12,165 research outputs found
Dynamic mechanical analysis and organization/storage of data for polymetric materials
Dynamic mechanical analysis was performed on a variety of temperature resistant polymers and composite resin matrices. Data on glass transition temperatures and degree of cure attained were derived. In addition a laboratory based computer system was installed and data base set up to allow entry of composite data. The laboratory CPU termed TYCHO is based on a DEC PDP 11/44 CPU with a Datatrieve relational data base. The function of TYCHO is integration of chemical laboratory analytical instrumentation and storage of chemical structures for modeling of new polymeric structures and compound
HepForge: A lightweight development environment for HEP software
Setting up the infrastructure to manage a software project can become a task
as significant writing the software itself. A variety of useful open source
tools are available, such as Web-based viewers for version control systems,
"wikis" for collaborative discussions and bug-tracking systems, but their use
in high-energy physics, outside large collaborations, is insubstantial.
Understandably, physicists would rather do physics than configure project
management tools.
We introduce the CEDAR HepForge system, which provides a lightweight
development environment for HEP software. Services available as part of
HepForge include the above-mentioned tools as well as mailing lists, shell
accounts, archiving of releases and low-maintenance Web space. HepForge also
exists to promote best-practice software development methods and to provide a
central repository for re-usable HEP software and phenomenology codes.Comment: 3 pages, 0 figures. To be published in proceedings of CHEP06. Refers
to the HepForge facility at http://hepforge.cedar.ac.u
HepData and JetWeb: HEP data archiving and model validation
The CEDAR collaboration is extending and combining the JetWeb and HepData
systems to provide a single service for tuning and validating models of
high-energy physics processes. The centrepiece of this activity is the fitting
by JetWeb of observables computed from Monte Carlo event generator events
against their experimentally determined distributions, as stored in HepData.
Caching the results of the JetWeb simulation and comparison stages provides a
single cumulative database of event generator tunings, fitted against a wide
range of experimental quantities. An important feature of this integration is a
family of XML data formats, called HepML.Comment: 4 pages, 0 figures. To be published in proceedings of CHEP0
Quark mass uncertainties revive KSVZ axion dark matter
The Kaplan-Manohar ambiguity in light quark masses allows for a larger
uncertainty in the ratio of up to down quark masses than naive estimates from
the chiral Lagrangian would indicate. We show that it allows for a relaxation
of experimental bounds on the QCD axion, specifically KSVZ axions in the eV mass range composing 100% of the galactic dark matter halo can evade the
experimental limits placed by the ADMX collaboration.Comment: 9 pages, 5 figure
Stops and MET: the shape of things to come
LHC experiments have placed strong bounds on the production of supersymmetric
colored particles (squarks and gluinos), under the assumption that all flavors
of squarks are nearly degenerate. However, the current experimental constraints
on stop squarks are much weaker, due to the smaller production cross section
and difficult backgrounds. While light stops are motivated by naturalness
arguments, it has been suggested that such particles become nearly impossible
to detect near the limit where their mass is degenerate with the sum of the
masses of their decay products. We show that this is not the case, and that
searches based on missing transverse energy (MET) have significant reach for
stop masses above 175 GeV, even in the degenerate limit. We consider direct
pair production of stops, decaying to invisible LSPs and tops with either
hadronic or semi-leptonic final states. Modest intrinsic differences in MET are
magnified by boosted kinematics and by shape analyses of MET or suitably-chosen
observables related to MET. For these observables we show that the
distributions of the relevant backgrounds and signals are well-described by
simple analytic functions, in the kinematic regime where signal is enhanced.
Shape analyses of MET-related distributions will allow the LHC experiments to
place significantly improved bounds on stop squarks, even in scenarios where
the stop-LSP mass difference is degenerate with the top mass. Assuming 20/fb of
luminosity at 8 TeV, we conservatively estimate that experiments can exclude or
discover degenerate stops with mass as large as ~ 360 GeV and 560 GeV for
massless LSPs.Comment: Version submitted to journal with improved analysis and small fixes,
27 pages, 11 figures, 2 table
Step-induced unusual magnetic properties of ultrathin Co/Cu films: ab initio study
We have performed ab initio studies to elucidate the unusual magnetic
behavior recently observed in epitaxial Co films upon absorption of
submonolayers of Cu and other materials. We find that a submonolayer amount of
Cu on a stepped Co/Cu (100) film changes dramatically the electronic and
magnetic structure of the system. The effect is mainly due to hybridization of
Co and Cu -electrons when copper forms a ``wire'' next to a Co step at the
surface. As a result, a non-collinear arrangement of magnetic moments
(switching of the easy axis) is promoted. [PACS 75.70.Ak,75.70.-i]Comment: 10 pages, RevTeX 3.0, 4 PostScript figures available on request from
A. Bratkovsky at [email protected]
The XMM-Newton survey of the Small Magellanic Cloud: The X-ray point-source catalogue
Local-Group galaxies provide access to samples of X-ray source populations of
whole galaxies. The XMM-Newton survey of the Small Magellanic Cloud (SMC)
completely covers the bar and eastern wing with a 5.6 deg^2 area in the
(0.2-12.0) keV band. To characterise the X-ray sources in the SMC field, we
created a catalogue of point sources and sources with moderate extent. Sources
with high extent (>40") have been presented in a companion paper. We searched
for point sources in the EPIC images using sliding-box and maximum-likelihood
techniques and classified the sources using hardness ratios, X-ray variability,
and their multi-wavelength properties. The catalogue comprises 3053 unique
X-ray sources with a median position uncertainty of 1.3" down to a flux limit
for point sources of ~10^-14 erg cm^-2 s^-1 in the (0.2-4.5) keV band,
corresponding to 5x10^33 erg s^-1 for sources in the SMC. We discuss
statistical properties, like the spatial distribution, X-ray colour diagrams,
luminosity functions, and time variability. We identified 49 SMC high-mass
X-ray binaries (HMXB), four super-soft X-ray sources (SSS), 34 foreground
stars, and 72 active galactic nuclei (AGN) behind the SMC. In addition, we
found candidates for SMC HMXBs (45) and faint SSSs (8) as well as AGN (2092)
and galaxy clusters (13). We present the most up-to-date catalogue of the X-ray
source population in the SMC field. In particular, the known population of
X-ray binaries is greatly increased. We find that the bright-end slope of the
luminosity function of Be/X-ray binaries significantly deviates from the
expected universal high-mass X-ray binary luminosity function.Comment: 32 pages, 18 figures, accepted for publication in A&A, catalog will
be available at CD
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