3,065 research outputs found
A density--functional study of interfacial properties of colloid--polymer mixtures
Interfacial properties of colloid--polymer mixtures are examined within an
effective one--component representation, where the polymer degrees of freedom
are traced out, leaving a fluid of colloidal particles interacting via
polymer--induced depletion forces. Restriction is made to zero, one and
two--body effective potentials, and a free energy functional is used which
treats colloid excluded volume correlations within Rosenfeld's Fundamental
Measure Theory, and depletion--induced attraction within first--order
perturbation theory. This functional allows a consistent treatment of both
ideal and interacting polymers. The theory is applied to surface properties
near a hard wall, to the depletion interaction between two walls, and to the
fluid--fluid interface of demixed colloid--polymer mixtures. The results of the
present theory compare well with predictions of a fully two--component
representation of mixtures of colloids and ideal polymers (the Asakura--Oosawa
model), and allow a systematic investigation of the effects of polymer--polymer
interactions on interfacial properties. In particular, the wall surface tension
is found to be significantly larger for interacting than for ideal polymers,
while the opposite trend is predicted for the fluid--fluid interfacial tension.Comment: submitted to J. Phys. Chem. B, special issue in honour of David
Chandle
Millimetre continuum observations of comet C/2009 P1 (Garradd)
Little is known about the physical properties of the nuclei of Oort cloud
comets. Measuring the thermal emission of a nucleus is one of the few means for
deriving its size and constraining some of its thermal properties. We attempted
to measure the nucleus size of the Oort cloud comet C/2009 P1 (Garradd). We
used the Plateau de Bure Interferometer to measure the millimetric thermal
emission of this comet at 157 GHz (1.9 mm) and 266 GHz (1.1 mm). Whereas the
observations at 266 GHz were not usable due to bad atmospheric conditions, we
derived a 3-sigma upper limit on the comet continuum emission of 0.41 mJy at
157 GHz. Using a thermal model for a spherical nucleus with standard thermal
parameters, we found an upper limit of 5.6 km for the radius. The dust
contribution to our signal is estimated to be negligible. Given the water
production rates measured for this comet and our upper limit, we estimated that
Garradd was very active, with an active fraction of its nucleus larger than
50%.Comment: Accepted for publication in Astronomy & Astrophysics. 5 pages, 2
figure
The properties of asteroid (2867) Steins from Spitzer observations and OSIRIS shape reconstruction
We report on the thermal properties and composition of asteroid (2867) Steins
derived from an analysis of new Spitzer Space Telescope (SST) observations
performed in March 2008, in addition to previously published SST observations
performed in November 2005. We consider the three-dimensional shape model and
photometric properties derived from OSIRIS images obtained during the flyby of
the Rosetta spacecraft in September 2008, which we combine with a thermal model
to properly interpret the observed SST thermal light curve and spectral energy
distributions. We obtain a thermal inertia in the range 100\pm50 JK-1m-2s-1/2
and a beaming factor (roughness) in the range 0.7-1.0. We confirm that the
infrared emissivity of Steins is consistent with an enstatite composition. The
November 2005 SST thermal light curve is most reliably interpreted by assuming
inhomogeneities in the thermal properties of the surface, with two different
regions of slightly different roughness, as observed on other small bodies,
such as the nucleus of comet 9P/Tempel 1. Our results emphasize that the shape
model is important to an accurate determination of the thermal inertia and
roughness. Finally, we present temperature maps of Steins, as seen by Rosetta
during its flyby, and discuss the interpretation of the observations performed
by the VIRTIS and MIRO instruments
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Characterization of the Subsurface of 67P/Churyumov-Gerasimenko's Abydos Site
We investigate the structure of the subsurface of the Abydos site using a cometary nucleus model with parameters adapted to comet 67P/Churyumov-Gerasimenko and the Abydos landing site. We aim to compare the production rates derived from our model with those of the main molecules measured by Ptolemy. This will allow us to retrieve the depths at which the different molecules still exist in solid form
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Spatial and temporal variations of the seasonal sea level cycle in the northwest Pacific
The seasonal sea level variations observed from tide gauges over 1900-2013 and gridded satellite altimeter product AVISO over 1993-2013 in the northwest Pacific have been explored. The seasonal cycle is able to explain 60-90% of monthly sea level variance in the marginal seas, while it explains less than 20% of variance in the eddy-rich regions. The maximum annual and semi-annual sea level cycles (30cm and 6cm) are observed in the north of the East China Sea and the west of the South China Sea respectively. AVISO was found to underestimate the annual amplitude by 25% compared to tide gauge estimates along the coasts of China and Russia.
The forcing for the seasonal sea level cycle was identified. The atmospheric pressure and the steric height produce 8-12cm of the annual cycle in the middle continental shelf and in the Kuroshio Current regions separately. The removal of the two attributors from total sea level permits to identify the sea level residuals that still show significant seasonality in the marginal seas. Both nearby wind stress and surface currents can explain well the long-term variability of the seasonal sea level cycle in the marginal seas and the tropics because of their influence on the sea level residuals. Interestingly, the surface currents are a better descriptor in the areas where the ocean currents are known to be strong. Here, they explain 50-90% of inter-annual variability due to the strong links between the steric height and the large-scale ocean currents
Activity distribution of comet 67P/Churyumov-Gerasimenko from combined measurements of non-gravitational forces and torques
Aims. Understanding the activity is vital for deciphering the structure, formation, and evolution of comets. We investigate models of cometary activity by comparing them to the dynamics of 67P/Churyumov-Gerasimenko.
Methods. We matched simple thermal models of water activity to the combined Rosetta datasets by fitting to the total outgassing rate and four components of the outgassing induced non-gravitational force and torque, with a final manual adjustment of the model parameters to additionally match the other two torque components. We parametrised the thermal model in terms of a distribution of relative activity over the surface of the comet, and attempted to link this to different terrain types. We also tested a more advanced thermal model based on a pebble structure.
Results. We confirm a hemispherical dichotomy and non-linear water outgassing response to insolation. The southern hemisphere of the comet and consolidated terrain show enhanced activity relative to the northern hemisphere and dust-covered, unconsolidated terrain types, especially at perihelion. We further find that the non-gravitational torque is especially sensitive to the activity distribution, and to fit the pole-axis orientation in particular, activity must be concentrated (in excess of the already high activity in the southern hemisphere and consolidated terrain) around the south pole and on the body and neck of the comet over its head. This is the case for both the simple thermal model and the pebble-based model. Overall, our results show that water activity cannot be matched by a simple model of sublimating surface ice driven by the insolation alone, regardless of the surface distribution, and that both local spatial and temporal variations are needed to fit the data.
Conclusions. Fully reconciling the Rosetta outgassing, torque, and acceleration data requires a thermal model that includes both diurnal and seasonal effects and also structure with depth (dust layers or ice within pebbles). This shows that cometary activity is complex. Nonetheless, non-gravitational dynamics provides a useful tool for distinguishing between different thermophysical models and aids our understanding
Angular Correlations in Internal Pair Conversion of Aligned Heavy Nuclei
We calculate the spatial correlation of electrons and positrons emitted by
internal pair conversion of Coulomb excited nuclei in heavy ion collisions. The
alignment or polarization of the nucleus results in an anisotropic emission of
the electron-positron pairs which is closely related to the anisotropic
emission of -rays. However, the angular correlation in the case of
internal pair conversion exhibits diverse patterns. This might be relevant when
investigating atomic processes in heavy-ion collisions performed at the Coulomb
barrier.Comment: 27 pages + 6 eps figures, uses revtex.sty and epsf.sty,
tar-compressed and uuencoded with uufile
Performance of a Tungsten-Cerium Fluoride Sampling Calorimeter in High-Energy Electron Beam Tests
A prototype for a sampling calorimeter made out of cerium fluoride crystals
interleaved with tungsten plates, and read out by wavelength-shifting fibres,
has been exposed to beams of electrons with energies between 20 and 150 GeV,
produced by the CERN Super Proton Synchrotron accelerator complex. The
performance of the prototype is presented and compared to that of a Geant4
simulation of the apparatus. Particular emphasis is given to the response
uniformity across the channel front face, and to the prototype's energy
resolution.Comment: 6 pages, 6 figures, Submitted to NIM
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