18,972 research outputs found
Test of a simple and flexible molecule model for alpha-, beta- and gamma-S8 crystals
S8 is the most stable compound of elemental sulfur in solid and liquid
phases, at ambient pressure and below 400K. Three crystalline phases of S8 have
been clearly identified in this range of thermodynamic parameters, although no
calculation of its phase diagram has been performed yet. alpha- and gamma-S8
are orientationally ordered crystals while beta-S8 is measured as
orientationally disordered. In this paper we analyze the phase diagram of S8
crystals, as given by a simple and flexible molecule model, via a series of
molecular dynamics (MD) simulations.
The calculations are performed in the constant pressure- constant temperature
ensemble, using an algorithm that is able to reproduce structural phase
transitions.Comment: RevTex,7 pages, 5 figures,to appear in J. Chem. Phy
Cycles of construing in radicalization and deradicalization: a study of Salafist Muslims.
© Taylor & Francis Group, LLC.This article explores radicalization and deradicalization by considering the experiences of six young Tunisian people who had become Salafist Muslims. Their responses to narrative interviews and repertory grid technique are considered from a personal construct perspective, revealing processes of construing and reconstruing, as well as relevant aspects of the structure and content of their construct systems. In two cases, their journeys involved not only radicalization but self-deradicalization, and their experiences are drawn on to consider implications for deradicalization.Peer reviewedFinal Accepted Versio
The life and work of Marquis Robert de Wavrin, an early visual anthropologist
This article traces the life and work of Marquis Robert de Wavrin de Villers au Tertre (1888–1971), a Belgian explorer and ethnographer. While fragments of his oeuvre are familiar to scholars of South America, he is almost completely unknown in historical studies, and largely forgotten within anthropology too. Here we will explore his filmic work as well as its contribution to the history of visual anthropology. While de Wavrin’s work cannot be divorced from the discipline’s colonial and Eurocentric heritage, we show that his visual record provides notable historic insights and merits further scholarly attention.SCOPUS: ar.jDecretOANoAutActifinfo:eu-repo/semantics/publishe
Technology requirements for advanced earth-orbital transportation systems, dual-mode propulsion
The application of dual-mode propulsion concepts to fully reusable single-stage-to-orbit (SSTO) vehicles is discussed. Dual-mode propulsion uses main rocket engines that consume hydrocarbon fuels as well as liquid hydrogen fuel. Liquid oxygen is used as the oxidizer. These engine concepts were integrated into transportation vehicle designs capable of vertical takeoff, delivering a payload to earth orbit, and return to earth with a horizontal landing. Benefits of these vehicles were assessed and compared with vehicles using single-mode propulsion (liquid hydrogen and oxygen engines). Technology requirements for such advanced transportation systems were identified. Figures of merit, including life-cycle cost savings and research costs, were derived for dual-mode technology programs, and were used for assessments of potential benefits of proposed technology activities. Dual-mode propulsion concepts display potential for significant cost and performance benefits when applied to SSTO vehicles
Technology requirements for advanced earth-orbital transportation systems: Summary report
Areas of advanced technology that are either critical or offer significant benefits to the development of future Earth-orbit transportation systems were identified. Technology assessment was based on the application of these technologies to fully reusable, single-state-to-orbit (SSTO) vehicle concepts with horizontal landing capability. Study guidelines included mission requirements similar to space shuttle, an operational capability beginning in 1995, and main propulsion to be advanced hydrogen-fueled rocket engines. The technical and economic feasibility of this class of SSTO concepts were evaluated as well as the comparative features of three operational take-off modes, which were vertical boost, horizontal sled launch, and horizontal take-off with subsequent inflight fueling. Projections of both normal and accelerated technology growth were made. Figures of merit were derived to provide relative rankings of technology areas. The influence of selected accelerated areas on vehicle design and program costs was analyzed by developing near-optimum point designs
Appropriating the Returns from Industrial Research and Development
macroeconomics, industrial research and development, patent law
PHENIX and the Reaction Plane: Recent Results
During the past several years, experiments at RHIC have established that a
dense partonic medium is produced in Au+Au collisions at sqrt(s)=200 GeV.
Subsequently, a primary goal of analysis has been to understand and
characterize the dynamics underlying this new form of matter. Among the many
probes available, the measurements with respect to the reaction plane has
proven to be crucial to our understanding of a wide range of topics, from the
hydrodynamics of the initial expansion of the collision region to high-pt jet
quenching phenomena. Few tools have the ability to shed light on such a wide
variety of observables as the reacion plane. In this article, we discuss recent
PHENIX measurements with respect to the reaction plane, and the implications
for understanding the underlying physics of RHIC collisions.Comment: 9 pages, 13 figures, Submitted for proceedings to the Winter Workshop
on Nuclear Dynamics 2010, Ocho Rios, Jamaic
The StarScan plate measuring machine: overview and calibrations
The StarScan machine at the U.S. Naval Observatory (USNO) completed measuring
photographic astrograph plates to allow determination of proper motions for the
USNO CCD Astrograph Catalog (UCAC) program. All applicable 1940 AGK2 plates,
about 2200 Hamburg Zone Astrograph plates, 900 Black Birch (USNO Twin
Astrograph) plates, and 300 Lick Astrograph plates have been measured. StarScan
comprises of a CCD camera, telecentric lens, air-bearing granite table, stepper
motor screws, and Heidenhain scales to operate in a step-stare mode. The
repeatability of StarScan measures is about 0.2 micrometer. The CCD mapping as
well as the global table coordinate system has been calibrated using a special
dot calibration plate and the overall accuracy of StarScan x,y data is derived
to be 0.5 micrometer. Application to real photographic plate data shows that
position information of at least 0.65 micrometer accuracy can be extracted from
course grain 103a-type emulsion astrometric plates. Transformations between
"direct" and "reverse" measures of fine grain emulsion plate measures are
obtained on the 0.3 micrometer level per well exposed stellar image and
coordinate, which is at the limit of the StarScan machine.Comment: 24 pages, 8 figures, accepted for PAS
On the stability around Chariklo and the confinement of its rings
Chariklo has two narrow and dense rings, C1R and C2R, located at 391 km and
405 km, respectively. In the light of new stellar occultation data, we study
the stability around Chariklo. We also analyse three confinement mechanisms, to
prevent the spreading of the rings, based on shepherd satellites in resonance
with the edges of the rings. This study is made through a set of numerical
simulations and the Poincar\'e surface of section technique. From the numerical
simulation results we verify that, from the current parameters referring to the
shape of Chariklo, the inner edge of the stable region is much closer to
Chariklo than the rings. The Poincar\'e surface of sections allow us to
identify the first kind periodic and quasi-periodic orbits, and also the
resonant islands corresponding to the 1:2, 2:5, and 1:3 resonances. We
construct a map of a versus e space which gives the location and width of the
stable region and the 1:2, 2:5, and 1:3 resonances. We found that the first
kind periodic orbits family can be responsible for a stable region whose
location and size meet that of C1R, for specific values of the ring particles'
eccentricities. However, C2R is located in an unstable region if the width of
the ring is assumed to be about 120 m. After analysing different systems we
propose that the best confinement mechanism is composed of three satellites,
two of them shepherding the inner edge of C1R and the outer edge of C2R, while
the third satellite would be trapped in the 1:3 resonance.Comment: Accepted for publication in Astronomy & Astrophysic
LOCAL VARIABILITY IN THE ORBIT OF SATURN'S F RING
This work was supported by the Science and Technology Facilities Council (grant number ST/F007566/1)
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