3,492 research outputs found
Elastic heterogeneity of soft random solids
Spatial heterogeneity in the elastic properties of soft random solids is
investigated via a two-pronged approach. First, a nonlocal phenomenological
model for the elastic free energy is examined. This features a quenched random
kernel, which induces randomness in the residual stress and Lame coefficients.
Second, a semi-microscopic model network is explored using replica statistical
mechanics. The Goldstone fluctuations of the semi-microscopic model are shown
to reproduce the phenomenological model, and via this correspondence the
statistical properties of the residual stress and Lame coefficients are
inferred. Correlations involving the residual stress are found to be
long-ranged and governed by a universal parameter that also gives the mean
shear modulus.Comment: 5 page
Statistical physics of isotropic-genesis nematic elastomers: I. Structure and correlations at high temperatures
Isotropic-genesis nematic elastomers (IGNEs) are liquid crystalline polymers
(LCPs) that have been randomly, permanently cross-linked in the
high-temperature state so as to form an equilibrium random solid. Thus, instead
of being free to diffuse throughout the entire volume, as they would be in the
liquid state, the constituent LCPs in an IGNE are mobile only over a finite
length-scale controlled by the density of cross-links. We address the effects
that such network-induced localization have on the liquid-crystalline
characteristics of an IGNE, as probed via measurements made at high
temperatures. In contrast with the case of uncross-linked LCPs, for IGNEs these
characteristics are determined not only by thermal fluctuations but also by the
quenched disorder associated with the cross-link constraints. To study IGNEs,
we consider a microscopic model of dimer nematogens in which the dimers
interact via orientation-dependent excluded volume forces. The dimers are,
furthermore, randomly, permanently cross-linked via short Hookean springs, the
statistics of which we model by means of a Deam-Edwards type of distribution.
We show that at length-scales larger than the size of the nematogens this
approach leads to a recently proposed phenomenological Landau theory of IGNEs
[Lu et al., Phys. Rev. Lett. 108, 257803 (2012)], and hence predicts a regime
of short-ranged oscillatory spatial correlations in the nematic alignment, of
both thermal and glassy types. In addition, we consider two alternative
microscopic models of IGNEs: (i) a wormlike chain model of IGNEs that are
formed via the cross-linking of side-chain LCPs; and (ii) a jointed chain model
of IGNEs that are formed via the cross-linking of main-chain LCPs. At large
length-scales, both of these models give rise to liquid-crystalline
characteristics that are qualitatively in line with those predicted by the
dimer-and-springs model.Comment: 33 pages, 6 figures, 6 appendice
ArrayBridge: Interweaving declarative array processing with high-performance computing
Scientists are increasingly turning to datacenter-scale computers to produce
and analyze massive arrays. Despite decades of database research that extols
the virtues of declarative query processing, scientists still write, debug and
parallelize imperative HPC kernels even for the most mundane queries. This
impedance mismatch has been partly attributed to the cumbersome data loading
process; in response, the database community has proposed in situ mechanisms to
access data in scientific file formats. Scientists, however, desire more than a
passive access method that reads arrays from files.
This paper describes ArrayBridge, a bi-directional array view mechanism for
scientific file formats, that aims to make declarative array manipulations
interoperable with imperative file-centric analyses. Our prototype
implementation of ArrayBridge uses HDF5 as the underlying array storage library
and seamlessly integrates into the SciDB open-source array database system. In
addition to fast querying over external array objects, ArrayBridge produces
arrays in the HDF5 file format just as easily as it can read from it.
ArrayBridge also supports time travel queries from imperative kernels through
the unmodified HDF5 API, and automatically deduplicates between array versions
for space efficiency. Our extensive performance evaluation in NERSC, a
large-scale scientific computing facility, shows that ArrayBridge exhibits
statistically indistinguishable performance and I/O scalability to the native
SciDB storage engine.Comment: 12 pages, 13 figure
Asteroid (3200) Phaethon: colors, phase curve, limits on cometary activity and fragmentation
We report on a multi-observatory campaign to examine asteroid 3200 Phaethon
during its December 2017 close approach to Earth, in order to improve our
measurements of its fundamental parameters, and to search for surface
variations, cometary activity and fragmentation. The mean colors of Phaethon
are B-V = 0.702 +/- 0.004, V-R = 0.309 +/- 0.003, R-I = 0.266 +/- 0.004,
neutral to slightly blue, consistent with previous classifications of Phaethon
as a F-type or B-type asteroid. Variations in Phaethon's B-V colors (but not
V-R or R-I) with observer sub-latitude are seen and may be associated with
craters observed by the Arecibo radar. High cadence photometry over phases from
20 to 100 degrees allows a fit to the values of the HG photometric parameters;
H = 14.57 +/- 0.02, 13.63 +/- 0.02, 13.28 +/- 0.02, 13.07 +/- 0.02; G = 0.00
+/- 0.01, -0.09 +/- 0.01, -0.10 +/- 0.01, -0.08 +/- 0.01 in the BVRI filters
respectively; the negative G values are consistent with other observations of F
type asteroids. Light curve variations were seen that are also consistent with
concavities reported by Arecibo, indicative of large craters on Phaethon's
surface whose ejecta may be the source of the Geminid meteoroid stream. A
search for gas/dust production set an upper limit of 0.06 +/- 0.02 kg/s when
Phaethon was 1.449 AU from the Sun, and 0.2 +/- 0.1 kg/s at 1.067 AU. A search
for meter-class fragments accompanying Phaethon did not find any whose on-sky
motion was not also consistent with background main belt asteroids.Comment: Accepted by the Astronomical Journal, 15 pages, 8 figures, 1 animated
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Effects of annealing on microstructure and microstrength of metallurgical coke
Two metallurgical cokes were heat treated at 1673 K to 2273 K (1400 degrees celsius to 2000 degrees celsius) in a nitrogen atmosphere. The effect of heat treatment on the microstructure and microstrength of metallurgical cokes was characterized using X-ray diffraction, Raman spectroscopy, and ultramicroindentation. In the process of heat treatment, the microstructure of the metallurgical cokes transformed toward the graphite structure. Raman spectroscopy of reactive maceral-derived component (RMDC) and inert maceral-derived component (IMDC) indicated that the graphitisation degree of the RMDC was slightly lower than that of the IMDC in the original cokes; however graphitisation of the RMDC progressed faster than that of the IMDC during annealing, and became significantly higher after annealing at 2273 K (2000 degrees celsius). The microstrength of cokes was significantly degraded in the process of heat treatment. The microstrength of the RMDC was lower, and of its deterioration caused by heat treatment was more severe than IMDC. The degradation of the microstrength of cokes was attributed to their increased graphitisation degree during the heat treatment
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