282 research outputs found
Phase Transition in a Stochastic Forest Fire Model and Effects of the Definition of Neighbourhood
We present results on a stochastic forest fire model, where the influence of
the neighbour trees is treated in a more realistic way than usual and the
definition of neighbourhood can be tuned by an additional parameter.
This model exhibits a surprisingly sharp phase transition which can be
shifted by redefinition of neighbourhood. The results can also be interpreted
in terms of disease-spreading and are quite unsettling from the epidemologist's
point of view, since variation of one crucial parameter only by a few percent
can result in the change from endemic to epidemic behaviour.Comment: 23 pages, 13 figure
Heterogeneous Pd catalysts as emulsifiers in Pickering emulsions for integrated multistep synthesis in flow chemistry
Within the “Compartmentalised Smart Factory” approach of the ONE-FLOW project the implementation of different catalysts in “compartments” provided by Pickering emulsions and their application in continuous flow is targeted. We present here the development of heterogeneous Pd-catalysts that are ready to be used in combination with biocatalysts for catalytic cascade syntheses of active pharmaceutical ingredients (APIs). In particular, we focus on the application of the catalytic systems for Suzuki-Miyaura cross coupling reactions, which is the key step in the syntheses of the targeted APIs valsartan and sacubitril. An immobilised enzyme will accomplish the final product formation via hydrolysis. In order to create large interfacial area for the catalytic reactions and to keep the reagents separated until required, the catalyst particles are used to stabilise Pickering emulsions of oil and water. A set of Ce-Sn-Pd-oxides with the molecular formula Ce0.99-xSnxPd0.01O2-(x= 0-0.99) has been prepared utilising a simple single-step solution combustion method. The high applicability of the catalysts for different functional groups and their minimal leaching behaviour is demonstrated with various Suzuki-Miyaura cross coupling reactions in batch as well as in continuous flow employing the so-called “Plug & Play reactor”. Finally, we demonstrate the use of these particles as the sole emulsifier of oil + water emulsions for a range of oils
Self-consistent modelling of Mercury’s surface composition and exosphere by solar wind sputtering
A Monte-Carlo model of exospheres was extended by treating the solar wind ion induced sputtering
process, quantitatively in a self-consistent way starting with the actual release of particles from the
mineral surface of Mercury. Mercury is a body without a significant atmosphere, thus, the surface is
effected by different processes that are mainly related to the radiation and plasma environment of
the Sun and to micrometeorites, which are delivered to Mercury’s surface. In such a case it can be
assumed that the composition of Mercury’s thin collisionless atmosphere, the exosphere, is related
to the composition of the planetary crustal materials. If so, then inferences regarding the bulk
chemistry of the planet can be made from a study of atoms and molecules in the exosphere after
they are released from the mineral surface by a variety of release processes. One difficult challenge
is the identification of the main source of some elements like H, He, Na or K. Generally it is
believed that H and He come primarily from the solar wind, while Na and K originate from
volatilized materials partitioned between Mercury’s crust and impacts from meteorites. Besides the
before mentioned elements corresponding to spectroscopic observations and experiments with soil
analogues, other elements such as O, Na, Mg, Al, Si, P, S, K, Ca, Ti, Cr, Fe, Ni, Zn, OH should also
be related with Mercury’s surface soils (Wurz et al., 2010, and references therein). Based on
available observational data and literature data we established a global model for the surface
mineralogy of Mercury and from that derived the average elemental composition of the surface.
Compositional data analysis has been employed for Mercury’s surface minerals recently by
(Sprague et al., 2009). In these cases the applied method was based on simple correlation methods,
which do not exploit the full potential of the available data. In addition, the closed nature of
compositional data, i.e., the assumption that component concentrations have to sum up to 100% in
an analysis, bears important implications for the statistical analysis of compositional data, which do
not seem to have been sufficiently appreciated until now. To investigate the default of the classical
additive analysis method our research group applied recently a more realistic multiplicative method
(Aitchison, 1986) based on the Euclidean space geometry of the simplex (see the chapter Elements
of simplicial linear algebra and geometry). Our recent results presented in detail in Wurz et al.,
(2010) for Mercury will be discussed. This model serves as a tool to estimate densities of species in
the exosphere depending on the release mechanism and the associated physical parameters
quantitatively describing the particle release from the surface
On the Possibility of Measuring the Gravitomagnetic Clock Effect in an Earth Space-Based Experiment
In this paper the effect of the post-Newtonian gravitomagnetic force on the
mean longitudes of a pair of counter-rotating Earth artificial satellites
following almost identical circular equatorial orbits is investigated. The
possibility of measuring it is examined. The observable is the difference of
the times required to in passing from 0 to 2 for both senses of
motion. Such gravitomagnetic time shift, which is independent of the orbital
parameters of the satellites, amounts to 5 s for Earth; it is
cumulative and should be measured after a sufficiently high number of
revolutions. The major limiting factors are the unavoidable imperfect
cancellation of the Keplerian periods, which yields a constraint of 10
cm in knowing the difference between the semimajor axes of the satellites,
and the difference of the inclinations of the orbital planes which, for
, should be less than . A pair of spacecrafts
endowed with a sophisticated intersatellite tracking apparatus and drag-free
control down to 10 cm s Hz level might allow to meet
the stringent requirements posed by such a mission.Comment: LaTex2e, 22 pages, no tables, 1 figure, 38 references. Final version
accepted for publication in Classical and Quantum Gravit
Observation of Fragile-to-Strong Dynamic Crossover in Protein Hydration Water
At low temperatures proteins exist in a glassy state, a state which has no
conformational flexibility and shows no biological functions. In a hydrated
protein, at and above 220 K, this flexibility is restored and the protein is
able to sample more conformational sub-states, thus becomes biologically
functional. This 'dynamical' transition of protein is believed to be triggered
by its strong coupling with the hydration water, which also shows a similar
dynamic transition. Here we demonstrate experimentally that this sudden switch
in dynamic behavior of the hydration water on lysozyme occurs precisely at 220
K and can be described as a Fragile-to-Strong dynamic crossover (FSC). At FSC,
the structure of hydration water makes a transition from predominantly
high-density (more fluid state) to low-density (less fluid state) forms derived
from existence of the second critical point at an elevated pressure.Comment: 6 pages (Latex), 4 figures (Postscript
The Hydrogen Exospheric Density Profile Measured with ASPERA-3/NPD
We have evaluated the Lyman-α limb emission from the exospheric hydrogen of Mars measured by the neutral particle detector of the ASPERA-3 instrument on Mars Express in 2004 at low solar activity (solar activity index = 42, F10.7=100). We derive estimates for the hydrogen exobase density, n H = 1010 m−3, and for the apparent temperature, T > 600 K. We conclude that the limb emission measurement is dominated by a hydrogen component that is considerably hotter than the bulk temperature at the exobase. The derived values for the exosphere density and temperature are compared with similar measurements done by the Mariner space probes in the 1969. The values found with Mars Express and Mariner data are brought in a broader context of exosphere models including the possibility of having two hydrogen components in the Martian exosphere. The present observation of the Martian hydrogen exosphere is the first one at high altitudes during low solar activity, and shows that for low solar activity exospheric densities are not higher than for high solar activit
The twin paradox and Mach's principle
The problem of absolute motion in the context of the twin paradox is
discussed. It is shown that the various versions of the clock paradox feature
some aspects which Mach might have been appreciated. However, the ultimate
cause of the behavior of the clocks must be attributed to the autonomous status
of spacetime, thereby proving the relational program advocated by Mach as
impracticable.Comment: Latex2e, 11 pages, 6 figures, 33 references, no tables. Accepted for
publication in The European Physical Journal PLUS (EPJ PLUS
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