids,
\delta_{\phi}/(1+w) \sim \Oo(10^{-4}) for super-voids and
\delta_{\phi}/(1+w) \sim \Oo(10^{-5}) for a typical virialised cluster. If
voids with radii of exist within the visible Universe then
may be as large as . Linear overdensities of
matter and super-clusters generally correspond to local voids in dark energy;
for a typical super-cluster: \delta_{\phi}/(1+w) \sim \Oo(-10^{-5}). The
approach taken in this work could be straightforwardly extended to study the
clustering of more general dark energy models.Comment: 20 pages, 14 figures. Accepted by the Astrophys.
Reconstructing late Cenozoic deformation in central Panamint Valley, California: Evolution of slip partitioning in the Walker Lane
Advanced composite applications for sub-micron biologically derived microstructures
A major thrust of advanced material development is in the area of self-assembled ultra-fine particulate based composites (micro-composites). The application of biologically derived, self-assembled microstructures to form advanced composite materials is discussed. Hollow 0.5 micron diameter cylindrical shaped microcylinders self-assemble from diacetylenic lipids. These microstructures have a multiplicity of potential applications in the material sciences. Exploratory development is proceeding in application areas such as controlled release for drug delivery, wound repair, and biofouling as well as composites for electronic and magnetic applications, and high power microwave cathodes
D = 5 maximally supersymmetric Yang-Mills theory diverges at six loops
The connection of maximally supersymmetric Yang-Mills theory to the (2,0)
theory in six dimensions has raised the possibility that it might be
perturbatively ultraviolet finite in five dimensions. We test this hypothesis
by computing the coefficient of the first potential ultraviolet divergence of
planar (large N_c) maximally supersymmetric Yang-Mills theory in D = 5, which
occurs at six loops. We show that the coefficient is nonvanishing. Furthermore,
the numerical value of the divergence falls very close to an approximate
exponential formula based on the coefficients of the divergences through five
loops. This formula predicts the approximate values of the ultraviolet
divergence at loop orders L > 6 in the critical dimension D = 4 + 6/L. To
obtain the six-loop divergence we first construct the planar six-loop
four-point amplitude integrand using generalized unitarity. The ultraviolet
divergence follows from a set of vacuum integrals, which are obtained by
expanding the integrand in the external momenta. The vacuum integrals are
integrated via sector decomposition, using a modified version of the FIESTA
program.Comment: 31 pages, revtex, 12 figure
Evolution of the central Garlock fault zone, California: A major sinistral fault embedded in a dextral plate margin
On Optimizing Distributed Tucker Decomposition for Dense Tensors
The Tucker decomposition expresses a given tensor as the product of a small
core tensor and a set of factor matrices. Apart from providing data
compression, the construction is useful in performing analysis such as
principal component analysis (PCA)and finds applications in diverse domains
such as signal processing, computer vision and text analytics. Our objective is
to develop an efficient distributed implementation for the case of dense
tensors. The implementation is based on the HOOI (Higher Order Orthogonal
Iterator) procedure, wherein the tensor-times-matrix product forms the core
routine. Prior work have proposed heuristics for reducing the computational
load and communication volume incurred by the routine. We study the two metrics
in a formal and systematic manner, and design strategies that are optimal under
the two fundamental metrics. Our experimental evaluation on a large benchmark
of tensors shows that the optimal strategies provide significant reduction in
load and volume compared to prior heuristics, and provide up to 7x speed-up in
the overall running time.Comment: Preliminary version of the paper appears in the proceedings of
IPDPS'1
Notes on the dynamics of noncommutative U(2) and commutative SU(3) instantons
We examine the dynamics of noncommutative instantons of instanton number 2 and commutative instantons of instanton number 3 in 5D super Yang-Mills theory. We begin by detailing the construction of the 1=4-Bogamolyni-Prasad-Somerfeldt instanton solutions, their moduli space, and the moduli space potential using an explicit parametrization of the moduli space coordinates in terms of the biquaternions. We then go on to numerically analyze the dynamics on the moduli spaces we have constructed, discussing some of the numerical issues which arose, and describing the numerical algorithm we developed to solve them
After Midnight: A Regression Discontinuity Design in Length of Postpartum Hospital Stays
Patients who receive more hospital treatment tend to have worse underlying health, confounding estimates of the returns to such care. This paper compares the costs and benefits of extending the length of hospital stay following delivery using a discontinuity in stay length for infants born close to midnight. Third-party reimbursement rules in California entitle newborns to a minimum number of hospital "days," counted as the number of midnights in care. A newborn delivered at 12:05 a.m. will have an extra night of reimbursable care compared to an infant born minutes earlier. We use a dataset of all California births from 1991-2002, including nearly 100,000 births within 20 minutes of midnight, and find that children born just prior to midnight have significantly shorter lengths of stay than those born just after midnight, despite similar observable characteristics. Furthermore, a law change in 1997 entitled newborns to a minimum of 2 days in care. The midnight discontinuity can therefore be used to consider two distinct treatments: increasing stay length from one to two nights (prior to the law change) and from two to three nights (following the law change). On both margins, we find no effect of stay length on readmissions or mortality for either the infant or the mother, and the estimates are precise. The results suggest that for uncomplicated births, longer hospitals stays incur substantial costs without apparent health benefits.
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