1,248 research outputs found
Adsorption of Line Segments on a Square Lattice
We study the deposition of line segments on a two-dimensional square lattice.
The estimates for the coverage at jamming obtained by Monte-Carlo simulations
and by -order time-series expansion are successfully compared. The
non-trivial limit of adsorption of infinitely long segments is studied, and the
lattice coverage is consistently obtained using these two approaches.Comment: 19 pages in Latex+5 postscript files sent upon request ; PTB93_
Automatic service categorisation through machine learning in emergent middleware
The modern environment of mobile, pervasive, evolving services presents a great challenge to traditional solutions for enabling interoperability. Automated solutions appear to be the only way to achieve interoperability with the needed level of flexibility and scalability. While necessary, the techniques used to determine compatibility, as a precursor to interaction, come at a substantial computational cost, especially when checks are performed between systems in unrelated domains. To overcome this, we apply machine learning to extract high-level functionality information through text categorisation of a system's interface description. This categorisation allows us to restrict the scope of compatibility checks, giving an overall performance gain when conducting matchmaking between systems. We have evaluated our approach on a corpus of web service descriptions, where even with moderate categorisation accuracy, a substantial performance benefit can be found. This in turn improves the applicability of our overall approach for achieving interoperability in the Connect project
X-ray line spectrometry in experiments with the aluminium Z-pinch
X-ray line spectrometry with temporal resolution was developed for registration of [He]- and [H]-like aluminium ions spectrum. It was chosen a scheme with scintillator converting X-ray spectrum into the visible image, which was transferred through the flexible optical fiber to the entrance slit of the streak camera. In Z-pinch experiment on the high current S-300 generator the aluminium line spectrum was registered with nanosecond time resolution. The simultaneous appearance of [He]- and [H]-like aluminium ions radiation was observed, that is the evidence of high electron temperature existence in the plasma for a long time before the main part of the load mass comes to the axis. The noticeably changing of radiating plasma parameters was found after the computer treatment of line spectra: the electron concentration is varied in five times ((3âŠ14)Ă10^19 cm^-3), electron temperature in three times (0.3âŠ1 keV), ion temperature in five times (20âŠ100 keV), â during 50 ns. The great difference between the electron and ion temperature holds during all radiation time and demonstrates the ineffective energy transfer from the kinetic energy of ions to electron.Đ Đ°Đ·ŃĐ°Đ±ĐŸŃĐ°ĐœĐ° ĐŒĐ”ŃĐŸĐŽĐžĐșĐ° ĐŽĐ»Ń ŃДгОŃŃŃĐ°ŃОО Ń ĐČŃĐ”ĐŒĐ”ĐœĐœŃĐŒ ŃĐ°Đ·ŃĐ”ŃĐ”ĐœĐžĐ”ĐŒ ŃĐ”ĐœŃĐłĐ”ĐœĐŸĐČŃĐșĐžŃ
Đ»ĐžĐœĐžĐč [He]- Đž [H]-ĐżĐŸĐŽĐŸĐ±ĐœŃŃ
ĐžĐŸĐœĐŸĐČ Đ°Đ»ŃĐŒĐžĐœĐžŃ. Đ Đ”ĐœŃĐłĐ”ĐœĐŸĐČŃĐșĐžĐč ŃпДĐșŃŃ ĐżŃĐ”ĐŸĐ±ŃĐ°Đ·ĐŸĐČŃĐČĐ°Đ»ŃŃ Ń ĐżĐŸĐŒĐŸŃŃŃ ŃŃĐžĐœŃОллŃŃĐŸŃĐ° ĐČ ĐČĐžĐŽĐžĐŒĐŸĐ” ĐžĐ·ĐŸĐ±ŃĐ°Đ¶Đ”ĐœĐžĐ”, ĐșĐŸŃĐŸŃĐŸĐ” пДŃĐ”ĐœĐŸŃĐžĐ»ĐŸŃŃ ĐłĐžĐ±ĐșĐžĐŒ ŃĐČĐ”ŃĐŸĐČĐŸĐŽĐŸĐŒ ĐœĐ° ĐČŃ
ĐŸĐŽĐœŃŃ ŃĐ”Đ»Ń ŃлДĐșŃŃĐŸĐœĐœĐŸ-ĐŸĐżŃĐžŃĐ”ŃĐșĐŸĐłĐŸ ĐżŃĐ”ĐŸĐ±ŃĐ°Đ·ĐŸĐČĐ°ŃДлŃ. РДгОŃŃŃĐ°ŃĐžŃ ŃпДĐșŃŃĐ° ĐżŃĐŸĐČĐŸĐŽĐžĐ»Đ°ŃŃ Ń ĐœĐ°ĐœĐŸŃĐ”ĐșŃĐœĐŽĐœŃĐŒ ŃĐ°Đ·ŃĐ”ŃĐ”ĐœĐžĐ”ĐŒ ĐČ ŃĐșŃпДŃĐžĐŒĐ”ĐœŃĐ°Ń
Ń Z-ĐżĐžĐœŃĐ”ĐŒ ĐœĐ° ŃОлŃĐœĐŸŃĐŸŃĐœĐŸĐŒ ĐłĐ”ĐœĐ”ŃĐ°ŃĐŸŃĐ” ĐĄ-300. ĐаблŃĐŽĐ°Đ»ĐŸŃŃ ĐŸĐŽĐœĐŸĐČŃĐ”ĐŒĐ”ĐœĐœĐŸĐ” ĐżĐŸŃĐČĐ»Đ”ĐœĐžĐ” Đ»ĐžĐœĐžĐč [He]- Đž [H]-ĐżĐŸĐŽĐŸĐ±ĐœŃŃ
ĐžĐŸĐœĐŸĐČ Đ°Đ»ŃĐŒĐžĐœĐžŃ, ŃŃĐŸ ŃĐČĐ»ŃĐ”ŃŃŃ ŃĐČОЎДŃДлŃŃŃĐČĐŸĐŒ ĐœĐ°Đ»ĐžŃĐžŃ ĐČŃŃĐŸĐșĐŸĐč ŃлДĐșŃŃĐŸĐœĐœĐŸĐč ŃĐ”ĐŒĐżĐ”ŃĐ°ŃŃŃŃ ĐČ ĐżĐ»Đ°Đ·ĐŒĐ” Đ·Đ°ĐŽĐŸĐ»ĐłĐŸ ĐŽĐŸ ĐŒĐŸĐŒĐ”ĐœŃĐ° ĐżŃĐžŃ
ĐŸĐŽĐ° Đș ĐŸŃĐž ĐŸŃĐœĐŸĐČĐœĐŸĐč ĐŒĐ°ŃŃŃ Z-ĐżĐžĐœŃĐ°. ĐĐŸĐŒĐżŃŃŃĐ”ŃĐœĐ°Ń ĐŸĐ±ŃĐ°Đ±ĐŸŃĐșĐ° ŃпДĐșŃŃĐŸĐČ ĐČŃŃĐČОла Đ·ĐœĐ°ŃĐžŃДлŃĐœŃĐ” ĐžĐ·ĐŒĐ”ĐœĐ”ĐœĐžŃ ĐżĐ°ŃĐ°ĐŒĐ”ŃŃĐŸĐČ ĐżĐ»Đ°Đ·ĐŒŃ ĐČ ĐżŃĐŸŃĐ”ŃŃĐ” ŃжаŃĐžŃ: ĐșĐŸĐœŃĐ”ĐœŃŃĐ°ŃОО ĐČ ĐżŃŃŃ ŃĐ°Đ· ((3âŠ14)Ă10^19 ŃĐŒ^-3), ŃлДĐșŃŃĐŸĐœĐœĐŸĐč ŃĐ”ĐŒĐżĐ”ŃĐ°ŃŃŃŃ ĐČ ŃŃĐž (0.3âŠ1 ĐșŃĐ), ĐžĐŸĐœĐœĐŸĐč ŃĐ”ĐŒĐżĐ”ŃĐ°ŃŃŃŃ ĐČ ĐżŃŃŃ ŃĐ°Đ· (20âŠ100 ĐșŃĐ) â Đ·Đ° 50 ĐœŃ. ĐĐŸĐ»ŃŃĐŸĐč ŃĐ°Đ·ŃŃĐČ ĐŒĐ”Đ¶ĐŽŃ ĐžĐŸĐœĐœĐŸĐč Đž ŃлДĐșŃŃĐŸĐœĐœĐŸĐč ŃĐ”ĐŒĐżĐ”ŃĐ°ŃŃŃĐ°ĐŒĐž ĐŽĐ”ĐŒĐŸĐœŃŃŃĐžŃŃĐ”Ń ĐœĐ”ŃŃŃĐ”ĐșŃĐžĐČĐœĐŸŃŃŃ ĐżĐ”ŃДЎаŃĐž ŃĐœĐ”ŃгОО ĐŸŃ ĐžĐŸĐœĐŸĐČ Đș ŃлДĐșŃŃĐŸĐœĐ°ĐŒ.Đ ĐŸĐ·ŃĐŸĐ±Đ»Đ”ĐœĐŸ ĐŒĐ”ŃĐŸĐŽĐžĐșŃ ĐŽĐ»Ń ŃĐ”ŃŃŃŃĐ°ŃŃŃ Đ· ŃĐ°ŃĐŸĐČĐžĐŒ ĐŽĐŸĐ·ĐČĐŸĐ»ĐŸĐŒ ŃĐ”ĐœŃĐłĐ”ĐœŃĐČŃŃĐșĐžŃ
Đ»ŃĐœŃĐč [He]- Ń [H]-ĐżĐŸĐŽŃĐ±ĐœĐžŃ
ŃĐŸĐœŃĐČ Đ°Đ»ŃĐŒŃĐœŃŃ. Đ Đ”ĐœŃĐłĐ”ĐœŃĐČŃŃĐșĐžĐč ŃпДĐșŃŃ ĐżĐ”ŃĐ”ŃĐČĐŸŃŃĐČĐ°ĐČŃŃ Đ·Đ° ĐŽĐŸĐżĐŸĐŒĐŸĐłĐŸŃ ŃŃĐžĐœŃОллŃŃĐŸŃĐ° Ń ĐČĐžĐŽĐžĐŒĐ” Đ·ĐŸĐ±ŃĐ°Đ¶Đ”ĐœĐœŃ, ŃĐŸ пДŃĐ”ĐœĐŸŃĐžĐ»ĐŸŃŃ ĐłĐœŃŃĐșĐžĐŒ ŃĐČŃŃĐ»ĐŸĐČĐŸĐŽĐŸĐŒ ĐœĐ° ĐČŃ
ŃĐŽĐœŃ ŃŃĐ»ĐžĐœŃ Đ”Đ»Đ”ĐșŃŃĐŸĐœĐœĐŸ-ĐŸĐżŃĐžŃĐœĐŸĐłĐŸ пДŃĐ”ŃĐČĐŸŃŃĐČĐ°ŃĐ°. Đ Đ”ŃŃŃŃĐ°ŃŃŃ ŃпДĐșŃŃĐ° ĐżŃĐŸĐČĐŸĐŽĐžĐ»Đ°ŃŃ Đ· ĐœĐ°ĐœĐŸŃĐ”ĐșŃĐœĐŽĐœĐžĐŒ ĐŽĐŸĐ·ĐČĐŸĐ»ĐŸĐŒ ĐČ Đ”ĐșŃпДŃĐžĐŒĐ”ĐœŃĐ°Ń
Đ· Z-ĐżŃĐœŃĐ”ĐŒ ĐœĐ° ĐżĐŸŃŃĐ¶ĐœĐŸŃŃŃŃĐŒĐŸĐČĐŸĐŒŃ ĐłĐ”ĐœĐ”ŃĐ°ŃĐŸŃŃ ĐĄ-300. ĐĄĐżĐŸŃŃĐ”ŃŃгалаŃŃ ĐŸĐŽĐœĐŸŃĐ°ŃĐœĐ° ĐżĐŸŃĐČĐ° Đ»ŃĐœŃĐč [He]- Ń [H]-ĐżĐŸĐŽŃĐ±ĐœĐžŃ
ŃĐŸĐœŃĐČ Đ°Đ»ŃĐŒŃĐœŃŃ, ŃĐŸ Ń ŃĐČŃĐŽŃĐ”ĐœĐœŃĐŒ ĐœĐ°ŃĐČĐœĐŸŃŃŃ ĐČĐžŃĐŸĐșĐŸŃ Đ”Đ»Đ”ĐșŃŃĐŸĐœĐœĐŸŃ ŃĐ”ĐŒĐżĐ”ŃĐ°ŃŃŃĐž ĐČ ĐżĐ»Đ°Đ·ĐŒŃ Đ·Đ°ĐŽĐŸĐČĐłĐŸ ĐŽĐŸ ĐŒĐŸĐŒĐ”ĐœŃŃ ĐżŃĐžŃ
ĐŸĐŽŃ ĐŽĐŸ ĐŸŃŃ ĐŸŃĐœĐŸĐČĐœĐŸŃ ĐŒĐ°ŃĐž Z-ĐżŃĐœŃĐ°. ĐĐŸĐŒĐż'ŃŃĐ”ŃĐœĐ° ĐŸĐ±ŃĐŸĐ±ĐșĐ° ŃпДĐșŃŃŃĐČ ĐČĐžŃĐČОла Đ·ĐœĐ°ŃĐœŃ Đ·ĐŒŃĐœĐž паŃĐ°ĐŒĐ”ŃŃŃĐČ ĐżĐ»Đ°Đ·ĐŒĐž ĐČ ĐżŃĐŸŃĐ”ŃŃ ŃŃĐžŃĐșŃ: ĐșĐŸĐœŃĐ”ĐœŃŃĐ°ŃŃŃ ĐČ Đż'ŃŃŃ ŃĐ°Đ·ŃĐČ ((3...14)Ă10^19ŃĐŒ^-3), ДлДĐșŃŃĐŸĐœĐœĐŸŃ ŃĐ”ĐŒĐżĐ”ŃĐ°ŃŃŃĐž ĐČ ŃŃĐž (0.3...1ĐșĐ”Đ), ŃĐŸĐœĐœĐŸŃ ŃĐ”ĐŒĐżĐ”ŃĐ°ŃŃŃĐž ĐČ Đż'ŃŃŃ ŃĐ°Đ·ŃĐČ (20...100 ĐșĐ”Đ) â Đ·Đ° 50 ĐœŃ. ĐДлОĐșĐžĐč ŃĐŸĐ·ŃĐžĐČ ĐŒŃж ŃĐŸĐœĐœĐŸŃ Đč ДлДĐșŃŃĐŸĐœĐœĐŸŃ ŃĐ”ĐŒĐżĐ”ŃĐ°ŃŃŃĐ°ĐŒĐž ĐŽĐ”ĐŒĐŸĐœŃŃŃŃŃ ĐœĐ”Đ”ŃĐ”ĐșŃĐžĐČĐœŃŃŃŃ ĐżĐ”ŃДЎаŃŃ Đ”ĐœĐ”ŃĐłŃŃ ĐČŃĐŽ ŃĐŸĐœŃĐČ ĐŽĐŸ ДлДĐșŃŃĐŸĐœŃĐČ
Magnetic fields in supernova remnants and pulsar-wind nebulae
We review the observations of supernova remnants (SNRs) and pulsar-wind
nebulae (PWNe) that give information on the strength and orientation of
magnetic fields. Radio polarimetry gives the degree of order of magnetic
fields, and the orientation of the ordered component. Many young shell
supernova remnants show evidence for synchrotron X-ray emission. The spatial
analysis of this emission suggests that magnetic fields are amplified by one to
two orders of magnitude in strong shocks. Detection of several remnants in TeV
gamma rays implies a lower limit on the magnetic-field strength (or a
measurement, if the emission process is inverse-Compton upscattering of cosmic
microwave background photons). Upper limits to GeV emission similarly provide
lower limits on magnetic-field strengths. In the historical shell remnants,
lower limits on B range from 25 to 1000 microGauss. Two remnants show
variability of synchrotron X-ray emission with a timescale of years. If this
timescale is the electron-acceleration or radiative loss timescale, magnetic
fields of order 1 mG are also implied. In pulsar-wind nebulae, equipartition
arguments and dynamical modeling can be used to infer magnetic-field strengths
anywhere from about 5 microGauss to 1 mG. Polarized fractions are considerably
higher than in SNRs, ranging to 50 or 60% in some cases; magnetic-field
geometries often suggest a toroidal structure around the pulsar, but this is
not universal. Viewing-angle effects undoubtedly play a role. MHD models of
radio emission in shell SNRs show that different orientations of upstream
magnetic field, and different assumptions about electron acceleration, predict
different radio morphology. In the remnant of SN 1006, such comparisons imply a
magnetic-field orientation connecting the bright limbs, with a non-negligible
gradient of its strength across the remnant.Comment: 20 pages, 24 figures; to be published in SpSciRev. Minor wording
change in Abstrac
AltitudeOmics: The Integrative Physiology of Human Acclimatization to Hypobaric Hypoxia and Its Retention upon Reascent.
An understanding of human responses to hypoxia is important for the health of millions of people worldwide who visit, live, or work in the hypoxic environment encountered at high altitudes. In spite of dozens of studies over the last 100 years, the basic mechanisms controlling acclimatization to hypoxia remain largely unknown. The AltitudeOmics project aimed to bridge this gap. Our goals were 1) to describe a phenotype for successful acclimatization and assess its retention and 2) use these findings as a foundation for companion mechanistic studies. Our approach was to characterize acclimatization by measuring changes in arterial oxygenation and hemoglobin concentration [Hb], acute mountain sickness (AMS), cognitive function, and exercise performance in 21 subjects as they acclimatized to 5260 m over 16 days. We then focused on the retention of acclimatization by having subjects reascend to 5260 m after either 7 (nâ=â14) or 21 (nâ=â7) days at 1525 m. At 16 days at 5260 m we observed: 1) increases in arterial oxygenation and [Hb] (compared to acute hypoxia: PaO2 rose 9±4 mmHg to 45±4 while PaCO2 dropped a further 6±3 mmHg to 21±3, and [Hb] rose 1.8±0.7 g/dL to 16±2 g/dL; 2) no AMS; 3) improved cognitive function; and 4) improved exercise performance by 8±8% (all changes p<0.01). Upon reascent, we observed retention of arterial oxygenation but not [Hb], protection from AMS, retention of exercise performance, less retention of cognitive function; and noted that some of these effects lasted for 21 days. Taken together, these findings reveal new information about retention of acclimatization, and can be used as a physiological foundation to explore the molecular mechanisms of acclimatization and its retention
Formation of Nanopits in Si Capping Layers on SiGe Quantum Dots
In-situ annealing at a high temperature of 640°C was performed for a low temperature grown Si capping layer, which was grown at 300°C on SiGe self-assembled quantum dots with a thickness of 50 nm. Square nanopits, with a depth of about 8 nm and boundaries along â©110âȘ, are formed in the Si capping layer after annealing. Cross-sectional transmission electron microscopy observation shows that each nanopit is located right over one dot with one to one correspondence. The detailed migration of Si atoms for the nanopit formation is revealed by in-situ annealing at a low temperature of 540°C. The final well-defined profiles of the nanopits indicate that both strain energy and surface energy play roles during the nanopit formation, and the nanopits are stable at 640°C. A subsequent growth of Ge on the nanopit-patterned surface results in the formation of SiGe quantum dot molecules around the nanopits
Measurement of the Charged Multiplicities in b, c and Light Quark Events from Z0 Decays
Average charged multiplicities have been measured separately in , and
light quark () events from decays measured in the SLD experiment.
Impact parameters of charged tracks were used to select enriched samples of
and light quark events, and reconstructed charmed mesons were used to select
quark events. We measured the charged multiplicities:
,
, from
which we derived the differences between the total average charged
multiplicities of or quark events and light quark events: and . We compared
these measurements with those at lower center-of-mass energies and with
perturbative QCD predictions. These combined results are in agreement with the
QCD expectations and disfavor the hypothesis of flavor-independent
fragmentation.Comment: 19 pages LaTex, 4 EPS figures, to appear in Physics Letters
Heavy quarkonium: progress, puzzles, and opportunities
A golden age for heavy quarkonium physics dawned a decade ago, initiated by
the confluence of exciting advances in quantum chromodynamics (QCD) and an
explosion of related experimental activity. The early years of this period were
chronicled in the Quarkonium Working Group (QWG) CERN Yellow Report (YR) in
2004, which presented a comprehensive review of the status of the field at that
time and provided specific recommendations for further progress. However, the
broad spectrum of subsequent breakthroughs, surprises, and continuing puzzles
could only be partially anticipated. Since the release of the YR, the BESII
program concluded only to give birth to BESIII; the -factories and CLEO-c
flourished; quarkonium production and polarization measurements at HERA and the
Tevatron matured; and heavy-ion collisions at RHIC have opened a window on the
deconfinement regime. All these experiments leave legacies of quality,
precision, and unsolved mysteries for quarkonium physics, and therefore beg for
continuing investigations. The plethora of newly-found quarkonium-like states
unleashed a flood of theoretical investigations into new forms of matter such
as quark-gluon hybrids, mesonic molecules, and tetraquarks. Measurements of the
spectroscopy, decays, production, and in-medium behavior of c\bar{c}, b\bar{b},
and b\bar{c} bound states have been shown to validate some theoretical
approaches to QCD and highlight lack of quantitative success for others. The
intriguing details of quarkonium suppression in heavy-ion collisions that have
emerged from RHIC have elevated the importance of separating hot- and
cold-nuclear-matter effects in quark-gluon plasma studies. This review
systematically addresses all these matters and concludes by prioritizing
directions for ongoing and future efforts.Comment: 182 pages, 112 figures. Editors: N. Brambilla, S. Eidelman, B. K.
Heltsley, R. Vogt. Section Coordinators: G. T. Bodwin, E. Eichten, A. D.
Frawley, A. B. Meyer, R. E. Mitchell, V. Papadimitriou, P. Petreczky, A. A.
Petrov, P. Robbe, A. Vair
Prostate cancer and Hedgehog signalling pathway
[Abstract] The Hedgehog (Hh) family of intercellular signalling proteins have come to be recognised as key mediators in many fundamental processes in embryonic development. Their activities are central to the growth, patterning and morphogenesis of many different regions within the bodies of vertebrates. In some contexts, Hh signals act as morphogens in the dose-dependent induction of distinct cell fates within a target field, in others as mitogens in the regulation of cell proliferation or as inducing factors controlling the form of a developing organ. These diverse functions of Hh proteins raise many intriguing questions about their mode of action. Various studies have now demonstrated the function of Hh signalling in the control of cell proliferation, especially for stem cells and stem-like progenitors. Abnormal activation of the Hh pathway has been demonstrated in a variety of human tumours. Hh pathway activity in these tumours is required for cancer cell proliferation and tumour growth. Recent studies have uncovered the role for Hh signalling in advanced prostate cancer and demonstrated that autocrine signalling by tumour cells is required for proliferation, viability and invasive behaviour. Thus, Hh signalling represents a novel pathway in prostate cancer that offers opportunities for prognostic biomarker development, drug targeting and therapeutic response monitoring
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