6,234 research outputs found
Effect of Patterned Slip on Micro and Nanofluidic Flows
We consider the flow of a Newtonian fluid in a nano or microchannel with
walls that have patterned variations in slip length. We formulate a set of
equations to describe the effects on an incompressible Newtonian flow of small
variations in slip, and solve these equations for slow flows. We test these
equations using molecular dynamics simulations of flow between two walls which
have patterned variations in wettability. Good qualitative agreement and a
reasonable degree of quantitative agreement is found between the theory and the
molecular dynamics simulations. The results of both analyses show that
patterned wettability can be used to induce complex variations in flow. Finally
we discuss the implications of our results for the design of microfluidic
mixers using slip.Comment: 13 pages, 12 figures, final version for publicatio
The QCD phase diagram at nonzero baryon, isospin and strangeness chemical potentials: Results from a hadron resonance gas model
We use a hadron resonance gas model to study the QCD phase diagram at nonzero
temperature, baryon, isospin and strangeness chemical potentials. We determine
the temperature of the transition from the hadronic phase to the quark gluon
plasma phase using two different methods. We find that the critical
temperatures derived in both methods are in very good agreement. We find that
the critical surface has a small curvature. We also find that the critical
temperature's dependence on the baryon chemical potential at zero isospin
chemical potential is almost identical to its dependence on the isospin
chemical potential at vanishing baryon chemical potential. This result, which
holds when the chemical potentials are small, supports recent lattice
simulation studies. Finally, we find that at a given baryon chemical potential,
the critical temperature is lowered as either the isospin or the strangeness
chemical potential are increased. Therefore, in order to lower the critical
temperature, it might be useful to use different isotopes in heavy ion
collision experiments.Comment: 7 pages, 15 figure
A non-parametric method for measuring the local dark matter density
We present a new method for determining the local dark matter density using
kinematic data for a population of tracer stars. The Jeans equation in the
-direction is integrated to yield an equation that gives the velocity
dispersion as a function of the total mass density, tracer density, and the
tilt term that describes the coupling of vertical and radial motions. We then
fit a dark matter mass profile to tracer density and velocity dispersion data
to derive credible regions on the vertical dark matter density profile. Our
method avoids numerical differentiation, leading to lower numerical noise, and
is able to deal with the tilt term while remaining one dimensional. In this
study we present the method and perform initial tests on idealised mock data.
We also demonstrate the importance of dealing with the tilt term for tracers
that sample kpc above the disc plane. If ignored, this results in a
systematic underestimation of the dark matter density.Comment: V2: Improved tracer density description; increased number of mocks to
explore outliers; corrected sign error in the (R, z) velocity dispersion;
main conclusions unchanged. 19 pages, 14 figure
Indirect Search for Neutralino Dark Matter with High Energy Neutrinos
We investigate the prospects of indirect searches for supersymmetric
neutralino dark matter. Relic neutralinos gravitationally accumulate in the Sun
and their annihilations produce high energy neutrinos. Muon neutrinos of this
origin can be seen in large detectors like AMANDA, IceCube and ANTARES. We
evaluate the relic density and the detection rate in several models---the
minimal supersymmetric model, minimal supergravity, and supergravity with
non-universal Higgs boson masses at the grand unification scale. We make
realistic estimates for the indirect detection rates including effects of the
muon detection threshold, quark hadronization, and solar absorption. We find
good prospects for detection of neutralinos with mass above 200 GeV.Comment: 36 pages in REVTEX, 18 figure
Auditing the Numeracy Demands of the Middle Years Curriculum
The National Numeracy Review Report recognized that numeracy development requires an across the curriculum commitment. To explore the nature of this commitment we conducted a numeracy audit of the South Australian Middle Years curriculum, using a numeracy model that incorporates mathematical knowledge, dispositions, tools, contexts, and a critical orientation. All learning areas in the published curriculum were found to have distinctive numeracy demands. The audit should encourage teachers to promote numeracy in even richer ways in the curriculum they enact with students
Relic Neutralino Densities and Detection Rates with Nonuniversal Gaugino Masses
We extend previous analyses on the interplay between nonuniversalities in the
gaugino mass sector and the thermal relic densities of LSP neutralinos, in
particular to the case of moderate to large tan beta. We introduce a set of
parameters that generalizes the standard unified scenario to cover the complete
allowed parameter space in the gaugino mass sector. We discuss the physical
significance of the cosmologically preferred degree of degeneracy between
charginos and the LSP and study the effect this degree of degeneracy has on the
prospects for direct detection of relic neutralinos in the next round of dark
matter detection experiments. Lastly, we compare the fine tuning required to
achieve a satisfactory relic density with the case of universal gaugino masses,
as in minimal supergravity, and find it to be of a similar magnitude. The
sensitivity of quantifiable measures of fine-tuning on such factors as the
gluino mass and top and bottom masses is also examined.Comment: Uses RevTeX; 14 pages, 16 figure
Departures From Axisymmetric Morphology and Dynamics in Spiral Galaxies
New HI synthesis data have been obtained for six face-on galaxies with the
Very Large Array. These data and reanalyses of three additional data sets make
up a sample of nine face-on galaxies analyzed for deviations from axisymmetry
in morphology and dynamics. This sample represents a subsample of galaxies
already analyzed for morphological symmetry properties in the R-band. Four
quantitative measures of dynamical nonaxisymmetry are compared to one another
and to the quantitative measures of morphological asymmetry in HI and R-band to
investigate the relationships between nonaxisymmetric morphology and dynamics.
We find no significant relationship between asymmetric morphology and most of
the dynamical measures in our sample. A possible relationship is found,
however, between morphology and dynamical position angle differences between
approaching and receding sides of the galaxy.Comment: 24 pages, 19 figures, AASTeX, accepted for publication in AJ,
postscript figures available at
ftp://culebra.tn.cornell.edu/pub/david/figures.tar.g
Experimental observation of Frohlich superconductivity in high magnetic fields
Resistivity and irreversible magnetisation data taken within the
high-magnetic-field CDWx phase of the quasi-two-dimensional organic metal
alpha-(BEDT-TTF)2KHg(SCN)4 are shown to be consistent with a field-induced
inhomogeneous superconducting phase. In-plane skin-depth measurements show that
the resistive transition on entering the CDWx phase is both isotropic and
representative of the bulk.Comment: ten pages, four figure
The Status of MSSM Higgs Boson Searches at LEP
The most recently available results from searches conducted by the four LEP
experiments at 189 GeV center-of-mass energy for Higgs bosons of the Minimal
Supersymmetric Standard Model (MSSM) are presented. No evidence for a signal
has been observed, and the null result is used by the experiments, both
individually and collectively, to exclude regions of the MSSM parameter space
and to set lower limits on Higgs boson masses at 95% confidence level in
constrained MSSM scenarios.Comment: 7 pages, 6 figures, REVTeX, to appear in the proceedings of the DPF
'99 conference, 5-9 January 1999, Los Angeles, C
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