4,382 research outputs found
Effect of spin-orbit interaction on a magnetic impurity in the vicinity of a surface
We propose a new mechanism for surface-induced magnetic anisotropy to explain
the thickness-dependence of the Kondo resistivity of thin films of dilute
magnetic alloys. The surface anisotropy energy, generated by spin-orbit
coupling on the magnetic impurity itself, is an oscillating function of the
distance d from the surface and decays as 1/d^2. Numerical estimates based on
simple models suggest that this mechanism, unlike its alternatives, gives rise
to an effect of the desired order of magnitude.Comment: 4 pages, 4 figure
On the Nature of the Strong Emission-Line Galaxies in Cluster Cl 0024+1654: Are Some the Progenitors of Low Mass Spheroidals?
We present new size, line ratio, and velocity width measurements for six
strong emission-line galaxies in the galaxy cluster, Cl 0024+1654, at redshift
z~0.4. The velocity widths from Keck spectra are all narrow (30<sigma<120
km/s), with three profiles showing double peaks. Four galaxies have low masses
(M<10^{10} Mo). Whereas three galaxies were previously reported to be possible
AGNs, none exhibit AGN-like emission line ratios or velocity widths. Two or
three appear as very blue spirals with the remainder more akin to luminous H-II
galaxies undergoing a strong burst of star formation. We propose that after the
burst subsides, these galaxies will transform into quiescent dwarfs, and are
thus progenitors of some cluster spheroidals (We adopt the nomenclature
suggested by Kormendy & Bender (1994), i.e., low-density, dwarf ellipsoidal
galaxies like NGC 205 are called `spheroidals' instead of `dwarf ellipticals')
seen today.Comment: 14 pages + 2 figures + 1 table, LaTeX, Acc. for publ. in ApJL also
available at http://www.ucolick.org/~deep/papers/papers.htm
Simulating Turbulence Using the Astrophysical Discontinuous Galerkin Code TENET
In astrophysics, the two main methods traditionally in use for solving the
Euler equations of ideal fluid dynamics are smoothed particle hydrodynamics and
finite volume discretization on a stationary mesh. However, the goal to
efficiently make use of future exascale machines with their ever higher degree
of parallel concurrency motivates the search for more efficient and more
accurate techniques for computing hydrodynamics. Discontinuous Galerkin (DG)
methods represent a promising class of methods in this regard, as they can be
straightforwardly extended to arbitrarily high order while requiring only small
stencils. Especially for applications involving comparatively smooth problems,
higher-order approaches promise significant gains in computational speed for
reaching a desired target accuracy. Here, we introduce our new astrophysical DG
code TENET designed for applications in cosmology, and discuss our first
results for 3D simulations of subsonic turbulence. We show that our new DG
implementation provides accurate results for subsonic turbulence, at
considerably reduced computational cost compared with traditional finite volume
methods. In particular, we find that DG needs about 1.8 times fewer degrees of
freedom to achieve the same accuracy and at the same time is more than 1.5
times faster, confirming its substantial promise for astrophysical
applications.Comment: 21 pages, 7 figures, to appear in Proceedings of the SPPEXA
symposium, Lecture Notes in Computational Science and Engineering (LNCSE),
Springe
Pyhtään kunnan kuljetusten optimointi ja tarkistustyökalu
Pyhtään kunta on yli 5 000 asukkaan maalaiskunta Kymenlaaksossa Kaakkois-Suomessa. Kunnan toimeksiantona selvitettiin kuljetusten parantamismahdollisuudet. Pyhtään kunnan kuljetusselvitys koostui neljästä eri kuljetusosa-alueesta: koulukuljetuksesta, vammaispalvelusta, ruokakuljetuksesta ja Pyhtään palvelulinjasta. Selvityksen pääpaino oli koulukuljetuksissa.
Tavoitteina oli löytää kuljetuksista kustannussäästöjä, selvittää vuoroliikenteen pysyvyys ja rakentaa tarkistustyökalu. Selvitystyö koostui myös Suomen lainsäädännön tarkastelusta, kuljetusten nykytilan selvittämisestä ja niiden mahdollisesta yhdistämisestä sekä koulukuljetuskustannusten laskemisesta.
Työmenetelmät olivat tiedon keruu ja analysointi, yhteydenotot ja haastattelut sekä tarkistustyökalun luominen MS Excel -taulukkolaskentaohjelmalla.
Työn tuloksena syntyivät koulukuljetuskartat ja ehdotus koulukuljetusportfolion laatimisesta sekä kaksi tarkistustyökalua. Lisäksi selvitystyössä päädyttiin siihen, että koulukuljetuskustannusten nousu on johtunut epäonnistuneesta kilpailutuksesta.The municipality of Pyhtää has over 5000 inhabitants and is located in Southern Finland. The aim of this thesis was to make a report to the municipality of Pyhtää, Finland. The report consisted of four different fields of transportation: school transport, services for the disabled, transport of perishable foodstuff and service line of Pyhtää. The main subject was the school transportation.
The aims of the thesis were to find cost savings, clarify the permanence of bus lines and create a control tool to the municipality’s personnel. The report also consisted of Finnish legislation, monitoring the present state of transport, drawing the route maps from the school transportation and counting the transportation costs.
The methods were finding and analyzing the available information, contacting and interviewing involved parties. The control tool was built with MS Office Excel –program.
The results of the thesis were the school transport’s route maps, suggestion to create a portfolio from the school transportation and two different versions of the control tool. In addition the thesis concluded that the cost of the school transportation has increased from the unsuccessful tendering
Friedel oscillations induced surface magnetic anisotropy
We present detailed numerical studies of the magnetic anisotropy energy of a
magnetic impurity near the surface of metallic hosts (Au and Cu), that we
describe in terms of a realistic tight-binding surface Green's function
technique. We study the case when spin-orbit coupling originates from the
d-band of the host material and we also investigate the case of a strong local
spin-orbit coupling on the impurity itself. The splitting of the impurity's
spin-states is calculated to leading order in the exchange interaction between
the impurity and the host atoms using a diagrammatic Green's function
technique. The magnetic anisotropy constant is an oscillating function of the
separation d from the surface: it asymptotically decays as 1/d2 and its
oscillation period is determined by the extremal vectors of the host's Fermi
Surface. Our results clearly show that the host-induced magnetic anisotropy
energy is by several orders of magnitude smaller than the anisotropy induced by
the local mechanism, which provides sufficiently large anisotropy values to
explain the size dependence of the Kondo resistance observed experimentally.Comment: 11 pages, 7 figures, submitted to PR
CLIWOC multilingual meteorological dictionary
This dictionary is the first attempt to express the wealth of archaic logbook wind force terms in a form that is comprehensible to the modern-day reader. Oliver and Kington (1970) and Lamb (1982) have drawn attention to the importance of logbooks in climatic studies, and Lamb (1991) offered a conversion scale for early eighteenth century English wind force terms, but no studies have thus far pursued the matter to any greater depth. This text attempts to make good this deficiency, and is derived from the research undertaken by the CLIWOC project1 in which British, Dutch, French and Spanish naval and merchant logbooks from the period 1750 to 1850 were used to derive a global database of climatic information. At an early stage in the project it was apparent that many of the logbook weather terms, whilst conforming to a conventional vocabulary, possessed meanings that were unclear to twenty-first century readers or had changed over time. This was particularly the case for the important element of wind force; but no special plea is entered for the evolution in nautical vocabulary, which often reflected more wide-ranging changes in the respective native languages.The key objective was to translate the archaic vocabulary of the late eighteenth and early nineteenth century mariner into expressions directly comparable with the Beaufort Scale (see Appendix I). Only then could the projects scientific programme be embarked upon. This dictionary is the result of the largest undertaking into logbook studies that has yet been carried out. Several thousand logbooks from British, Dutch, French and Spanish archives were examined, and the exercise offered a unique opportunity to explore the vocabulary of the one hundred year period beginning in 1750. The logbooks from which the raw data have been abstracted range widely across the North and South Atlantic and the Indian Oceans. Only the Pacific, largely in consequence of the paucity of regular naval activity in that area, is not well represented. The range of climates encountered in this otherwise wide geographic domain gives ample opportunity for the full range of the mariners nautical weather vocabulary to be assessed, from the calms of the Equatorial regions, through the gales of the mid-latitude systems to the fearsome storms of the tropical latitudes. The Trade Winds belts, the Doldrums, the unsettled mid-latitudes, even the icy wastes of the high latitudes, are all embraced in this study. It is not here intended to pass any judgements on the climatological record of the logbooks, and this text seeks only to provide a means of understanding archaic wind force terms and, other than to indicate those items that were not commonly used, no information is given on the frequency with which different terms appeared in the logbooks. Attention is, furthermore, confined to Dutch, English, French and Spanish because these once great imperial powers were the only nations able to support wide-ranging ocean-going fleets with their attendant collections of logbooks and documents over this long period of time. The work is offered to the wider academic community in the hope that they will prove to be of as much value as it has been to the CLIWOC team
A Semi-Empirical Model of the Infra-Red Universe
We present a simple model of the infra-red universe, based as much as
possible on local observations. We model the luminosity and number evolution of
disk and starburst galaxies, including the effects of dust, gas and spectral
evolution. Although simple, our approach is able to reproduce observations of
galaxy number counts and the infra-red and sub-millimeter extra-galactic
backgrounds. It provides a useful probe of galaxy formation and evolution out
to high redshift. The model demonstrates the significant role of the starburst
population and predicts high star formation rates at redshifts 3 to 4,
consistent with recent extinction-corrected observations of Lyman break
galaxies. Starbursting galaxies are predicted to dominate the current SCUBA
surveys. Their star formation is driven predominantly by strong tidal
interactions and mergers of galaxies. This leads to the creation of spheroidal
stellar systems, which may act as the seeds for disk formation as gas infalls.
We predict the present-day baryonic mass in bulges and halos is comparable to
that in disks. From observations of the extra-galactic background, the model
predicts that the vast majority of star formation in the Universe occurs at
z<5.Comment: 23 pages including 9 figures. To appear in ApJ. Model results
available electronically at http://astro.berkeley.edu/~jt/irmodel.htm
Feasibility as feedstock of the cyanobacterium Chroococcidiopsis sp. 029 cultivated with urine-supplemented moon and mars regolith simulants
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