3,171 research outputs found
EvoL: The new Padova T-SPH parallel code for cosmological simulations - I. Basic code: gravity and hydrodynamics
We present EvoL, the new release of the Padova N-body code for cosmological
simulations of galaxy formation and evolution. In this paper, the basic Tree +
SPH code is presented and analysed, together with an overview on the software
architectures. EvoL is a flexible parallel Fortran95 code, specifically
designed for simulations of cosmological structure formation on cluster,
galactic and sub-galactic scales. EvoL is a fully Lagrangian self-adaptive
code, based on the classical Oct-tree and on the Smoothed Particle
Hydrodynamics algorithm. It includes special features such as adaptive
softening lengths with correcting extra-terms, and modern formulations of SPH
and artificial viscosity. It is designed to be run in parallel on multiple CPUs
to optimize the performance and save computational time. We describe the code
in detail, and present the results of a number of standard hydrodynamical
tests.Comment: 33 pages, 49 figures, accepted on A&
Practical theories for service life prediction of critical aerospace structural components
A new second-order theory was developed for predicting the service lives of aerospace structural components. The predictions based on this new theory were compared with those based on the Ko first-order theory and the classical theory of service life predictions. The new theory gives very accurate service life predictions. An equivalent constant-amplitude stress cycle method was proposed for representing the random load spectrum for crack growth calculations. This method predicts the most conservative service life. The proposed use of minimum detectable crack size, instead of proof load established crack size as an initial crack size for crack growth calculations, could give a more realistic service life
Integrity in the fresh produce supply chain: solutions and approaches to an emerging issue
Food fraud is the misrepresentation of food in terms of labelling or documentation. The fresh produce supply chain is global with fresh produce grown many thousands of miles from the point of purchase and consumption. Long supply and complex fresh produce supply chains provide opportunity for fraudulent activity to occur especially further processing or re-packing of products to mask opaque practice and non-compliant behaviour. Price premiums for products designated as âhigh-valueâ, for example, organic produce, produce of particular provenance, or geographical production area provides motivation for less scrupulous actors to present for sale, produce that is mislabelled or misrepresented. People integrity as well as data, product and process integrity are gaining wider attention in the horticultural sector. Types of fraud critiqued in this review paper include mislabelling, substitution or misrepresentation of origin (country or regional location), method of production (organic or conventional) or incorrect varietal declaration. These challenges and the existing and emerging technologies that are both used within a quality assurance programme and alternatively used by regulators when investigating potential instances of fraudulent behaviour are considered. New methodological solutions and approaches are emerging and suc techniques will develop rapidly to meet the growing challenge of fraud and to ensure consumer trust in the industry is maintained especially as types of food fraud evolve and become more sophisticated
Employer Perceptions of Online Degrees: A Literature Review
This literature review explores the research about the perception of online degrees by potential employers or âgatekeepersâ in comparison with those earned in a traditional format. This is important because these perceptions can affect the employment opportunities or lack thereof of students and, in turn, institutions
Tests of Spurious Transport in Smoothed Particle Hydrodynamics
We have performed a series of systematic tests to evaluate the effects of
spurious transport in three-dimensional smoothed particle hydrodynamics (SPH)
calculations. Our tests investigate (i) particle diffusion, (ii) shock heating,
(iii) numerical viscosity, and (iv) angular momentum transport. The results are
useful for quantifying the accuracy of the SPH scheme, especially for problems
where shear flows or shocks are present, as well as for problems where true
hydrodynamic mixing is relevant.
We examine the different forms of artificial viscosity (AV) which have been
proposed by Monaghan, by Hernquist & Katz, and by Balsara. For each form, our
tests suggest a single set of values for the AV parameters and
(coefficients of the linear and quadratic terms) which are appropriate in a
large number of situations. We also discuss how these parameters should be
adjusted depending on the goals of the particular application. We find that
both the Hernquist & Katz and Balsara forms introduce relatively small amounts
of numerical viscosity. Furthermore, both Monaghan's and Balsara's AV do well
at treating shocks and at limiting the amount of spurious mixing. For these
reasons, we endorse the Balsara AV for use in a broad range of applications.Comment: 49 pages, 26 figures as 30 postscript files, submitted to The Journal
of Computational Physic
The X-ray Ridge Surrounding Sgr A* at the Galactic Center
We present the first detailed simulation of the interaction between the
supernova explosion that produced Sgr A East and the wind-swept inner ~ 2-pc
region at the Galactic center. The passage of the supernova ejecta through this
medium produces an X-ray ridge ~ 9'' to 15'' to the NE of the supermassive
black hole Sagittarius A* (Sgr A*). We show that the morphology and X-ray
intensity of this feature match very well with recently obtained Chandra
images, and we infer a supernova remnant age of less than 2,000 years. This
young age--a factor 3--4 lower than previous estimates--arises from our
inclusion of stellar wind effects in the initial (pre-explosion) conditions in
the medium. The supernova does not clear out the central ~ 0.2-pc region around
Sgr~A* and does not significantly alter the accretion rate onto the central
black hole upon passage through the Galactic center.Comment: 10 pages, 3 figures, submitted to ApJ
Composition Mixing during Blue Straggler Formation and Evolution
We use smoothed-particle hydrodynamics to examine differences between direct
collisions of single stars and binary star mergers in their roles as possible
blue straggler star formation mechanisms. We find in all cases that core helium
in the progenitor stars is largely retained in the core of the remnant, almost
independent of the type of interaction or the central concentration of the
progenitor stars.
We have also modelled the subsequent evolution of the hydrostatic remnants,
including mass loss and energy input from the hydrodynamical interaction. The
combination of the hydrodynamical and hydrostatic models enables us to predict
that little mixing will occur during the merger of two globular cluster stars
of equal mass. In contrast to the results of Proctor Sills, Bailyn, & Demarque
(1995), we find that neither completely mixed nor unmixed models can match the
absolute colors of observed blue stragglers in NGC 6397 at all luminosity
levels. We also find that the color distribution is probably the crucial test
for explanations of BSS formation - if stellar collisions or mergers are the
correct mechanisms, a large fraction of the lifetime of the straggler must be
spent away from the main sequence. This constraint appears to rule out the
possibility of completely mixed models. For NGC 6397, unmixed models predict
blue straggler lifetimes ranging from about 0.1 to 4 Gyr, while completely
mixed models predict a range from about 0.6 to 4 Gyr.Comment: AASTeX, 28 pg., accepted for ApJ, also available at
http://ucowww.ucsc.edu/~erics/bspaper.htm
Equilibrium Configurations of Strongly Magnetized Neutron Stars with Realistic Equations of State
We investigate equilibrium sequences of magnetized rotating stars with four
kinds of realistic equations of state (EOSs) of SLy (Douchin et al.), FPS
(Pandharipande et al.), Shen (Shen et al.), and LS (Lattimer & Swesty).
Employing the Tomimura-Eriguchi scheme to construct the equilibrium
configurations. we study the basic physical properties of the sequences in the
framework of Newton gravity. In addition we newly take into account a general
relativistic effect to the magnetized rotating configurations. With these
computations, we find that the properties of the Newtonian magnetized stars,
e.g., structure of magnetic field, highly depends on the EOSs.
The toroidal magnetic fields concentrate rather near the surface for Shen and
LS EOSs than those for SLy and FPS EOSs. The poloidal fields are also affected
by the toroidal configurations. Paying attention to the stiffness of the EOSs,
we analyze this tendency in detail. In the general relativistic stars, we find
that the difference due to the EOSs becomes small because all the employed EOSs
become sufficiently stiff for the large maximum density, typically greater than
. The maximum baryon mass of the magnetized stars
with axis ratio increases about up to twenty percents for that of
spherical stars. We furthermore compute equilibrium sequences at finite
temperature, which should serve as an initial condition for the hydrodynamic
study of newly-born magnetars. Our results suggest that we may obtain
information about the EOSs from the observation of the masses of magnetars.Comment: submitted to MNRA
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